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Sample records for alma senoidal sujeitas

  1. Exploring the Sun with ALMA

    Science.gov (United States)

    Bastian, T. S.; Bárta, M.; Brajša, R.; Chen, B.; Pontieu, B. D.; Gary, D. E.; Fleishman, G. D.; Hales, A. S.; Iwai, K.; Hudson, H.; Kim, S.; Kobelski, A.; Loukitcheva, M.; Shimojo, M.; Skokić, I.; Wedemeyer, S.; White, S. M.; Yan, Y.

    2018-03-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) Observatory opens a new window onto the Universe. The ability to perform continuum imaging and spectroscopy of astrophysical phenomena at millimetre and submillimetre wavelengths with unprecedented sensitivity opens up new avenues for the study of cosmology and the evolution of galaxies, the formation of stars and planets, and astrochemistry. ALMA also allows fundamentally new observations to be made of objects much closer to home, including the Sun. The Sun has long served as a touchstone for our understanding of astrophysical processes, from the nature of stellar interiors, to magnetic dynamos, non-radiative heating, stellar mass loss, and energetic phenomena such as solar flares. ALMA offers new insights into all of these processes.

  2. A Look Inside Hurricane Alma

    Science.gov (United States)

    2002-01-01

    Hurricane season in the eastern Pacific started off with a whimper late last month as Alma, a Category 2 hurricane, slowly made its way up the coast of Baja California, packing sustained winds of 110 miles per hour and gusts of 135 miles per hour. The above image of the hurricane was acquired on May 29, 2002, and displays the rainfall rates occurring within the storm. Click the image above to see an animated data visualization (3.8 MB) of the interior of Hurricane Alma. The images of the clouds seen at the beginning of the movie were retrieved from the National Oceanic and Atmospheric Association's (NOAA's) Geostationary Orbiting Environmental Satellite (GOES) network. As the movie continues, the clouds are peeled away to reveal an image of rainfall levels in the hurricane. The rainfall data were obtained by the Precipitation Radar aboard NASA's Tropical Rainfall Measuring Mission (TRMM) satellite. The Precipitation Radar bounces radio waves off of clouds to retrieve a reading of the number of large, rain-sized droplets within the clouds. Using these data, scientists can tell how much precipitation is occurring within and beneath a hurricane. In the movie, yellow denotes areas where 0.5 inches of rain is falling per hour, green denotes 1 inch per hour, and red denotes over 2 inches per hour. (Please note that high resolution still images of Hurricane Alma are available in the NASA Visible Earth in TIFF format.) Image and animation courtesy Lori Perkins, NASA Goddard Space Flight Center Scientific Visualization Studio

  3. Alma Tapia: the modern line

    Directory of Open Access Journals (Sweden)

    Carmen Gaitán Salinas

    2017-12-01

    Full Text Available Educated within institucionismo circles and member of one of the most relevant Spanish families at the beginning of the 20th century, Alma Tapia participated in the artistic scene through illustration, poster design and her involvement in the Madrid Lyceum Club Femenino. After the Spanish Civil War and the victory of general Franco, her political beliefs led her to exile in Mexico, where she continued working in the editorial field. She was an artist who contributed to the continuation and dissemination of the extensive and valuable cultural legacy developed in Spain during the first third of the 20th century.

  4. ALMA - the atacama large millimeter array

    Science.gov (United States)

    Wild, W.; Cunningham, C.

    The Atacama Large Millimeter Array (ALMA) is a major ground based project for millimeter and submillimeter astronomy to be realized during this decade. It comprises an array of 64 telescopes of 12 meter diameter, each equipped with 10 receivers bands covering the atmospheric windows from 30 GHz to 950 GHz. Baselines up to several kilometers will allow sub-arcsecond resolution. The ALMA array will be located on a high - altitude (5000 m) plateau in the Atacama Desert in Northern Chile. The project is a joint venture of Europe and North America (USA and Canada) with Japan intending to join later on. This contribution will give an overview of the ALMA project including its science capabilities, technical specifications and current status.

  5. First ALMA Transporter Ready for Challenging Duty

    Science.gov (United States)

    2008-07-01

    The first of two ALMA transporters -- unique vehicles designed to move high-tech radio-telescope antennas in the harsh, high-altitude environment of the Atacama Large Millimeter/submillimeter Array -- has been completed and passed its initial operational tests. The 130-ton machine moves on 28 wheels and will be able to transport a 115-ton antenna and set it down on a concrete pad within millimeters of a prescribed position. ALMA Transporter The ALMA Transporter on a Test Run CREDIT: ESO Click on image for high-resolution file (244 KB) The ALMA transporter rolled out of its hangar and underwent the tests at the Scheuerle Fahrzeugfabrik company site near Nuremberg, Germany. The machine is scheduled for delivery at the ALMA site in Chile by the end of 2007, and a second vehicle will follow about three months later. ALMA is a giant, international observatory under construction in the Atacama Desert of northern Chile at an elevation of 16,500 feet. Using at least 66 high-precision antennas, with the possibility of increasing the number in the future, ALMA will provide astronomers with an unprecedented ability to explore the Universe as seen at wavelengths of a few millimeters to less than a millimeter. By moving the antennas from configurations as compact as 150 meters to as wide as 15 kilometers, the system will provide a zoom-lens ability for scientists. "The ability to move antennas to reconfigure the array is vital to fulfilling ALMA's scientific mission. The operations plan calls for moving antennas on a daily basis to provide the flexibility that will be such a big part of ALMA's scientific value. That's why the transporters are so important and why this is such a significant milestone," said Adrian Russell, North American Project Manager for ALMA. "The ALMA antennas will be assembled and their functionality will be verified at a base camp, located at an altitude of 2900 meters (9500 feet) and the transporters will in a first step bring the telescopes up to the

  6. ESO and NSF Sign Agreement on ALMA

    Science.gov (United States)

    2003-02-01

    Green Light for World's Most Powerful Radio Observatory On February 25, 2003, the European Southern Observatory (ESO) and the US National Science Foundation (NSF) are signing a historic agreement to construct and operate the world's largest and most powerful radio telescope, operating at millimeter and sub-millimeter wavelength. The Director General of ESO, Dr. Catherine Cesarsky, and the Director of the NSF, Dr. Rita Colwell, act for their respective organizations. Known as the Atacama Large Millimeter Array (ALMA), the future facility will encompass sixty-four interconnected 12-meter antennae at a unique, high-altitude site at Chajnantor in the Atacama region of northern Chile. ALMA is a joint project between Europe and North America. In Europe, ESO is leading on behalf of its ten member countries and Spain. In North America, the NSF also acts for the National Research Council of Canada and executes the project through the National Radio Astronomy Observatory (NRAO) operated by Associated Universities, Inc. (AUI). The conclusion of the ESO-NSF Agreement now gives the final green light for the ALMA project. The total cost of approximately 650 million Euro (or US Dollars) is shared equally between the two partners. Dr. Cesarsky is excited: "This agreement signifies the start of a great project of contemporary astronomy and astrophysics. Representing Europe, and in collaboration with many laboratories and institutes on this continent, we together look forward towards wonderful research projects. With ALMA we may learn how the earliest galaxies in the Universe really looked like, to mention but one of the many eagerly awaited opportunities with this marvellous facility". "With this agreement, we usher in a new age of research in astronomy" says Dr. Colwell. "By working together in this truly global partnership, the international astronomy community will be able to ensure the research capabilities needed to meet the long-term demands of our scientific enterprise, and

  7. ALMA - the Atacama Large Millimeter Array

    NARCIS (Netherlands)

    Wild, W.; Cunningham, C.

    2002-01-01

    The Atacama Large Millimeter Array (ALMA) is a major ground based project for millimeter and submillimeter astronomy to be realized during this decade. It comprises an array of 64 telescopes of 12 meter diameter, each equipped with 10 receivers bands covering the atmospheric windows from 30 GHz to

  8. The ALMA Real Time Control System

    Science.gov (United States)

    Kern, Jeffrey S.; Juerges, Thomas A.; Marson, Ralph G.

    2009-01-01

    The Atacama Large Millimeter Array (ALMA) is a revolutionary millimeter and submillimeter array being developed on the Atacama plateau of northern Chile. An international partnership lead by NRAO, ESO, and NAOJ this powerful and flexible telescope will provide unprecedented observations of this relatively unexplored frequency range. The control subsystem for the Atacama Large Millimeter Array must coordinate the monitor and control of at least sixty six antennas (in four different styles), two correlators, and all of the ancillary equipment (samplers, local oscillators, front ends, etc.). This equipment will be spread over tens of kilometers and operated remotely. Operation of the array requires a robust, scalable, and maintainable real time control system. The real time control system is responsible for monitoring and control of any devices where there are fixed deadlines. Examples in the ALMA context are antenna pointing and fringe tracking. Traditionally the real time portion of a large software system is an intricate and error prone portion of the software. As a result the real time portion is very expensive in terms of effort expended both during construction and during maintenance phases of a project. The ALMA real time control system uses a Linux based real time operating system to interact with the hardware and the CORBA based ALMA Common Software to communicate in the distributed computing environment. Mixing the requirements of real time computing and the non-deterministic CORBA middleware has produced an interesting design. We discuss the architecture, design, and implementation of the ALMA real time control system. Highlight some lessons learned along the way, and justify our assertion that this should be the last large scale real time control system in radio astronomy.

  9. CURA MÉDICA DE ALMAS (CMA

    Directory of Open Access Journals (Sweden)

    Ancisar Restrepo Toro

    2001-01-01

    Full Text Available La «Cura médica de almas» tiene como objetivo señalar otra zona de aplicación de la Logoterapia, el acercamiento al hombre que sufre, al homo patiens, pero no ya a su sufrimiento en sí mismo sino a su humanidad. Si la Logoterapia, en su sentido más estricto, es la terapia indicada para las neurosis noógenas o en otros casos es complementaria de las psicoterapias, en el caso de la «Cura médica de almas» ya no es intervención terapéutica sino, específicamente, ejercicio de la humanidad del terapeuta en contacto con la humanidad de su paciente.

  10. Alma M. Karlin – in private

    Directory of Open Access Journals (Sweden)

    Maja Šučur

    2014-06-01

    Full Text Available The article presents the Slovenian writer and traveler, Alma M. Karlin, from two perspectives—the public and the private. The author begins with a summary of the most well-known facts of Alma Karlin's life: She describes her journey around the world, her motivation for writing literary works and travel logs, she places herself into the linguistic and political milieu and uncovers her contribution to the deconstruction of the role a woman was expected to perform in the early 20th century. In this text, the author exposes the previously secret or intentionally hidden elements of Karlin's privacy, for example her relationships with love and the physical. She also brings to light Karlin's relationships with men. However, the author focuses especially on the relationship between Alma Karlin and Thea Gamelin and the related speculations about Karlin's lesbianism, offering a new insight through the concept of the romantic friendship. The article raises the question whether the researching that ignores all the possible interpretations of Karlin’s life and identity has also become an act of heteronormativity.

  11. NRAO Welcomes Taiwan as a New North American ALMA Partner

    Science.gov (United States)

    2008-12-01

    The National Radio Astronomy Observatory (NRAO) has announced a formal agreement enabling Taiwanese astronomers to participate in the North American component of the international ALMA partnership, alongside American and Canadian astronomers. Taiwan's efforts will be led by the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA). ALMA, the Atacama Large Millimeter/submillimeter Array, is the most ambitious ground-based astronomical observatory in history. Currently under construction in Chile’s Atacama Desert at an altitude of 16,500 feet, it promises to revolutionize our understanding of the formation of planets, stars, and galaxies when it begins full science operations early in the next decade. The agreement, signed by the Taipei Economic and Cultural Representative Office and the American Institute in Taiwan, provides for approximately $20 million in ALMA construction funding through the National Science Council (NSC), Taiwan’s equivalent to the US National Science Foundation (NSF) and Canada's National Research Council (NRC), which have jointly funded North America's existing contribution to the international ALMA project. Activities under the agreement will include joint research projects, development projects, collaboration on construction, support of observatory operations and other forms of cooperation. Access to ALMA observing time will be shared, as will membership on advisory committees. “Taiwan is a world-class center for submillimeter-wavelength astronomical research, and we’re delighted that the ALMA project and all its future users will benefit from the resources and expertise that Taiwan’s deepening participation brings to this great, global endeavor,” said Dr. Fred Lo, NRAO's director. This new agreement increases and diversifies Taiwan’s Academia Sinica investment in ALMA beyond the levels achieved through its participation in the East Asian component of the ALMA partnership, which is led by the National Astronomical

  12. ALMA Achieves Major Milestone With Antenna-Link Success

    Science.gov (United States)

    2007-03-01

    The Atacama Large Millimeter/submillimeter Array (ALMA), an international telescope project, reached a major milestone on March 2, when two ALMA prototype antennas were first linked together as an integrated system to observe an astronomical object. The milestone achievement, technically termed "First Fringes," came at the ALMA Test Facility (ATF) on the grounds of the National Radio Astronomy Observatory's (NRAO) Very Large Array (VLA) radio telescope in New Mexico. NRAO is a facility of the National Science Foundation (NSF), managed by Associated Universities, Incorporated (AUI). AUI also is designated by NSF as the North American Executive for ALMA. ALMA Test Facility ALMA Test Facility, New Mexico: VertexRSI antenna, left; AEC antenna, right. CREDIT: Drew Medlin, NRAO/AUI/NSF Click on image for page of graphics and full information Faint radio waves emitted by the planet Saturn were collected by the two ALMA antennas, then processed by new, state-of-the-art electronics to turn the two antennas into a single, high-resolution telescope system, called an interferometer. Such pairs of antennas are the basic building blocks of multi-antenna imaging systems such as ALMA and the VLA. In such a system, each antenna is combined electronically with every other antenna to form a multitude of pairs. Each pair contributes unique information that is used to build a highly-detailed image of the astronomical object under observation. When completed in 2012, ALMA will have 66 antennas. The successful Saturn observation began at 7:13 p.m., U.S. Mountain Time Friday (0213 UTC Saturday). The planet's radio emissions at a frequency of 104 GigaHertz (GHz) were tracked by the ALMA system for more than an hour. "Our congratulations go to the dedicated team of scientists, engineers and technicians who produced this groundbreaking achievement for ALMA. Much hard work and many long hours went into this effort, and we appreciate it all. This team should be very proud today," said NRAO

  13. World-Wide Effort Bringing ALMA Telescope Into Reality

    Science.gov (United States)

    2008-02-01

    In the thin, dry air of northern Chile's Atacama Desert, at an altitude of 16,500 feet, an amazing new telescope system is taking shape, on schedule to provide the world's astronomers with unprecedented views of the origins of stars, galaxies, and planets. The Atacama Large Millimeter/submillimeter Array (ALMA) will open an entirely new "window" on the Universe, allowing scientists to unravel longstanding and important astronomical mysteries. ALMA Artist's Concept Artist's Concept of Completed ALMA CREDIT: ALMA/ESO/NRAO/NAOJ Click on image for high-resolution file (182 KB) "Most of the photons in the Universe are in the wavelength range that ALMA will receive, and ALMA will give us our first high-resolution views at these wavelengths. This will be a tremendous advancement for astronomy and open one of our science's last frontiers," Anneila Sargent, a Caltech professor and ALMA Board member, told the American Association for the Advancement of Science at its meeting in Boston, Mass. The millimeter and submillimeter wavelength range lies between what is traditionally considered radio waves and infrared waves. ALMA, a system using up to 66 high-precision dish antennas working together, will provide astronomers with dramatically greater sensitivity, the ability to detect faint objects, and resolving power, the ability to see fine detail, than has ever before been available in this range. "This ambitious project is the product of an international collaboration that spans the globe," Sargent said. "ALMA truly will enable transformational science and providing this capability has required a massive, world-wide effort," she added. The ALMA project is a partnership between Europe, Japan and North America in cooperation with the Republic of Chile. ALMA is funded in Europe by ESO, in Japan by the National Institutes of Natural Sciences in cooperation with the Academia Sinica in Taiwan and in North America by the U.S. National Science Foundation in cooperation with the

  14. Solar Prominence Modelling and Plasma Diagnostics at ALMA Wavelengths

    Science.gov (United States)

    Rodger, Andrew; Labrosse, Nicolas

    2017-09-01

    Our aim is to test potential solar prominence plasma diagnostics as obtained with the new solar capability of the Atacama Large Millimeter/submillimeter Array (ALMA). We investigate the thermal and plasma diagnostic potential of ALMA for solar prominences through the computation of brightness temperatures at ALMA wavelengths. The brightness temperature, for a chosen line of sight, is calculated using the densities of electrons, hydrogen, and helium obtained from a radiative transfer code under non-local thermodynamic equilibrium (non-LTE) conditions, as well as the input internal parameters of the prominence model in consideration. Two distinct sets of prominence models were used: isothermal-isobaric fine-structure threads, and large-scale structures with radially increasing temperature distributions representing the prominence-to-corona transition region. We compute brightness temperatures over the range of wavelengths in which ALMA is capable of observing (0.32 - 9.6 mm), however, we particularly focus on the bands available to solar observers in ALMA cycles 4 and 5, namely 2.6 - 3.6 mm (Band 3) and 1.1 - 1.4 mm (Band 6). We show how the computed brightness temperatures and optical thicknesses in our models vary with the plasma parameters (temperature and pressure) and the wavelength of observation. We then study how ALMA observables such as the ratio of brightness temperatures at two frequencies can be used to estimate the optical thickness and the emission measure for isothermal and non-isothermal prominences. From this study we conclude that for both sets of models, ALMA presents a strong thermal diagnostic capability, provided that the interpretation of observations is supported by the use of non-LTE simulation results.

  15. A segunda alma do partido dos trabalhadores

    Directory of Open Access Journals (Sweden)

    André Singer

    2010-12-01

    Full Text Available Os dois mandatos de Lula formaram a síntese contraditória das "duas almas" que hoje habitam o PT. Foi o fato de ter implementado, simultaneamente, políticas que beneficiam o capital e promovem a inclusão dos mais pobres, com uma melhora relativa na situação dos trabalhadores, que permitiu a convivência dos princípios estabelecidos em sua fundação, no colégio Sion em 1980, e as diretrizes do programa de governo apresentadas em 2002 na convenção do Anhembi, em São Paulo.Lula's presidency seem to have blended PT's two apparently contradictory "souls". By implementing policies that favor capital while at the same time foster the social inclusion of the poor, and that have also improved working class citizens' life standards, Lula has been able, as a president, to preserve the ideals that animated the party's foundation and the more pragmatic programme for government set out in 2002.

  16. ALMA nutator design and preliminary performances

    Science.gov (United States)

    Martin-Cocher, Pierre; Ford, John; Koch, Patrick M.; Ni, Chih-Wen; Chen, Wei-Long; Chen, Ming-Tang; Raffin, Philippe; Ong, Ching-Long; Ho, Paul T. P.; Symmes, Arthur H.

    2012-09-01

    We report the past two years of collaboration between the different actors on the ALMA nutator. Building on previous developments, the nutator has seen changes in much of the design. A high-modulus carbon fiber structure has been added on the back of the mirror in order to transfer the voice coils forces with less deformation, thus reducing delay problems due to flexing. The controller is now an off-the-shelf National Instrument NI-cRIO, and the amplifier a class D servo drive from Advanced Motion Controls, with high peak power able to drive the coils at 300 Volts DC. The stow mechanism has been totally redesigned to improve on the repeatability and precision of the stow position, which is also the reference for the 26 bits Heidenhain encoders. This also improves on the accuracy of the stow position with wind loading. Finally, the software, written largely with National Instrument's LabView, has been developed. We will discuss these changes and the preliminary performance achieved to date.

  17. The Soul of Lupus with ALMA (SOLA) Project Overview

    Science.gov (United States)

    Saito, M.; de Gregorio, I.; Team SOLA

    2015-12-01

    The SOLA (Soul of Lupus with ALMA) project is conducting comprehensive studies of the Lupus Molecular Clouds and their star formation processes. Our goal is to exploit ALMA and other facilities over a wide wavelength range to establish a prototypical low-mass star forming scenario based on the Lupus region. We focus mainly on 10-104 au scale physics, kinematics, density, and temperature, together with detailed modelling of radiative transfer. Our unique source catalog so far contains more than 700 sources at various evolutionary stages and we have obtained complementary data with Mopra, APEX, etc. In the poster, we will report the latest status of SOLA and the expected outcome in observing runs in the near future, including ALMA Cycle 3.

  18. η Carinae Baby Homunculus uncovered by ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Abraham, Zulema; Beaklini, Pedro P. B. [Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, R. do Matão 1226, Cidade Universitária, CEP 05508-900 São Paulo, SP (Brazil); Falceta-Gonçalves, Diego, E-mail: zulema.abraham@iag.usp.br [Escola de Artes, Ciências e Humanidades, Universidade de São Paulo, R. Arlindo Bettio 1000, 03828-000 São Paulo, SP (Brazil)

    2014-08-20

    We report observations of η Carinae obtained with ALMA in the continuum of 100, 230, 280, and 660 GHz in 2012 November, with a resolution that varied from 2.''88 to 0.''45 for the lower and higher frequencies, respectively. The source is not resolved, even at the highest frequency; its spectrum is characteristic of thermal bremsstrahlung of a compact source, but different from the spectrum of optically thin wind. The recombination lines H42α, He42α, H40α, He40α, H50β, H28α, He28α, H21α, and He21α were also detected, and their intensities reveal non-local thermodynamic equilibrium effects. We found that the line profiles could only be fit by an expanding shell of dense and ionized gas, which produces a slow shock in the surroundings of η Carinae. Combined with fittings to the continuum, we were able to constrain the shell size, radius, density, temperature, and velocity. The detection of the He recombination lines is compatible with the high-temperature gas and requires a high-energy ionizing photon flux, which must be provided by the companion star. The mass-loss rate and wind velocity, necessary to explain the formation of the shell, are compatible with an luminous blue variable eruption. The position, velocity, and physical parameters of the shell coincide with those of the Weigelt blobs. The dynamics found for the expanding shell correspond to matter ejected by η Carinae in 1941 in an event similar to that which formed the Little Homunculus; for that reason, we called the new ejecta the 'Baby Homunculus'.

  19. Por mi alma subiré a Dios. El concepto de alma de san Agustín de Hipona

    OpenAIRE

    Saeteros Pérez, Tamara

    2013-01-01

    El presente artículo pretende recoger las claves fundamentales de la doctrina sobre el alma de san Agustín de Hipona. Magna natura et magna quaestio est (Hipona De; trad. 1968; 14; 4; 6); puesto que ocupará durante toda su vida el pensamiento y las obras del santo obispo. Buscar su propia alma; adentrarse en su santuario; descubrir la imagen de Dios en ella; su bondad; su grandeza; su vida para volverla luego a Dios; su origen y meta de todos sus esfuerzos. Tal es el itinerario que nos traza...

  20. CORBA-based Common Software for the ALMA project

    Science.gov (United States)

    Chiozzi, Gianluca; Gustafsson, Birger; Jeram, Bogdan; Plesko, Mark; Sekoranja, Matej; Tkacik, Gasper; Zagar, K.

    2002-12-01

    The Atacama Large Millimeter Array (ALMA) is a joint project between astronomical organizations in Europe and North America. ALMA will consist of at least 64 12-meter antennas operating in the millimeter and sub-millimeter range, with baselines up to 14 km. It will be located at an altitude above 5000m in the Chilean Atacama desert. The ALMA Common Software (ACS) provides a software infrastructure common to all partners and consists of a documented collection of common patterns and of components that implement those patterns. The heart of ACS is an object model based on Distributed Objects (DOs), implemented as CORBA objects. The teams responsible for the control system development use DOs as the basis for components and devices such as an antenna mount control. ACS provides common CORBA-based services such as logging, error and alarm management, configuration database and lifecycle management. A code generator creates a Java Bean for each DO. Programmers can write Java client applications by connecting those Beans with data-manipulation and visualization Beans. ACS is based on the experience gained in the astronomical and particle accelerator domains, and reuses and extends proven concepts and components. Although designed for ALMA, ACS can be used in other new control systems, since it implements proven design patterns using state of the art, stable and reliable technology. This paper presents the architecture of ACS and its status, detailing the object model and major services.

  1. Design and evaluation of ALMA band 9 quasioptical system

    NARCIS (Netherlands)

    Baryshev, A.; Carter, M.; Jellema, W.; Hesper, R.

    2004-01-01

    The Atacama Large Millimeter Array (ALMA) project requires the development of reliable quasi-optical systems with requirements similar to the ones in space. The operating condition for optical elements of higher frequency channels are similar to the conditions in spacecraft, since these elements are

  2. The 2014 ALMA Long Baseline Campaign : An Overview

    NARCIS (Netherlands)

    ALMA Partnership, [Unknown; Fomalont, E. B.; Vlahakis, C.; Corder, S.; Remijan, A.; Barkats, D.; Lucas, R.; Hunter, T. R.; Brogan, C. L.; Asaki, Y.; Matsushita, S.; Dent, W. R. F.; Hills, R. E.; Phillips, N.; Richards, A. M. S.; Cox, P.; Amestica, R.; Broguiere, D.; Cotton, W.; Hales, A. S.; Hiriart, R.; Hirota, A.; Hodge, J. A.; Impellizzeri, C. M. V.; Kern, J.; Kneissl, R.; Liuzzo, E.; Marcelino, N.; Marson, R.; Mignano, A.; Nakanishi, K.; Nikolic, B.; Perez, J. E.; Pérez, L. M.; Toledo, I.; Aladro, R.; Butler, B.; Cortes, J.; Cortes, P.; Dhawan, V.; Di Francesco, J.; Espada, D.; Galarza, F.; Garcia-Appadoo, D.; Guzman-Ramirez, L.; Humphreys, E. M.; Jung, T.; Kameno, S.; Laing, R. A.; Leon, S.; Mangum, J.; Marconi, G.; Nagai, H.; Nyman, L.-A.; Radiszcz, M.; Rodón, J. A.; Sawada, T.; Takahashi, S.; Tilanus, R. P. J.; van Kempen, T.; Vila Vilaro, B.; Watson, L. C.; Wiklind, T.; Gueth, F.; Tatematsu, K.; Wootten, A.; Castro-Carrizo, A.; Chapillon, E.; Dumas, G.; de Gregorio-Monsalvo, I.; Francke, H.; Gallardo, J.; Garcia, J.; Gonzalez, S.; Hibbard, J. E.; Hill, T.; Kaminski, T.; Karim, A.; Krips, M.; Kurono, Y.; Lopez, C.; Martin, S.; Maud, L.; Morales, F.; Pietu, V.; Plarre, K.; Schieven, G.; Testi, L.; Videla, L.; Villard, E.; Whyborn, N.; Alves, F.; Andreani, P.; Avison, A.; Barta, M.; Bedosti, F.; Bendo, G. J.; Bertoldi, F.; Bethermin, M.; Biggs, A.; Boissier, J.; Brand, J.; Burkutean, S.; Casasola, V.; Conway, J.; Cortese, L.; Dabrowski, B.; Davis, T. A.; Diaz Trigo, M.; Fontani, F.; Franco-Hernandez, R.; Fuller, G.; Galvan Madrid, R.; Giannetti, A.; Ginsburg, A.; Graves, S. F.; Hatziminaoglou, E.; Hogerheijde, M.; Jachym, P.; Jimenez Serra, I.; Karlicky, M.; Klaasen, P.; Kraus, M.; Kunneriath, D.; Lagos, C.; Longmore, S.; Leurini, S.; Maercker, M.; Magnelli, B.; Marti Vidal, I.; Massardi, M.; Maury, A.; Muehle, S.; Muller, S.; Muxlow, T.; O’Gorman, E.; Paladino, R.; Petry, D.; Pineda, J.; Randall, S.; Richer, J. S.; Rossetti, A.; Rushton, A.; Rygl, K.; Sanchez Monge, A.; Schaaf, R.; Schilke, P.; Stanke, T.; Schmalzl, M.; Stoehr, F.; Urban, S.; van Kampen, E.; Vlemmings, W.; Wang, K.; Wild, W.; Yang, Y.; Iguchi, S.; Hasegawa, T.; Saito, M.; Inatani, J.; Mizuno, N.; Asayama, S.; Kosugi, G.; Morita, K.-I.; Chiba, K.; Kawashima, S.; Okumura, S. K.; Ohashi, N.; Ogasawara, R.; Sakamoto, S.; Noguchi, T.; Huang, Y.-D.; Liu, S.-Y.; Kemper, F.; Koch, P. M.; Chen, M.-T.; Chikada, Y.; Hiramatsu, M.; Iono, D.; Shimojo, M.; Komugi, S.; Kim, J.; Lyo, A.-R.; Muller, E.; Herrera, C.; Miura, R. E.; Ueda, J.; Chibueze, J.; Su, Y.-N.; Trejo-Cruz, A.; Wang, K.-S.; Kiuchi, H.; Ukita, N.; Sugimoto, M.; Kawabe, R.; Hayashi, M.; Miyama, S.; Ho, P. T. P.; Kaifu, N.; Ishiguro, M.; Beasley, A. J.; Bhatnagar, S.; Braatz, J. A., III; Brisbin, D. G.; Brunetti, N.; Carilli, C.; Crossley, J. H.; D’Addario, L.; Donovan Meyer, J. L.; Emerson, D. T.; Evans, A. S.; Fisher, P.; Golap, K.; Griffith, D. M.; Hale, A. E.; Halstead, D.; Hardy, E. J.; Hatz, M. C.; Holdaway, M.; Indebetouw, R.; Jewell, P. R.; Kepley, A. A.; Kim, D.-C.; Lacy, M. D.; Leroy, A. K.; Liszt, H. S.; Lonsdale, C. J.; Matthews, B.; McKinnon, M.; Mason, B. S.; Moellenbrock, G.; Moullet, A.; Myers, S. T.; Ott, J.; Peck, A. B.; Pisano, J.; Radford, S. J. E.; Randolph, W. T.; Rao Venkata, U.; Rawlings, M. G.; Rosen, R.; Schnee, S. L.; Scott, K. S.; Sharp, N. K.; Sheth, K.; Simon, R. S.; Tsutsumi, T.; Wood, S. J.

    2015-01-01

    A major goal of the Atacama Large Millimeter/submillimeter Array (ALMA) is to make accurate images with resolutions of tens of milliarcseconds, which at submillimeter (submm) wavelengths requires baselines up to ∼15 km. To develop and test this capability, a Long Baseline Campaign (LBC) was carried

  3. Alma-0: an imperative language that supports declarative programming

    NARCIS (Netherlands)

    K.R. Apt (Krzysztof); J. Brunekreef; V. Partinton; A. Schaerf

    1997-01-01

    textabstractWe describe here an implemented small programming language, called Alma, that augments the expressive power of imperative programming by a limited number of features inspired by the logic programming paradigm. These additions encourage declarative programming and make it a more

  4. ALMA to Help Solving Acute Mountain Sickness Mystery

    Science.gov (United States)

    2007-04-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) astronomical project will not only enlarge our knowledge of the vast Universe beyond the imaginable. It will also help scientists learn more about the human body. Located 5000m above sea level, in the Chilean Atacama desert, ALMA is the highest site for ground-based astronomy. This property will be put to good use for academic institutions in Chile and in Europe in order to study the human response to extreme altitude conditions. During a ceremony held on 2 April in Antofagasta, the largest town close to ESO's Very Large Telescope, representatives from ALMA, ESO and the University of Antofagasta have officially launched a collaborative agreement that also involves the University of Chile and the University of Copenhagen (Denmark). The newly established cooperation aims at contributing to the promotion of teaching, scientific research, and the expansion of altitude physiology and medicine or other related areas considered appropriate. ESO PR Photo 20/07 ESO PR Photo 20/07 Working at 5000 metres "An increasing number of people are periodically exposed to brisk changes in altitude, and not only for astronomical research," said Jacques Lassalle, the ALMA Safety Manager. "Short stays at high altitude alternate with short stays at sea level but the corresponding shifts are very often established by agreement, and not based on scientific arguments. With this project, we aim at improving our knowledge and procedures in order to protect the long term health of the operators, engineers, and scientists as well as ALMA visitors of all ages and all physical conditions," he added. Around the world, a large number of people systematically commute between sea level and high altitude, for example when working in mountainous mines. This poses stringent conditions that may affect health, wellbeing and working performance. Some of the factors in question are the shift work regime, the perturbation of circadian rhythms, fatigue

  5. Fideísmo y racionalismo en las tres potencias del alma

    Directory of Open Access Journals (Sweden)

    José Andrés Calvo Rodríguez

    2004-12-01

    Full Text Available Dentro de la gnoseología luliana, las tres potencias del alma racional (Voluntad, Memoria y Entendimiento adquieren una especial importancia por ser los instrumentos del alma que permiten el acceso y el conocimiento del amor divino. A este respecto escribe Cruz Hernández: «Las potencias del alma, además, tanto por su naturaleza como por su actividad, reflejan las virtudes divinas; y, de un modo eminente, la Trinidad personal».1 De esta manera, no hay mejor espejo de Dios en el hombre que el alma, donde reside la presencia divina. Por esto, el Libro de amigo y Amado, considerando la reiterativa presencia de las tres potencias del alma que presenta, simplemente propone un viaje errático por el interior del alma humana en busca de Dios y, en definitiva, en busca del propio yo del místico.

  6. Design and Characterization of the ALMA Band 5 Vacuum Window

    Science.gov (United States)

    Schroder, Arne; Murk, Axel; Yagoubov, Pavel; Patt, Ferdinand

    2016-01-01

    This paper summarizes the electromagnetic design process of the vacuum window for the Atacama Large Millimeter/sub-millimeter Array (ALMA) Band 5 (163-211 GHz). We have carried out investigations by means of numerical simulations as well as reflection and transmission measurements. Simulations were performed using the finite element method, an efficient quasi-analytical technique, and rigorous coupled-wave analysis. We used an injection-molded vacuum window prototype as a starting point of the design process and investigated deterioration in the electromagnetic performance caused by different types of manufacturing artifacts. Following these analyses, an optimization of the window has been performed based on simulations. We measured the reflectivity and transmittance of the newly designed window and this paper demonstrates that the optimized window exhibits a return loss better than -20 dB, as required by the ALMA specifications.

  7. New Inspiring Planetarium Show Introduces ALMA to the Public

    Science.gov (United States)

    2009-03-01

    As part of a wide range of education and public outreach activities for the International Year of Astronomy 2009 (IYA2009), ESO, together with the Association of French Language Planetariums (APLF), has produced a 30-minute planetarium show, In Search of our Cosmic Origins. It is centred on the global ground-based astronomical Atacama Large Millimeter/submillimeter Array (ALMA) project and represents a unique chance for planetariums to be associated with the IYA2009. ESO PR Photo 09a/09 Logo of the ALMA Planetarium Show ESO PR Photo 09b/09 Galileo's first observations with a telescope ESO PR Photo 09c/09 The ALMA Observatory ESO PR Photo 09d/09 The Milky Way band ESO PR Video 09a/09 Trailer in English ALMA is the leading telescope for observing the cool Universe -- the relic radiation of the Big Bang, and the molecular gas and dust that constitute the building blocks of stars, planetary systems, galaxies and life itself. It is currently being built in the extremely arid environment of the Chajnantor plateau, at 5000 metres altitude in the Chilean Andes, and will start scientific observations around 2011. ALMA, the largest current astronomical project, is a revolutionary telescope, comprising a state-of-the-art array of 66 giant 12-metre and 7-metre diameter antennas observing at millimetre and submillimetre wavelengths. In Search of our Cosmic Origins highlights the unprecedented window on the Universe that this facility will open for astronomers. "The show gives viewers a fascinating tour of the highest observatory on Earth, and takes them from there out into our Milky Way, and beyond," says Douglas Pierce-Price, the ALMA Public Information Officer at ESO. Edited by world fulldome experts Mirage3D, the emphasis of the new planetarium show is on the incomparable scientific adventure of the ALMA project. A young female astronomer guides the audience through a story that includes unique animations and footage, leading the viewer from the first observations by Galileo

  8. A psicopatologia como uma experiência da alma

    OpenAIRE

    Zanoni,Anna Paula; Serbena,Carlos Augusto

    2011-01-01

    Este trabalho teórico apresenta a visão do psicólogo arquetípico James Hillman sobre a psicopatologia. Ele defende que "patologizar" é um movimento da psique válido, necessário e autêntico, que permite um encontro com a alma e com os sentidos e que deve ser compreendido metaforicamente. Sua visão se contrapõe ao modelo médico e nominalista dominante, que tem uma visão literal da psicopatologia e que acaba por afastá-la dos sentidos, da alma e do próprio sujeito. A crítica maior de Hillman é s...

  9. A psicopatologia como uma experiência da alma

    Directory of Open Access Journals (Sweden)

    Anna Paula Zanoni

    2011-09-01

    Full Text Available Este trabalho teórico apresenta a visão do psicólogo arquetípico James Hillman sobre a psicopatologia. Ele defende que "patologizar" é um movimento da psique válido, necessário e autêntico, que permite um encontro com a alma e com os sentidos e que deve ser compreendido metaforicamente. Sua visão se contrapõe ao modelo médico e nominalista dominante, que tem uma visão literal da psicopatologia e que acaba por afastá-la dos sentidos, da alma e do próprio sujeito. A crítica maior de Hillman é sobre a relação literal da psicologia com as palavras e termos psicopatológicos.

  10. Towards a dynamical scheduler for ALMA: a science - software collaboration

    Science.gov (United States)

    Avarias, Jorge; Toledo, Ignacio; Espada, Daniel; Hibbard, John; Nyman, Lars-Ake; Hiriart, Rafael

    2016-07-01

    State-of-the art astronomical facilities are costly to build and operate, hence it is essential that these facilities must be operated as much efficiently as possible, trying to maximize the scientific output and at the same time minimizing overhead times. Over the latest decades the scheduling problem has drawn attention of research because new facilities have been demonstrated that is unfeasible to try to schedule observations manually, due the complexity to satisfy the astronomical and instrumental constraints and the number of scientific proposals to be reviewed and evaluated in near real-time. In addition, the dynamic nature of some constraints make this problem even more difficult. The Atacama Large Millimeter/submillimeter Array (ALMA) is a major collaboration effort between European (ESO), North American (NRAO) and East Asian countries (NAOJ), under operations on the Chilean Chajnantor plateau, at 5.000 meters of altitude. During normal operations at least two independent arrays are available, aiming to achieve different types of science. Since ALMA does not observe in the visible spectrum, observations are not limited to night time only, thus a 24/7 operation with little downtime as possible is expected when full operations state will have been reached. However, during preliminary operations (early-science) ALMA has been operated on tied schedules using around half of the whole day-time to conduct scientific observations. The purpose of this paper is to explain how the observation scheduling and its optimization is done within ALMA, giving details about the problem complexity, its similarities and differences with traditional scheduling problems found in the literature. The paper delves into the current recommendation system implementation and the difficulties found during the road to its deployment in production.

  11. ALMA and VLA observations of the HD 141569 system

    Science.gov (United States)

    White, Jacob Aaron; Boley, A. C.; MacGregor, M. A.; Hughes, A. M.; Wilner, D. J.

    2018-03-01

    We present VLA 9 mm (33 GHz) and archival ALMA 2.9 mm (103 GHz) observations of the HD 141569 system. The VLA observations achieve a resolution of 0.25 arcsec (˜28 au) and a sensitivity of 4.7 μJy beam- 1. We find (1) a 52 ± 5 μJy point source at the location of HD 141569A that shows potential variability, (2) the detected flux is contained within the SED-inferred central clearing of the disc meaning the spectral index of the dust disc is steeper than previously inferred, and (3) the M dwarf companions are also detected and variable. Previous lower resolution VLA observations (semester 14A) found a higher flux density, interpreted as solely dust emission. When combined with ALMA observations, the VLA 14A observations suggested the spectral index, and grain size distribution of HD 141569's disc was shallow and an outlier among debris systems. Using archival ALMA observations of HD 141569 at 0.87 and 2.9 mm, we find a dust spectral index of αmm = 1.81 ± 0.20. The VLA 16A flux corresponds to a brightness temperature of ˜5 × 106 K, suggesting strong non-disc emission is affecting the inferred grain properties. The VLA 16A flux density of the M2V companion HD 141569B is 149 ± 9 μJy, corresponding to a brightness temperature of ˜2 × 108 K and suggesting significant stellar variability when compared to the VLA14A observations, which are smaller by a factor of ˜6.

  12. ALMA suggests outflows in z ˜ 5.5 galaxies

    Science.gov (United States)

    Gallerani, S.; Pallottini, A.; Feruglio, C.; Ferrara, A.; Maiolino, R.; Vallini, L.; Riechers, D. A.; Pavesi, R.

    2018-01-01

    We present the first attempt to detect outflows from galaxies approaching the Epoch of Reionization (EoR) using a sample of nine star-forming (SFR = 31 ± 20 M⊙ yr- 1) z ∼ 5.5 galaxies for which the [C II]158 μm line has been previously obtained with Atacama Large Millimeter Array (ALMA). We first fit each line with a Gaussian function and compute the residuals by subtracting the best-fitting model from the data. We combine the residuals of all sample galaxies and find that the total signal is characterized by a flux excess of ∼0.5 mJy extended over ∼1000 km s-1. Although we cannot exclude that part of this signal is due to emission from faint satellite galaxies, we show that the most probable explanation for the detected flux excess is the presence of broad wings in the [C II] lines, signatures of starburst-driven outflows. We infer an average outflow rate of \\dot{M}=54± 23 M_{⊙} yr^{-1}, providing a loading factor η =\\dot{M}/SFR=1.7± 1.3 in agreement with observed local starbursts. Our interpretation is consistent with outcomes from zoomed hydrosimulations of Dahlia, a z ∼ 6 galaxy (SFR˜ 100 M_{⊙} yr^{-1}), whose feedback-regulated star formation results into an outflow rate \\dot{M}˜ 30 M_{⊙} yr^{-1}. The quality of the ALMA data is not sufficient for a detailed analysis of the [C II] line profile in individual galaxies. Nevertheless, our results suggest that starburst-driven outflows are in place in the EoR and provide useful indications for future ALMA campaigns. Deeper observations of the [C II] line in this sample are required to better characterize feedback at high-z and to understand the role of outflows in shaping early galaxy formation.

  13. Breve historia del alma en la antigüedad

    OpenAIRE

    Fructuoso, Josa

    2006-01-01

    La psicología como ciencia se erige sobre un concepto tan poco científico como el “alma”, un concepto fundamental en el pensamiento occidental y que, desde su categoría de mito, se inserta en la filosofía, recorriéndola a lo largo de toda su historia. En sus orígenes prefilosóficos y homéricos, el mito del alma es aún un concepto emergente y disperso que, antes de pasar a convertirse en el principio de inmortalidad atrapado en la cárcel mortal del cuerpo, propio de la corrie...

  14. Modelo conceitual para projetos de instalações produtivas sujeitas à Vigilância Sanitária / Conceptual model for production facilities projects subject to Sanitary Surveillance

    Directory of Open Access Journals (Sweden)

    Marcelo Battesini

    2014-08-01

    Full Text Available O projeto de instalações produtivas objeto da ação de Vigilância Sanitária é uma atividade complexa e multidisciplinar que deve resultar em arranjos espaciais capazes de otimizar a obtenção de produtos e atender à regulação sanitária. A linguagem utilizada na legisla-ção sanitária dificulta sua compreensão por projetistas, prejudicando o entendimento da relação direta entre o risco sanitário, as instalações e os fluxos por elas condicionados. O objetivo do artigo é propor um Modelo Conceitual para projetos de Instalações Produtivas sujeitas à Vigilância Sanitária (MCIP-VISA. A coleta de dados ocorrida durante o processo de trabalho participativo e multidisciplinar no nível estadual da VISA, no RS, no período de 2000 a 2010, caracterizam a natureza aplicada e a abordagem qualitativa utilizada. Como resultados são apresentados uma sistematização dos requisitos legais para instalações, as diferentes formas de compor os espaços, os fluxos e o sequenciamento de processos, e as implicações práticas da utilização do modelo no projeto e avaliação de instalações. A aplicação do MCIP-VISA em situações reais demonstrou não haver incompatibilidade entre projetar instalações que minimizem os riscos sanitários e simultaneamente otimizem a produção. A demanda legal pela aprovação dos projetos de instalações pela VISA se mos-trou um momento oportuno à reflexão sobre o planejamento de infraestruturas físicas capazes de viabilizar o cumprimento das Boas Práticas de Fabricação. ------------------------------------------------------------------------ The design of production facilities subject to Sanitary Surveillance is a complex and multi-disciplinary activity that should result in spatial arrangements that optimize the products obtainment and meet the sanitary regulation. The language used in health legislation diffi-cult its understanding by designers, hindering the understanding of the direct

  15. La ciencia del alma en IBN Bayya (Avempace

    Directory of Open Access Journals (Sweden)

    Lomba, Joaquín

    2007-01-01

    Full Text Available El objetivo de este trabajo es la interpretación de del más importante aspecto de la filosofía de Ibn Bayya (Avempace a base de la lectura de su Kitab al nafs, primer comentario del De anima de Aristóteles en Occidente. Este estudio sobre el alma es, para Avempace, constituye la principal ciencia porque sin el análisis de la propia alma es imposible conocer el resto de las ciencias y del mundo. Este autor, en todas sus obras encentra el ideal del filósofo y del hombre sabio, sobre todo, en la progresiva desmaterialización de toda su vida. Este objetivo se obtiene mediante el transcendeer de tres formas de vida, concretamente, las formas materiales, el primer nivel espiritual y, por fin, el segundo nivel espiritual. La culminación de este itinerario es alcanzar el segundo nivel espiritual, concretamente, la unión con el Intelecto Agente mediante un misticismo espiritual o «amor Dei intellectualis». Los materiales básicos de esta filosofía están conteniddos en este comentario al aristotélico al De anima

  16. ALMA BAND 8 CONTINUUM EMISSION FROM ORION SOURCE I

    Energy Technology Data Exchange (ETDEWEB)

    Hirota, Tomoya; Matsumoto, Naoko [Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka-shi, Tokyo 181-8588 (Japan); Machida, Masahiro N.; Matsushita, Yuko [Department of Earth and Planetary Sciences, Faculty of Sciences, Kyushu University, Motooka 744, Nishi-ku, Fukuoka-shi, Fukuoka 819-0395 (Japan); Motogi, Kazuhito; Honma, Mareki [Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, Hoshigaoka2-12, Mizusawa-ku, Oshu-shi, Iwate 023-0861 (Japan); Kim, Mi Kyoung [Korea Astronomy and Space Science Institute, Hwaam-dong 61-1, Yuseong-gu, Daejeon, 305-348 (Korea, Republic of); Burns, Ross A., E-mail: tomoya.hirota@nao.ac.jp [Joint Institute for VLBI in Europe, Postbus 2, 7990 AA, Dwingeloo (Netherlands)

    2016-12-20

    We have measured continuum flux densities of a high-mass protostar candidate, a radio source I in the Orion KL region (Orion Source I) using the Atacama Large Millimeter/Submillimeter Array (ALMA) at band 8 with an angular resolution of 0.″1. The continuum emission at 430, 460, and 490 GHz associated with Source I shows an elongated structure along the northwest–southeast direction perpendicular to the so-called low-velocity bipolar outflow. The deconvolved size of the continuum source, 90 au × 20 au, is consistent with those reported previously at other millimeter/submillimeter wavelengths. The flux density can be well fitted to the optically thick blackbody spectral energy distribution, and the brightness temperature is evaluated to be 700–800 K. It is much lower than that in the case of proton–electron or H{sup −} free–free radiations. Our data are consistent with the latest ALMA results by Plambeck and Wright, in which the continuum emission was proposed to arise from the edge-on circumstellar disk via thermal dust emission, unless the continuum source consists of an unresolved structure with a smaller beam filling factor.

  17. Business Intelligence Applied to the ALMA Software Integration Process

    Science.gov (United States)

    Zambrano, M.; Recabarren, C.; González, V.; Hoffstadt, A.; Soto, R.; Shen, T.-C.

    2012-09-01

    Software quality assurance and planning of an astronomy project is a complex task, specially if it is a distributed collaborative project such as ALMA, where the development centers are spread across the globe. When you execute a software project there is much valuable information about this process itself that you might be able to collect. One of the ways you can receive this input is via an issue tracking system that will gather the problem reports relative to software bugs captured during the testing of the software, during the integration of the different components or even worst, problems occurred during production time. Usually, there is little time spent on analyzing them but with some multidimensional processing you can extract valuable information from them and it might help you on the long term planning and resources allocation. We present an analysis of the information collected at ALMA from a collection of key unbiased indicators. We describe here the extraction, transformation and load process and how the data was processed. The main goal is to assess a software process and get insights from this information.

  18. Violence in Teoría del alma china

    Directory of Open Access Journals (Sweden)

    Victor Hugo Martinez Bravo

    2015-12-01

    Full Text Available El propósito de este artículo es analizar la función que desempeña la violencia (violencia individual, violencia sistémica en Teoría del alma china, un texto híbrido que se inserta en una tradición narrativa caracterizada, tanto por conceder un valor central a la mordacidad, criticar al poder y la violencia de Estado, como por expresar un desprecio por el reduccionismo al que comúnmente conduce el concepto “literatura nacional” y un asco por la noción de “patria”. En Teoría del alma china hay una influencia directa de la figura de Karl Kraus, de La colonia penitenciaria de Kafka, de Trastorno de Bernhard, de También los enanos empezaron pequeños de Herzog, y posiblemente de El matadero de Esteban Echeverría. Todas estas obras influyen en la configuración una poética ambivalente en el texto de Aguilera con respecto a la violencia: por un lado, se presenta una violencia politizada, contra el sistema, y por otro, una violencia “estetizada”.

  19. Solar research with ALMA: Czech node of European ARC as your user-support infrastructure

    Science.gov (United States)

    Bárta, M.; Skokić, I.; Brajša, R.; Czech ARC Node Team

    2017-08-01

    ALMA (Atacama Large Millimeter/sub-millimeter Array) is by far the largest project of current ground-based observational facilities in astronomy and astrophysics. It is built and operated in the world-wide cooperation (ESO, NRAO, NAOJ) at altitude of 5000m in the desert of Atacama, Chile. Because of its unprecedented capabilities, ALMA is considered as a cutting-edge research device in astrophysics with potential for many breakthrough discoveries in the next decade and beyond. In spite it is not exclusively solar-research dedicated instrument, science observations of the Sun are now possible and has recently started in the observing Cycle 4 (2016-2017). In order to facilitate user access to this top-class, but at the same moment very complicated device to researchers lacking technical expertise, a network of three ALMA Regional Centers (ARCs) has been formed in Europe, North America, and East Asia as a user-support infrastructure and interface between the observatory and users community. After short introduction to ALMA the roles of ARCs and hint how to utilize their services will be presented, with emphasis to the specific (and in Europe unique) mission of the Czech ARC node in solar research with ALMA. Finally, peculiarities of solar observations that demanded the development of the specific Solar ALMA Observing Modes will be discussed and the results of Commissioning and Science Verification observing campaigns (solar ALMA maps) will be shown.

  20. Astronomers Break Ground on Atacama Large Millimeter Array (ALMA) - World's Largest Millimeter Wavelength Telescope

    Science.gov (United States)

    2003-11-01

    Scientists and dignitaries from Europe, North America and Chile are breaking ground today (Thursday, November 6, 2003) on what will be the world's largest, most sensitive radio telescope operating at millimeter wavelengths . ALMA - the "Atacama Large Millimeter Array" - will be a single instrument composed of 64 high-precision antennas located in the II Region of Chile, in the District of San Pedro de Atacama, at the Chajnantor altiplano, 5,000 metres above sea level. ALMA 's primary function will be to observe and image with unprecedented clarity the enigmatic cold regions of the Universe, which are optically dark, yet shine brightly in the millimetre portion of the electromagnetic spectrum. The Atacama Large Millimeter Array (ALMA) is an international astronomy facility. ALMA is an equal partnership between Europe and North America, in cooperation with the Republic of Chile, and is funded in North America by the U.S. National Science Foundation (NSF) in cooperation with the National Research Council of Canada (NRC), and in Europe by the European Southern Observatory (ESO) and Spain. ALMA construction and operations are led on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc. (AUI), and on behalf of Europe by ESO. " ALMA will be a giant leap forward for our studies of this relatively little explored spectral window towards the Universe" , said Dr. Catherine Cesarsky , Director General of ESO. "With ESO leading the European part of this ambitious and forward-looking project, the impact of ALMA will be felt in wide circles on our continent. Together with our partners in North America and Chile, we are all looking forward to the truly outstanding opportunities that will be offered by ALMA , also to young scientists and engineers" . " The U.S. National Science Foundation joins today with our North American partner, Canada, and with the European Southern Observatory, Spain, and Chile to prepare

  1. Molecular Gas in Disks around Young Stars with ALMA

    Science.gov (United States)

    Hughes, A. Meredith; Factor, Samuel; Lieman-Sifry, Jesse; Flaherty, Kevin; Daley, Cail; Mann, Rita; Roberge, Aki; Di Francesco, James; Williams, Jonathan; Ricci, Luca; Matthews, Brenda; Bally, John; Johnstone, Doug; Kospal, Agnes; Moor, Attila; Kamp, Inga; Wilner, David; Andrews, Sean; Kastner, Joel H.; Abraham, Peter

    2018-01-01

    Molecular gas is a critical component of the planet formation process. In this poster, we present two analyses of the molecular gas component of circumstellar disks at extremes (young, old) of the pre-main sequence phase.(1) We characterize the molecular gas content of the disk around d216-0939, a pre-main sequence star in the Orion Nebula Cluster, using ALMA observations of CO(3-2), HCO+(4-3), and HCN(4-3) observed at 0.5" resolution. We model the density and temperature structure of the disk, returning abundances generally consistent with chemical modeling of protoplanetary disks, and obtain a dynamical mass measurement of the central star of 2.2+/-0.4 M_sun, which is inconsistent with the previously determined spectral type of K5. We also report the detection of a spatially unresolved high-velocity blue-shifted excess emission feature with a measurable position offset from the central star, consistent with an object in Keplerian orbit at 60+/-20 au. The feature is due to a local temperature and/or density enhancement consistent with either a hydrodynamic vortex or the expected signature of the envelope of a forming protoplanet within the disk, providing evidence that planet formation is ongoing within this massive and relatively isolated Orion proplyd. This work is published in Factor et al. (2017). (2) We present ~0.4" resolution images of CO(3-2) and associated continuum emission from the gas-bearing debris disk around the nearby A star 49 Ceti, observed with ALMA. We analyze the ALMA visibilities in tandem with the broadband spectral energy distribution to measure the radial surface density profiles of dust and gas emission from the system. The radial extent of the gas disk (~220 au) is smaller than that of the dust disk (~300 au), consistent with recent observations of other gas-bearing debris disks. While there are so far only three broad debris disks with well characterized radial dust profiles at millimeter wavelengths, 49 Ceti’s disk shows a markedly

  2. ALMA Explores How Supermassive Black Holes Talk to Their Galaxies

    Science.gov (United States)

    Kohler, Susanna

    2017-03-01

    We believe that supermassive black holes evolve in tandem with their host galaxies but how do the two communicate? Observations from the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed new clues about how a monster black hole talks to its galaxy.A Hubble image of the central galaxy in the Phoenix cluster. [Adapted from Russell et al. 2017]Observing FeedbackActive galactic nuclei (AGN), the highly luminous centers of some galaxies, are thought to radiate due to active accretion onto the supermassive black hole at their center.Its long been suspected that the radiation and outflowing material which often takes the form of enormous bipolar radio jets emitted into the surroundings influence the AGNs host galaxy, affecting star formation rates and the evolution of the galaxy. This AGN feedback has been alternately suggested to trigger star formation, quench it, and truncate the growth of massive galaxies.The details of this feedback process, however, have yet to be thoroughly understood in part because its difficult to obtain detailed observations of how AGN outflows interact with the galactic gas surrounding them. Now, a team of scientists led by Helen Russell (Institute of Astronomy in Cambridge, UK) has published the results of a new, high-resolution look at the gas in a massive galaxy in the center of the Phoenix cluster.Many Uses for FuelThe Phoenix cluster, a nearby (z = 0.596) group of star-forming galaxies, is the most luminous X-ray cluster known. The central galaxy in the cluster is especially active: it hosts a starburst of 500800 solar masses per year, the largest starburst found in any galaxy below a redshift of z= 1.The star formation in this galaxy is sustained by an enormous reservoir of cold molecular gas roughly 20 billion solar masses worth. This reservoir also powers the galaxys central black hole, fueling powerful radio jets that extend into the hot atmosphere of the galaxy and blow a giant bubble into the hot gas at each pole.ALMA

  3. Tiers of the maintenance concept at ALMA in operations

    Science.gov (United States)

    Rabanus, David

    2014-08-01

    The Atacama Large Millimeter/submillimeter Array finds itself in the transition into full operations. Previous construction activities are being wrapped up, and regular, repetitive maintenance and upkeep will dominate the daily life, which asks for a consolidation and streamlining of the activities at the observatory. Especially the shifting focus to the high site of the observatory deserves more attention, since assembly, integration and verification activities at the base camp have ceased by now. In parallel, adjustments in the host country's labor legislation for operations at high geographic altitudes demand a review of the way things are done. This talk outlines the underlying operational concepts, lists the limiting constraints, describes the implementation of our reactions to those, and outlines our future intentions, which will be one in a number of steps towards optimization of the productivity of the observatory. The latter is the top level goal, which the Joint ALMA Observatory (JAO) has signed up for.

  4. A Complete ALMA Map of the Fomalhaut Debris Disk

    Energy Technology Data Exchange (ETDEWEB)

    MacGregor, Meredith A.; Wilner, David J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Matrà, Luca; Kennedy, Grant M.; Wyatt, Mark C.; Shannon, Andrew [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Kalas, Paul; Duchene, Gaspard; Graham, James R. [Astronomy Department, University of California, Berkeley CA 94720-3411 (United States); Pan, Margaret [MIT Department of Earth, Atmospheric, and Planetary Sciences, Cambridge, MA 02139 (United States); Hughes, A. Meredith [Department of Astronomy, Van Vleck Observatory, Wesleyan University, Middletown, CT 06459 (United States); Rieke, George H.; Su, Kate [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Clampin, Mark [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Fitzgerald, Michael P. [Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095 (United States); Holland, Wayne S. [UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Institute for Astronomy, Royal Observatory, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Panić, Olja [School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT (United Kingdom)

    2017-06-10

    We present ALMA mosaic observations at 1.3 mm (223 GHz) of the Fomalhaut system with a sensitivity of 14 μ Jy/beam. These observations provide the first millimeter map of the continuum dust emission from the complete outer debris disk with uniform sensitivity, enabling the first conclusive detection of apocenter glow. We adopt an MCMC modeling approach that accounts for the eccentric orbital parameters of a collection of particles within the disk. The outer belt is radially confined with an inner edge of 136.3 ± 0.9 au and width of 13.5 ± 1.8 au. We determine a best-fit eccentricity of 0.12 ± 0.01. Assuming a size distribution power-law index of q = 3.46 ± 0.09, we constrain the dust absorptivity power-law index β to be 0.9 < β < 1.5. The geometry of the disk is robustly constrained with inclination 65.°6 ± 0.°3, position angle 337.°9 ± 0.°3, and argument of periastron 22.°5 ± 4.°3. Our observations do not confirm any of the azimuthal features found in previous imaging studies of the disk with Hubble Space Telescope , SCUBA, and ALMA. However, we cannot rule out structures ≤10 au in size or that only affect smaller grains. The central star is clearly detected with a flux density of 0.75 ± 0.02 mJy, significantly lower than predicted by current photospheric models. We discuss the implications of these observations for the directly imaged Fomalhaut b and the inner dust belt detected at infrared wavelengths.

  5. ALMA OBSERVATIONS OF HD 141569’s CIRCUMSTELLAR DISK

    Energy Technology Data Exchange (ETDEWEB)

    White, J. A.; Boley, A. C. [Department of Physics and Astronomy, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada); Hughes, A. M.; Flaherty, K. M. [Department of Astronomy, Van Vleck Observatory, Wesleyan University, 96 Foss Hill Drive, Middletown, CT 06459 (United States); Ford, E. [Center for Exoplanets and Habitable Worlds, 525 Davey Laboratory, The Pennsylvania State University, University Park, PA 16802-2111 (United States); Wilner, D.; Payne, M. [Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Corder, S., E-mail: jawhite@astro.ubc.ca [North American ALMA Science Center, National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA, 22903 (United States)

    2016-09-20

    We present ALMA band 7 (345 GHz) continuum and {sup 12}CO( J = 3-2) observations of the circumstellar disk surrounding HD 141569. At an age of about 5 Myr, the disk has a complex morphology that may be best interpreted as a nascent debris system with gas. Our 870 μ m ALMA continuum observations resolve a dust disk out to approximately 56 au from the star (assuming a distance of 116 pc) with 0.″38 resolution and 0.07 mJy beam{sup −1} sensitivity. We measure a continuum flux density for this inner material of 3.8 ± 0.4 mJy (including calibration uncertainties). The {sup 12}CO(3-2) gas is resolved kinematically and spatially from about 30 to 210 au. The integrated {sup 12}CO(3-2) line flux density is 15.7 ± 1.6 Jy km s{sup −1}. We estimate the mass of the millimeter debris and {sup 12}CO(3-2) gas to be ≳0.04 M {sub ⊕} and ∼2 × 10{sup −3} M {sub ⊕}, respectively. If the millimeter grains are part of a collisional cascade, then we infer that the inner disk (<50 au) has ∼160 M {sub ⊕} contained within objects less than 50 km in radius, depending on the planetesimal size distribution and density assumptions. Markov Chain Monte Carlo modeling of the system reveals a disk morphology with an inclination of 53.°4 centered around an M = 2.39 M {sub ⊙} host star ( M sin( i ) = 1.92 M {sub ⊙}). We discuss whether the gas in HD 141569's disk may be second generation. If it is, the system can be used to study the clearing stages of planet formation.

  6. The Academic Publication Service AlmaDL Journals and the New Challenges of Open Access

    Directory of Open Access Journals (Sweden)

    Piero Grandesso

    2018-03-01

    Full Text Available AlmaDL Journals is an Open Access publishing service of the University of Bologna, Italy. After 5 years from the publication of the first paper in Conservation Science in Cultural Heritage about the service, we review the transformations and the growth it has experienced during this time span, with a look at the changes that have occurred in Open Access publishing that have driven and inspired the modifications adopted by AlmaDL Journals.

  7. El (reconocimiento de la madre en La mitad del alma

    Directory of Open Access Journals (Sweden)

    Sandra J. Schumm

    2011-01-01

    Full Text Available Resumen: La mitad del alma de Carme Riera, en que C rememora a su madre, enfatiza la importancia del reconocimiento de las mujeres en la memoria histórica. Desde el mito griego de Atena, quien ignoraba a su madre Metis, la sociedad patriarcal ha excluido a la madre, lo cual promete que la hija conlleve negación también, según Amber Jacobs en On Matricide. Jacobs observa que en La Oresteia hay crímenes sancionados contra las mujeres, las hijas están deprimidas, existe incesto contra la hija, la reproducción familiar se paraliza, toda la sociedad sufre y la hija se desperdicia también cuando la madre es menospreciada. Jacobs afirma que este desprecio de la madre que transcurría en los mitos griegos continúa en la sociedad y la psicología hoy en día. En esta novela de Riera, la hija protagonista, quien desconoce a su madre, sufre de un estado depresivo, la falta de creatividad y una conexión demasiado fuerte con su padre, semejante a lo que Jacobs observa en los mitos, pero la escritura de C sobre su madre la integrará en la consciencia y mejorará la situación de la hija y, últimamente, la de toda la civilización.Summary: Carme Riera‟s La mitad del alma, in which C recollects her mother, emphasizes the importance of the recognition of women in historic memory. Ever since the Greek myth of Athena, who was ignorant of the existence of her mother, Metis, patriarchal society has excluded the mother, a fact which promises that the daughter will also experience negation, according to Amber Jacobs in On Matricide. Jacobs observes that in La Oresteia there are sanctioned crimes against women, the daughters are depressed, there is incest against the daughter, she is dishonored, family reproduction stops, and all of society suffers when the mother is not appreciated. Jacobs affirms that the distain of the mother that took place in Greek myths continues in society and psychology today. In this novel by Riera, the protagonist/daughter, who

  8. Exploring Molecular Complexity in the Interstellar Medium with Alma

    Science.gov (United States)

    Belloche, Arnaud

    2017-06-01

    The search for complex organic molecules (COMs) in the interstellar medium (ISM) relies heavily on the progress made in the laboratory to record and characterize the rotational spectra of these molecules. Almost 200 different molecules have been identified in the ISM so far, in particular thanks to millimeter-wavelength observations of the star-forming molecular cloud core Sgr B2(N) in the Galactic Center region. The advent of the Atacama Large Millimeter/submillimeter Array (ALMA) has recently opened a new door to explore the molecular complexity of the ISM. Thanks to its high angular resolution, the spectral confusion of star-forming cores can be reduced, and its tremendous sensitivity allows astronomers to detect molecules of low abundance that could not be probed by previous generations of telescopes. I will present results of the EMoCA survey conducted toward Sgr B2(N) with ALMA. The main goal of this spectral line survey is to decipher the molecular content of Sgr B2(N) in order to test the predictions of astrochemical numerical simulations and gain insight into the chemical processes at work in the ISM. I will in particular report on the tentative detection of N-methylformamide, on the deuterium fractionation of COMs, and on the detection of a branched alkyl molecule in the ISM. The latter detection has unveiled a new domain in the structures available to the chemistry of star-forming regions and established a further connection to the COMs found in meteorites. A. Belloche, A. A. Meshcheryakov, R. T. Garrod et al. 2017, A&A, in press, DOI: 10.1051/0004-6361/201629724 A. Belloche, H. S. P. Müller, R. T. Garrod, and K. M. Menten 2016, A&A, 587, A91 A. Belloche, R. T. Garrod, H. S. P. Müller, and K. M. Menten 2014, Science, 345, 1584 R. T. Garrod, A. Belloche, H. S. P. Müller, and K. M. Menten 2017, A&A, in press, DOI: 10.1051/0004-6361/201630254.

  9. Design and performance of the ALMA-J prototype antenna

    Science.gov (United States)

    Ukita, Nobuharu; Saito, Masao; Ezawa, Hajime; Ikenoue, Bungo; Ishizaki, Hideharu; Iwashita, Hiroyuki; Yamaguchi, Nobuyuki; Hayakawa, Takahiro

    2004-10-01

    The National Astronomical Observatory of Japan has constructed a prototype 12-m antenna of the Atacama Compact Array to evaluate its performance at the ALMA Test Facility in the NRAO VLA observatory in New Mexico, the United States. The antenna has a CFRP tube backup structure (BUS) with CFRP boards to support 205 machined Aluminum surface panels. Their accuracies were measured to be 5.9 m rms on average. A chemical treatment technique of the surface panels has successfully applied to scatter the solar radiation, which resulted in a subreflector temperature increase of about 25 degrees relative to ambient temperature during direct solar observations. Holography measurements and panel adjustments led to a final surface accuracy of 20 m rms, (weighted by 12dB edge taper), after three rounds of the panel adjustments. Based on a long term temperature monitoring of the BUS and thermal deformation FEM calculation, the BUS thermal deformation was estimated to be less than 3.1 m rms. We have employed gear drive mechanism both for a fast position switching capability and for smooth drive at low velocities. Servo errors measured with angle encoders were found to be less than 0.1 arcseconds rms at rotational velocities below 0.1 degrees s-1 and to increase to 0.7 arcseconds rms at the maximum speed of the 'on-the-fly' scan as a single dish, 0.5 deg s-1 induced by the irregularity of individual gear tooth profiles. Simultaneous measurements of the antenna motion with the angle encoders and seismic accelerometers mounted at the primary reflector mirror edges and at the subreflector showed the same amplitude and phase of oscillation, indicating that they are rigid, suggesting that it is possible to estimate where the antenna is actually pointing from the encoder readout. Continuous tracking measurements of Polaris during day and night have revealed a large pointing drift due to thermal distortion of the yoke structure. We have applied retrospective thermal corrections to

  10. Solar Observations with the Atacama Large Millimeter/submillimeter Array (ALMA)

    Science.gov (United States)

    Bastian, Timothy S.

    2015-04-01

    The Atacama Large Millimeter/Submillimeter Array (ALMA) is a joint North American, European, and East Asian project that opens the mm-submm wavelength part of the electromagnetic spectrum for general astrophysical exploration, providing high-resolution imaging in frequency bands currently ranging from 84 GHz to 950 GHz (300 microns to 3 mm). Despite being a general purpose instrument, provisions have been made to enable solar observations with ALMA. Radiation emitted at ALMA wavelengths originates mostly from the chromosphere, which plays an important role in the transport of matter and energy, and the in heating the outer layers of the solar atmosphere. Despite decades of research, the solar chromosphere remains a significant challenge: both to observe, owing to the complicated formation mechanisms of currently available diagnostics; and to understand, as a result of the complex nature of the structure and dynamics of the chromosphere. ALMA has the potential to change the scene substantially as it serves as a nearly linear thermometer at high spatial and temporal resolution, enabling us to study the complex interaction of magnetic fields and shock waves and yet-to-be-discovered dynamical processes. Moreover, ALMA will play an important role in the study of energetic emissions associated with solar flares at sub-THz frequencies.In this paper we describe recent efforts to ensure that ALMA can be usefully exploited by the scientific community to address outstanding questions in solar physics. We summarize activities by the ALMA solar development team comprised of scientists from the East Asia, North America, and Europe. These activities include instrument testing, development of calibration and imaging strategies, software requirements development, and science simulations. Opportunities for the wider community to contribute to these efforts will be highlighted.

  11. ALMA Images of the Orion Hot Core at 349 GHz

    Energy Technology Data Exchange (ETDEWEB)

    Wright, M. C. H.; Plambeck, R. L., E-mail: wright@astro.berkeley.edu [Radio Astronomy Laboratory, University of California, Berkeley, CA 94720 (United States)

    2017-07-10

    We present ALMA images of the dust and molecular line emission in the Orion Hot Core at 349 GHz. At 0.″2 angular resolution the images reveal multiple clumps in an arc ∼1″ east of Orion Source I, the protostar at the center of the Kleinmann–Low Nebula, and another chain of peaks from IRc7 toward the southwest. The molecular line images show narrow filamentary structures at velocities >10 km s{sup −1} away from the heavily resolved ambient cloud velocity ∼5 km s{sup −1}. Many of these filaments trace the SiO outflow from Source I, and lie along the edges of the dust emission. Molecular line emission at excitation temperatures 300–2000 K, and velocities >10 km s{sup −1} from the ambient cloud, suggest that the Hot Core may be heated in shocks by the outflow from Source I or from the Becklin–Neugebauer (BN)/SrcI explosion. The spectral line observations also reveal a remarkable molecular ring, ∼2″ south of SrcI, with a diameter ∼600 au. The ring is seen in high-excitation transitions of HC{sub 3}N, HCN v 2 = 1, and SO{sub 2}. An impact of ejecta from the BN/SrcI explosion with a dense dust clump could result in the observed ring of shocked material.

  12. Primary health care: making Alma-Ata a reality.

    Science.gov (United States)

    Walley, John; Lawn, Joy E; Tinker, Anne; de Francisco, Andres; Chopra, Mickey; Rudan, Igor; Bhutta, Zulfiqar A; Black, Robert E

    2008-09-13

    The principles agreed at Alma-Ata 30 years ago apply just as much now as they did then. "Health for all" by the year 2000 was not achieved, and the Millennium Development Goals (MDGs) for 2015 will not be met in most low-income countries without substantial acceleration of primary health care. Factors have included insufficient political prioritisation of health, structural adjustment policies, poor governance, population growth, inadequate health systems, and scarce research and assessment on primary health care. We propose the following priorities for revitalising primary health care. Health-service infrastructure, including human resources and essential drugs, needs strengthening, and user fees should be removed for primary health-care services to improve use. A continuum of care for maternal, newborn, and child health services, including family planning, is needed. Evidence-based, integrated packages of community and primary curative and preventive care should be adapted to country contexts, assessed, and scaled up. Community participation and community health workers linked to strengthened primary-care facilities and first-referral services are needed. Furthermore, intersectoral action linking health and development is necessary, including that for better water, sanitation, nutrition, food security, and HIV control. Chronic diseases, mental health, and child development should be addressed. Progress should be measured and accountability assured. We prioritise research questions and suggest actions and measures for stakeholders both locally and globally, which are required to revitalise primary health care.

  13. Exploring No-SQL alternatives for ALMA monitoring system

    Science.gov (United States)

    Shen, Tzu-Chiang; Soto, Ruben; Merino, Patricio; Peña, Leonel; Bartsch, Marcelo; Aguirre, Alvaro; Ibsen, Jorge

    2014-07-01

    The Atacama Large Millimeter /submillimeter Array (ALMA) will be a unique research instrument composed of at least 66 reconfigurable high-precision antennas, located at the Chajnantor plain in the Chilean Andes at an elevation of 5000 m. This paper describes the experience gained after several years working with the monitoring system, which has a strong requirement of collecting and storing up to 150K variables with a highest sampling rate of 20.8 kHz. The original design was built on top of a cluster of relational database server and network attached storage with fiber channel interface. As the number of monitoring points increases with the number of antennas included in the array, the current monitoring system demonstrated to be able to handle the increased data rate in the collection and storage area (only one month of data), but the data query interface showed serious performance degradation. A solution based on no-SQL platform was explored as an alternative to the current long-term storage system. Among several alternatives, mongoDB has been selected. In the data flow, intermediate cache servers based on Redis were introduced to allow faster streaming of the most recently acquired data to web based charts and applications for online data analysis.

  14. Health for All Now! Reviving the spirit of Alma Ata in the Twenty-first century: An Introduction to the Alma Ata Declaration

    Directory of Open Access Journals (Sweden)

    Fran Baum

    2007-01-01

    Full Text Available Abstract In 1978 two United Nations organizations, the World Health Organization and UNICEF, held a joint conference at Alma Ata in the Soviet Union at which health was described as a human right to which all people were entitled. The goal of achieving health for all by the end of the century was established. The Alma Ata Declaration on Primary Health Care emerged from this conference. It was endorsed on the 12th September 1978, and has inspired subsequent generations of health activists. It has become a common meeting ground where likeminded public health personnel can compare and discuss strategy and relate their discussion to a common document. The slogan “Health for All by the Year 2000”, while not achieved, has been a rallying call for progressive health workers and activists. The Declaration has also inspired the global people’s health movement and two global people’s health assemblies. The concept “primary health care” has been crucial to the improvement of many countries’ health systems and, while its meaning has been variously interpreted, the pursuit of the ideal of comprehensive primary health care still motivates health workers around the world who want to ensure a more people-centred, responsive and effective and efficient health care system for their community and country. Thus the Alma Ata Declaration is a quite remarkable document and has made an impact that few other before or since have had. This article describes the international context that enabled the drafting and adoption of the Alma Ata Declaration. It then describes the document and assesses the reasons for its importance. The struggles for the ideals and strategies of the Declaration through the progressively more hostile international climate of the 1980s and 1990s are discussed. Finally, the prospects for a revival of the spirit of Alma Ata are assessed.

  15. Supporting Student Learning in Computer Science Education via the Adaptive Learning Environment ALMA

    Directory of Open Access Journals (Sweden)

    Alexandra Gasparinatou

    2015-10-01

    Full Text Available This study presents the ALMA environment (Adaptive Learning Models from texts and Activities. ALMA supports the processes of learning and assessment via: (1 texts differing in local and global cohesion for students with low, medium, and high background knowledge; (2 activities corresponding to different levels of comprehension which prompt the student to practically implement different text-reading strategies, with the recommended activity sequence adapted to the student’s learning style; (3 an overall framework for informing, guiding, and supporting students in performing the activities; and; (4 individualized support and guidance according to student specific characteristics. ALMA also, supports students in distance learning or in blended learning in which students are submitted to face-to-face learning supported by computer technology. The adaptive techniques provided via ALMA are: (a adaptive presentation and (b adaptive navigation. Digital learning material, in accordance with the text comprehension model described by Kintsch, was introduced into the ALMA environment. This material can be exploited in either distance or blended learning.

  16. The ALMA Band 9 receiver. Design, construction, characterization, and first light : Design, construction, characterization, and first light

    NARCIS (Netherlands)

    Baryshev, A. M.; Hesper, R.; Mena, F. P.; Klapwijk, T. M.; van Kempen, T. A.; Hogerheijde, M. R.; Jackson, B. D.; Adema, J.; Gerlofsma, G. J.; Bekema, M. E.; Barkhof, J.; de Haan-Stijkel, L. H. R.; van den Bemt, M.; Koops, A.; Keizer, K.; Pieters, C.; Koops van het Jagt, J.; Schaeffer, H.H.A.; Zijlstra, T.; Kroug, M.; Lodewijk, C. F. J.; Wielinga, K.; Boland, W.; de Graauw, M. W. M.; van Dishoeck, E. F.; Jager, H.; Wild, W.

    Aims: We describe the design, construction, and characterization of the Band 9 heterodyne receivers (600-720 GHz) for the Atacama Large Millimeter/submillimeter Array (ALMA). First-light Band 9 data, obtained during ALMA commissioning and science verification phases, are presented as well. Methods:

  17. The Cultural Implications of Primary Health Care and the Declaration of Alma-Ata: The Health District of Kedougou, Senegal

    Science.gov (United States)

    Blanas, Demetri A.

    2008-01-01

    In 1978, the World Health Organization (WHO) and the international health community convoked a conference in Alma-Ata, Kazakhstan, to address global inequalities in health. The conference resulted in the publication of the "Declaration of Alma-Ata," which made the ambitious call "for urgent action by all governments, all health and…

  18. The ALMA View of the OMC1 Explosion in Orion

    Energy Technology Data Exchange (ETDEWEB)

    Bally, John; Youngblood, Allison [Astrophysical and Planetary Sciences Department University of Colorado, UCB 389 Boulder, Colorado 80309 (United States); Ginsburg, Adam [ESO Headquarters Karl-Schwarzschild-Str. 2 D-85748, Garching bei Munchen (Germany); Arce, Hector [Department of Astronomy Steinbach Hall, 52 Hillhouse Avenue, Yale University, New Haven, CT 06511 (United States); Eisner, Josh [Steward Observatory University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Zapata, Luis [Instituto de Radioastronomía y Astrofísíca, UNAM Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacán, México (Mexico); Zinnecker, Hans, E-mail: john.bally@colorado.edu [Deutsches SOFIA Institut (DSI) University of Stuttgart, Pfaffenwaldring 29, D-70569 (Germany)

    2017-03-01

    Most massive stars form in dense clusters where gravitational interactions with other stars may be common. The two nearest forming massive stars, the BN object and Source I, located behind the Orion Nebula, were ejected with velocities of ∼29 and ∼13 km s{sup −1} about 500 years ago by such interactions. This event generated an explosion in the gas. New ALMA observations show in unprecedented detail, a roughly spherically symmetric distribution of over a hundred {sup 12}CO J = 2−1 streamers with velocities extending from V {sub LSR} = −150 to +145 km s{sup −1}. The streamer radial velocities increase (or decrease) linearly with projected distance from the explosion center, forming a “Hubble Flow” confined to within 50″ of the explosion center. They point toward the high proper-motion, shock-excited H{sub 2} and [Fe ii] “fingertips” and lower-velocity CO in the H{sub 2} wakes comprising Orion's “fingers.” In some directions, the H{sub 2} “fingers” extend more than a factor of two farther from the ejection center than the CO streamers. Such deviations from spherical symmetry may be caused by ejecta running into dense gas or the dynamics of the N -body interaction that ejected the stars and produced the explosion. This ∼10{sup 48} erg event may have been powered by the release of gravitational potential energy associated with the formation of a compact binary or a protostellar merger. Orion may be the prototype for a new class of stellar explosiozn responsible for luminous infrared transients in nearby galaxies.

  19. ALMA OBSERVATIONS OF HCN AND ITS ISOTOPOLOGUES ON TITAN

    Energy Technology Data Exchange (ETDEWEB)

    Molter, Edward M.; Nixon, C. A.; Cordiner, M. A.; Charnley, S. B.; Lindberg, J. E. [NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States); Serigano, J. [Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD 21218 (United States); Irwin, P. G. J. [Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, University of Oxford, Parks Road, Oxford, OX1 3PU (United Kingdom); Teanby, N. A., E-mail: edward.m.molter@nasa.gov [School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol, BS8 1RJ (United Kingdom)

    2016-08-01

    We present sub-millimeter spectra of HCN isotopologues on Titan, derived from publicly available ALMA flux calibration observations of Titan taken in early 2014. We report the detection of a new HCN isotopologue on Titan, H{sup 13}C{sup 15}N, and confirm an earlier report of detection of DCN. We model high signal-to-noise observations of HCN, H{sup 13}CN, HC{sup 15}N, DCN, and H{sup 13}C{sup 15}N to derive abundances and infer the following isotopic ratios: {sup 12}C/{sup 13}C = 89.8 ± 2.8, {sup 14}N/{sup 15}N = 72.3 ± 2.2, D/H = (2.5 ± 0.2) × 10{sup −4}, and HCN/H{sup 13}C{sup 15}N = 5800 ± 270 (1 σ errors). The carbon and nitrogen ratios are consistent with and improve on the precision of previous results, confirming a factor of ∼2.3 elevation in {sup 14}N/{sup 15}N in HCN compared to N{sub 2} and a lack of fractionation in {sup 12}C/{sup 13}C from the protosolar value. This is the first published measurement of D/H in a nitrile species on Titan, and we find evidence for a factor of ∼2 deuterium enrichment in hydrogen cyanide compared to methane. The isotopic ratios we derive may be used as constraints for future models to better understand the fractionation processes occurring in Titan’s atmosphere.

  20. ETHYL CYANIDE ON TITAN: SPECTROSCOPIC DETECTION AND MAPPING USING ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Cordiner, M. A.; Palmer, M. Y.; Nixon, C. A.; Charnley, S. B.; Mumma, M. J.; Serigano, J. [NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States); Irwin, P. G. J. [Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, University of Oxford, Parks Road, Oxford, OX1 3PU (United Kingdom); Teanby, N. A. [School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol, BS8 1RJ (United Kingdom); Kisiel, Z. [Institute of Physics, Polish Academy of Sciences, Al. Lotnikøw 32/46, 02-668 Warszawa (Poland); Kuan, Y.-J.; Chuang, Y.-L. [National Taiwan Normal University, Taipei 116, Taiwan (China); Wang, K.-S., E-mail: martin.cordiner@nasa.gov [Institute of Astronomy and Astrophysics, Academia Sinica, Taipei 106, Taiwan (China)

    2015-02-10

    We report the first spectroscopic detection of ethyl cyanide (C{sub 2}H{sub 5}CN) in Titan’s atmosphere, obtained using spectrally and spatially resolved observations of multiple emission lines with the Atacama Large Millimeter/submillimeter Array (ALMA). The presence of C{sub 2}H{sub 5}CN in Titan’s ionosphere was previously inferred from Cassini ion mass spectrometry measurements of C{sub 2}H{sub 5}CNH{sup +}. Here we report the detection of 27 rotational lines from C{sub 2}H{sub 5}CN (in 19 separate emission features detected at >3σ confidence) in the frequency range 222–241 GHz. Simultaneous detections of multiple emission lines from HC{sub 3}N, CH{sub 3}CN, and CH{sub 3}CCH were also obtained. In contrast to HC{sub 3}N, CH{sub 3}CN, and CH{sub 3}CCH, which peak in Titan’s northern (spring) hemisphere, the emission from C{sub 2}H{sub 5}CN is found to be concentrated in the southern (autumn) hemisphere, suggesting a distinctly different chemistry for this species, consistent with a relatively short chemical lifetime for C{sub 2}H{sub 5}CN. Radiative transfer models show that C{sub 2}H{sub 5}CN is most concentrated at altitudes ≳200 km, suggesting production predominantly in the stratosphere and above. Vertical column densities are found to be in the range (1–5) × 10{sup 14} cm{sup −2}.

  1. The ALMA View of the OMC1 Explosion in Orion

    International Nuclear Information System (INIS)

    Bally, John; Youngblood, Allison; Ginsburg, Adam; Arce, Hector; Eisner, Josh; Zapata, Luis; Zinnecker, Hans

    2017-01-01

    Most massive stars form in dense clusters where gravitational interactions with other stars may be common. The two nearest forming massive stars, the BN object and Source I, located behind the Orion Nebula, were ejected with velocities of ∼29 and ∼13 km s −1 about 500 years ago by such interactions. This event generated an explosion in the gas. New ALMA observations show in unprecedented detail, a roughly spherically symmetric distribution of over a hundred 12 CO J = 2−1 streamers with velocities extending from V LSR = −150 to +145 km s −1 . The streamer radial velocities increase (or decrease) linearly with projected distance from the explosion center, forming a “Hubble Flow” confined to within 50″ of the explosion center. They point toward the high proper-motion, shock-excited H 2 and [Fe ii] “fingertips” and lower-velocity CO in the H 2 wakes comprising Orion's “fingers.” In some directions, the H 2 “fingers” extend more than a factor of two farther from the ejection center than the CO streamers. Such deviations from spherical symmetry may be caused by ejecta running into dense gas or the dynamics of the N -body interaction that ejected the stars and produced the explosion. This ∼10 48 erg event may have been powered by the release of gravitational potential energy associated with the formation of a compact binary or a protostellar merger. Orion may be the prototype for a new class of stellar explosiozn responsible for luminous infrared transients in nearby galaxies.

  2. The SOLA Team: A Star Formation Project To Study the Soul of Lupus with ALMA

    Science.gov (United States)

    De Gregorio-Monsalvo, Itziar; Saito, M.; Rodon, J.; Takahashi, S.

    2017-06-01

    The SOLA team is a multi-national and multi-wavelength collaboration composed by scientists with technical expertise in ALMA and in infrared and optical techniques. The aim of the team is to establish a low-mass star formation scenario based on the Lupus molecular clouds. In this talk I will present our unique catalog of pre-stellar and proto-stellar cores toward Lupus molecular clouds, the results on our latest studies in protoplanetary disks, as well as our ALMA Cycle 3 data aiming at testing the formation mechanism of sub-stellar objects in Lupus molecular clouds.

  3. A web-based dashboard for the high-level monitoring of ALMA

    Science.gov (United States)

    Pietriga, Emmanuel; Filippi, Giorgio; Véliz, Luis; del Campo, Fernando; Ibsen, Jorge

    2014-07-01

    The ALMA radio-telescope's operations depend on the availability of high-level, easy-to-understand status information about all of its components. The ALMA Dashboard aims at providing an all-in-one-place near-real-time overview of the observatory's key elements and figures to both line and senior management. The Dashboard covers a wide range of elements beyond antennas, such as pads, correlator and central local oscillator. Data can be displayed in multiple ways, including: a table view, a compact view fitting on a single screen, a timeline showing detailed information over time, a logbook, a geographical map.

  4. Non-Equilibrium Chemistry of O-Rich AGB Stars as Revealed by ALMA

    Science.gov (United States)

    Wong, Ka Tat

    2018-04-01

    Chemical models suggest that pulsation driven shocks propagating from the stellar surfaces of oxygen-rich evolved stars to the dust formation zone trigger non-equilibrium chemistry in the shocked gas near the star, including the formation of carbon-bearing molecules in the stellar winds dominated by oxygen-rich chemistry. Recent long-baseline ALMA observations are able to give us a detailed view of the molecular line emission and absorption at an angular resolution of a few stellar radii. I am going to present the latest results from the ALMA observations of IK Tau and o Cet in late 2017, with a particular focus on HCN.

  5. The Best of Two Worlds: ALMA + IRAM30M Observations of the Orion Integral Shape Filament

    Science.gov (United States)

    Hacar Gonzalez, Alvaro

    2018-01-01

    We have investigated the internal gas structure of the Orion Integral Shape filament using two large-scale, 150-pointing ALMA-12m mosaics and previous IRAM30m single-dish (SD) observations. From the combination of both single-dish and interferometric data we have produced a high-dynamic range and high-sensitivity map describing the internal gas structure of this filament at scales between 2 pc and 2000 AU (Hacar et al, submitted to A&A). In a series of individual CASA reductions (w/o SD data + w/o feathering), we have investigated the impact of the different uv-coverages on both the total flux and line velocity structure of our ALMA maps. Our analysis highlights the critical role played by the zero-spacing data at the different stages of the cleaning process. The results of these ALMA+IRAM30m experiments emphasize the need of high-sensitivity SD observations for the analysis of large-scale interferometric maps. During my talk, I will discuss the implications of these experiments on the dawn of the ALMA era and in the context of the new AtLAST telescope.

  6. Construction and Characterization of a Sideband-separating heterodyne mixer for Band 9 of ALMA

    NARCIS (Netherlands)

    Mena, F. P.; Kooi, J.; Baryshev, A. M.; Lodewijk, C. F. J.; Klapwijk, T. M.; Hesper, R.; Wild, W.

    2007-01-01

    In this article we present the design, modeling and construction of a side-band-separating (2SB) heterodyne receiver for the frequency range from 600 to 720 GHz that corresponds to band 9 band of ALMA. The characteristics of this receiver present a significant improvement over the current

  7. The ALMA Data Mining Toolkit I: Archive Setup and User Usage

    Science.gov (United States)

    Teuben, P.; Pound, M.; Mundy, L.; Looney, L.; Friedel, D. N.

    2014-05-01

    We report on an ALMA development study and project where we employ a novel approach to add data and data descriptors to ALMA archive data and allowing further flexible data mining on retrieved data. We call our toolkit ADMIT (the ALMA Data Mining Toolkit) that works within the Python based CASA environment. What is described here is a design study, with some exiting toy code to prove the concept. After ingestion of science ready datacubes, ADMIT will compute a number of basic and advanced data products, and their descriptors. Examples of such data products are cube statistics, line identification tables, line cubes, moment maps, an integrated spectrum, overlap integrals and feature extraction tables. Together with a descriptive XML file, a small number of visual aids are added to a ZIP file that is deposited into the archive. Large datasets (such as line cubes) will have to be rederived by the user once they have also downloaded the actual ALMA Data Products, or via VO services if available. ADMIT enables the user to rederive all its products with different methods and parameters, and compare archive product with their own.

  8. Development of a 0.6 THz SIS Receiver for ALMA

    NARCIS (Netherlands)

    Baryshev, A. M.; van de Stadt, H.; Schaeffer, H.; Hesper, R.; Zijlstra, T.; Zuiddam, M.; Wild, W.; de Jong, L

    2001-01-01

    The Atacama Large Millimeter Array (ALMA) requires low noise SIS receivers for frequencies from about 80 GHz to 950 GHz with very large IF bandwidth (4-12 GHz). Additional requirements for these receivers are high reliability, low cost and the possibility of series production. In this paper we

  9. SÓCRATES E O CUIDADO DE SI OU A TERAPÊUTICA DA ALMA

    Directory of Open Access Journals (Sweden)

    Raimundo Araújo dos Santos

    2008-03-01

    Full Text Available Esse artigo pretende ser uma abordagem simples, na verdade, um resumo, recolhido dostextos de Platão sobre o auto-conhecimento e o cuidado de si. Esses são os elementos queconstituem a base do saber ético iniciado por Sócrates e o ponto de partida do que chamamosterapêutica da alma.

  10. Equilibrium chemical reaction of supersonic hydrogen-air jets (the ALMA computer program)

    Science.gov (United States)

    Elghobashi, S.

    1977-01-01

    The ALMA (axi-symmetrical lateral momentum analyzer) program is concerned with the computation of two dimensional coaxial jets with large lateral pressure gradients. The jets may be free or confined, laminar or turbulent, reacting or non-reacting. Reaction chemistry is equilibrium.

  11. NRAO welcomes new Head of the North American ALMA Science Center

    Science.gov (United States)

    2008-09-01

    The National Radio Astronomy Observatory (NRAO) has announced the appointment of Dr. Carol Jean Lonsdale as the Observatory's new Assistant Director for the North American ALMA Science Center (NAASC). As NAASC head, Lonsdale will lead the team that will enable North American astronomers to exploit the capabilities of the Atacama Large Millimeter/submillimeter Array (ALMA), a powerful new international astronomical facility under construction in the high-altitude Atacama Desert of northeastern Chile. Dr. Carol Lonsdale Dr. Carol Lonsdale CREDIT: NRAO/AUI/NSF "With ALMA, our understanding of such crucial processes as the formation of galaxies, stars, and planetary systems is going to take a giant leap. I look forward to leading the people here at NRAO who are working to make ALMA accessible to a wide range of science users," said Lonsdale. Lonsdale comes to NRAO with an extensive background in overseeing large astronomical projects. She has held senior positions at the Infrared Processing and Analysis Center (IPAC) of the California Institute of Technology, where she served as Senior Research Scientist, Head of Science Staff, and Manager of the Wide-Field Infrared Explorer and Infrared Science Archive. She has been a science team member on the Infrared-Red Astronomy Satellite, Two Micron All Sky Survey, Wide-Field Infrared Survey Explorer, and other missions. "Carol brings a new dimension to the NAASC, with broad experience in user support of space infrared missions at IPAC and world-class scientific leadership in the study of star forming galaxies," said Christopher Carilli, who headed the NAASC prior to his new appointment as NRAO Chief Scientist. When completed in 2012, ALMA will be an array of at least 66 high-precision radio telescopes that will image faint millimeter- and submillimeter-wavelength light emitted by cold objects in the Universe, such as molecular clouds where stars are forming. It will also study warmer objects in the early Universe whose infrared

  12. A Multi-Wavelength View of Planet Forming Regions: Unleashing the Full Power of ALMA

    Science.gov (United States)

    Tazzari, Marco

    2017-11-01

    Observations at sub-mm/mm wavelengths allow us to probe the solids in the interior of protoplanetary disks, where the bulk of the dust is located and planet formation is expected to occur. However, the actual size of dust grains is still largely unknown due to the limited angular resolution and sensitivity of past observations. The upgraded VLA and, especially, the ALMA observatories provide now powerful tools to resolve grain growth in disks, making the time ripe for developing a multi-wavelength analysis of sub-mm/mm observations of disks. In my contribution I will present a novel analysis method for multi-wavelength ALMA/VLA observations which, based on the self-consistent modelling of the sub-mm/mm disk continuum emission, allows us to constrain simultaneously the size distribution of dust grains and the disk's physical structure (Tazzari et al. 2016, A&A 588 A53). I will also present the recent analysis of spatially resolved ALMA Band 7 observations of a large sample of disks in the Lupus star forming region, from which we obtained a tentative evidence of a disk size-disk mass correlation (Tazzari et al. 2017, arXiv:1707.01499). Finally, I will introduce galario, a GPU Accelerated Library for the Analysis of Radio Interferometry Observations. Fitting the observed visibilities in the uv-plane is computationally demanding: with galario we solve this problem for the current as well as for the full-science ALMA capabilities by leveraging on the computing power of GPUs, providing the computational breakthrough needed to fully exploit the new wealth of information delivered by ALMA.

  13. Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): High-Resolution Interferometric Imaging

    Science.gov (United States)

    Shimojo, M.; Bastian, T. S.; Hales, A. S.; White, S. M.; Iwai, K.; Hills, R. E.; Hirota, A.; Phillips, N. M.; Sawada, T.; Yagoubov, P.; Siringo, G.; Asayama, S.; Sugimoto, M.; Brajša, R.; Skokić, I.; Bárta, M.; Kim, S.; de Gregorio-Monsalvo, I.; Corder, S. A.; Hudson, H. S.; Wedemeyer, S.; Gary, D. E.; De Pontieu, B.; Loukitcheva, M.; Fleishman, G. D.; Chen, B.; Kobelski, A.; Yan, Y.

    2017-07-01

    Observations of the Sun at millimeter and submillimeter wavelengths offer a unique probe into the structure, dynamics, and heating of the chromosphere; the structure of sunspots; the formation and eruption of prominences and filaments; and energetic phenomena such as jets and flares. High-resolution observations of the Sun at millimeter and submillimeter wavelengths are challenging due to the intense, extended, low-contrast, and dynamic nature of emission from the quiet Sun, and the extremely intense and variable nature of emissions associated with energetic phenomena. The Atacama Large Millimeter/submillimeter Array (ALMA) was designed with solar observations in mind. The requirements for solar observations are significantly different from observations of sidereal sources and special measures are necessary to successfully carry out this type of observations. We describe the commissioning efforts that enable the use of two frequency bands, the 3-mm band (Band 3) and the 1.25-mm band (Band 6), for continuum interferometric-imaging observations of the Sun with ALMA. Examples of high-resolution synthesized images obtained using the newly commissioned modes during the solar-commissioning campaign held in December 2015 are presented. Although only 30 of the eventual 66 ALMA antennas were used for the campaign, the solar images synthesized from the ALMA commissioning data reveal new features of the solar atmosphere that demonstrate the potential power of ALMA solar observations. The ongoing expansion of ALMA and solar-commissioning efforts will continue to enable new and unique solar observing capabilities.

  14. The ALMA Phasing System: A Beamforming Capability for Ultra-high-resolution Science at (Sub)Millimeter Wavelengths

    Science.gov (United States)

    Matthews, L. D.; Crew, G. B.; Doeleman, S. S.; Lacasse, R.; Saez, A. F.; Alef, W.; Akiyama, K.; Amestica, R.; Anderson, J. M.; Barkats, D. A.; Baudry, A.; Broguière, D.; Escoffier, R.; Fish, V. L.; Greenberg, J.; Hecht, M. H.; Hiriart, R.; Hirota, A.; Honma, M.; Ho, P. T. P.; Impellizzeri, C. M. V.; Inoue, M.; Kohno, Y.; Lopez, B.; Martí-Vidal, I.; Messias, H.; Meyer-Zhao, Z.; Mora-Klein, M.; Nagar, N. M.; Nishioka, H.; Oyama, T.; Pankratius, V.; Perez, J.; Phillips, N.; Pradel, N.; Rottmann, H.; Roy, A. L.; Ruszczyk, C. A.; Shillue, B.; Suzuki, S.; Treacy, R.

    2018-01-01

    The Atacama Millimeter/submillimeter Array (ALMA) Phasing Project (APP) has developed and deployed the hardware and software necessary to coherently sum the signals of individual ALMA antennas and record the aggregate sum in Very Long Baseline Interferometry (VLBI) Data Exchange Format. These beamforming capabilities allow the ALMA array to collectively function as the equivalent of a single large aperture and participate in global VLBI arrays. The inclusion of phased ALMA in current VLBI networks operating at (sub)millimeter wavelengths provides an order of magnitude improvement in sensitivity, as well as enhancements in u–v coverage and north–south angular resolution. The availability of a phased ALMA enables a wide range of new ultra-high angular resolution science applications, including the resolution of supermassive black holes on event horizon scales and studies of the launch and collimation of astrophysical jets. It also provides a high-sensitivity aperture that may be used for investigations such as pulsar searches at high frequencies. This paper provides an overview of the ALMA Phasing System design, implementation, and performance characteristics.

  15. The Impacts of ALMA Primary Variables on Profitability An Empirical Study of Indonesian Banking

    Directory of Open Access Journals (Sweden)

    Sapto Jumono

    2015-04-01

    Full Text Available This study aims to determine the impact of liquidity on BEP and ROE in Indonesian banking industry. The supporting theory in this study is ALMA theory. Based on annual data for the period 2001-2014 and following purposive sampling technique, the acquired amount of sample study is 97 banks. The data is analyzed using panel data regression of GMM Arrelano Bond, as a novelty in data processing, therefore the speed of adjustment can be known. The ALMA variables such as LAR, capital, leverage, operating expenses, interest income, and CAR sensitivity have a significant effect on BEP and ROE. Meanwhile LDR, NPL, the FBI have no impact on profitability. The implication of this study is the fact that banking performance in Indonesia can be leveled up through the reduction in mortgage interest rates and increment of credit volume and FBI.

  16. Corpo e Alma em Foucault: Postulados para uma Metodologia da Psicologia

    Directory of Open Access Journals (Sweden)

    Fernando de Almeida Silveira

    2003-01-01

    Full Text Available Michel Foucault destaca o corpo como expressão de poderes e de saberes que se articulam estrategicamente na história da sociedade ocidental. O corpo é, simultaneamente, agente e peça dentro de um jogo de forças presente em toda a rede social, que o torna depositário de marcas e de sinais que nele se inscrevem nesses embates, os quais, por sua vez, têm na corporeidade seu "campo de prova". E a alma surge como instrumento de atuação dos poderes/saberes sobre o corpo, no processo de constituição do corpo histórico dos sujeitos. O objetivo deste trabalho é desenvolver postulados sobre o corpo e a alma em Foucault, para o estudo e a prática da Psicologia.

  17. Design and Performance of ALMA Band 1 Receiver and its Future Prospects

    Science.gov (United States)

    Chiong, Chau Ching

    2018-01-01

    ALMA Band 1 receiver covering 35-50 GHz is with the largest relative bandwidth among ten ALMA bands. The Band 1 receiver front-end cartridges are now in preproduction stage. Even with the large noise contribution from the warm optics (5-11 K), the first three Band 1 cartridges still exhibit state-of-the-art receiver noise temperature of 16-31 K for any combination of the RF and LO frequencies. In the presentation, we will not only present the Band 1 receiver design and system performance, but also discuss the future prospects to further enhance its performance and capabilities with lower receiver noise temperature, wider RF and IF frequency coverage, focal plane array configuration, and digital signal processing.

  18. VizieR Online Data Catalog: AS 209 ALMA image (Fedele+, 2018)

    Science.gov (United States)

    Fedele, D.; Tazzari, M.; Booth, R.; Testi, L.; Clarke, C. J.; Pascucci, I.; Kospal, A.; Semenov, D.; Bruderer, S.; Henning, T.; Teague, R.

    2018-02-01

    The ALMA observations of AS 209 (J2000: RA=16:49:15.296, DE=-14:22:09.02) have been performed on 2016 September 22 (with 38 antennas) and 26 (41 antennas) in band 6 (211-275GHz) as part of the project ID 2015.1.00486.S (PI: D. Fedele). The correlator setup includes a broad (2GHz bandwidth) spectral window centered at 230GHz. (2 data files).

  19. ALMA OBSERVATIONS OF Ly α BLOB 1: HALO SUBSTRUCTURE ILLUMINATED FROM WITHIN

    Energy Technology Data Exchange (ETDEWEB)

    Geach, J. E. [Centre for Astrophysics Research, University of Hertfordshire, Hatfield, AL10 9AB (United Kingdom); Narayanan, D. [Dept. of Physics and Astronomy, Haverford College, PA 19041 (United States); Matsuda, Y.; Ao, Y.; Kubo, M. [National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588 (Japan); Hayes, M. [Stockholm University, Dept. of Astronomy and Oskar Klein Centre for Cosmoparticle Physics, SE-10691, Stockholm (Sweden); Mas-Ribas, Ll.; Dijkstra, M. [Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, NO-0315 Oslo (Norway); Steidel, C. C. [California Institute of Technology, 1216 East California Boulevard, MS 249-17, Pasadena, CA 91125 (United States); Chapman, S. C. [Dept. of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 4R2 (Canada); Feldmann, R. [Dept. of Astronomy, University of California Berkeley, CA 94720 (United States); Avison, A. [UK ALMA Regional Centre Node, Manchester (United Kingdom); Agertz, O. [Dept. of Physics, University of Surrey, GU2 7XH, Surrey (United Kingdom); Birkinshaw, M.; Bremer, M. N. [H. H. Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol, BS8 1TL (United Kingdom); Clements, D. L. [Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ (United Kingdom); Dannerbauer, H. [Instituto de Astrofísica de Canarias, La Laguna, Tenerife (Spain); Farrah, D. [Dept. of Physics, Virginia Tech, Blacksburg, VA 24061 (United States); Harrison, C. M. [Centre for Extragalactic Astronomy, Dept. of Physics, Durham University, South Road, Durham, DH1 3LE (United Kingdom); Michałowski, M. J., E-mail: j.geach@herts.ac.uk [Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ (United Kingdom); and others

    2016-11-20

    We present new Atacama Large Millimeter/Submillimeter Array (ALMA) 850 μ m continuum observations of the original Ly α Blob (LAB) in the SSA22 field at z = 3.1 (SSA22-LAB01). The ALMA map resolves the previously identified submillimeter source into three components with a total flux density of S {sub 850} = 1.68 ± 0.06 mJy, corresponding to a star-formation rate of ∼150 M {sub ⊙} yr{sup -1}. The submillimeter sources are associated with several faint ( m ≈ 27 mag) rest-frame ultraviolet sources identified in Hubble Space Telescope Imaging Spectrograph (STIS) clear filter imaging ( λ ≈ 5850 Å). One of these companions is spectroscopically confirmed with the Keck Multi-Object Spectrometer For Infra-Red Exploration to lie within 20 projected kpc and 250 km s{sup -1} of one of the ALMA components. We postulate that some of these STIS sources represent a population of low-mass star-forming satellites surrounding the central submillimeter sources, potentially contributing to their growth and activity through accretion. Using a high-resolution cosmological zoom simulation of a 10{sup 13} M {sub ⊙} halo at z = 3, including stellar, dust, and Ly α radiative transfer, we can model the ALMA+STIS observations and demonstrate that Ly α photons escaping from the central submillimeter sources are expected to resonantly scatter in neutral hydrogen, the majority of which is predicted to be associated with halo substructure. We show how this process gives rise to extended Ly α emission with similar surface brightness and morphology to observed giant LABs.

  20. Quiescent Prominences in the Era of ALMA. II. Kinetic Temperature Diagnostics

    Science.gov (United States)

    Gunár, Stanislav; Heinzel, Petr; Anzer, Ulrich; Mackay, Duncan H.

    2018-01-01

    We provide the theoretical background for diagnostics of the thermal properties of solar prominences observed by the Atacama Large Millimeter/submillimeter Array (ALMA). To do this, we employ the 3D Whole-Prominence Fine Structure (WPFS) model that produces synthetic ALMA-like observations of a complex simulated prominence. We use synthetic observations derived at two different submillimeter/millimeter (SMM) wavelengths—one at a wavelength at which the simulated prominence is completely optically thin and another at a wavelength at which a significant portion of the simulated prominence is optically thick—as if these were the actual ALMA observations. This allows us to develop a technique for an analysis of the prominence plasma thermal properties from such a pair of simultaneous high-resolution ALMA observations. The 3D WPFS model also provides detailed information about the distribution of the kinetic temperature and the optical thickness along any line of sight. We can thus assess whether the measure of the kinetic temperature derived from observations accurately represents the actual kinetic temperature properties of the observed plasma. We demonstrate here that in a given pixel the optical thickness at the wavelength at which the prominence plasma is optically thick needs to be above unity or even larger to achieve a sufficient accuracy of the derived information about the kinetic temperature of the analyzed plasma. Information about the optical thickness cannot be directly discerned from observations at the SMM wavelengths alone. However, we show that a criterion that can identify those pixels in which the derived kinetic temperature values correspond well to the actual thermal properties in which the observed prominence can be established.

  1. DETECTION OF LENSING SUBSTRUCTURE USING ALMA OBSERVATIONS OF THE DUSTY GALAXY SDP.81

    Energy Technology Data Exchange (ETDEWEB)

    Hezaveh, Yashar D.; Mao, Yao-Yuan; Morningstar, Warren; Blandford, Roger D.; Levasseur, Laurence Perreault; Wechsler, Risa H. [Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University, 452 Lomita Mall, Stanford, CA 94305-4085 (United States); Dalal, Neal; Wen, Di; Kemball, Athol; Vieira, Joaquin D. [Astronomy Department, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana IL 61801 (United States); Marrone, Daniel P. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Carlstrom, John E. [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Fassnacht, Christopher D. [Department of Physics, University of California, One Shields Avenue, Davis, CA 95616 (United States); Holder, Gilbert P. [Department of Physics, McGill University, 3600 Rue University, Montreal, Quebec H3A 2T8 (Canada); Marshall, Philip J. [Kavli Institute for Particle Astrophysics and Cosmology and Department of Particle Physics and Astrophysics, SLAC National Accelerator Laboratory, Menlo Park, CA 94305 (United States); Murray, Norman [CITA, University of Toronto, 60 St. George St., Toronto ON M5S 3H8 (Canada)

    2016-05-20

    We study the abundance of substructure in the matter density near galaxies using ALMA Science Verification observations of the strong lensing system SDP.81. We present a method to measure the abundance of subhalos around galaxies using interferometric observations of gravitational lenses. Using simulated ALMA observations we explore the effects of various systematics, including antenna phase errors and source priors, and show how such errors may be measured or marginalized. We apply our formalism to ALMA observations of SDP.81. We find evidence for the presence of a M = 10{sup 8.96±0.12} M {sub ⊙} subhalo near one of the images, with a significance of 6.9 σ in a joint fit to data from bands 6 and 7; the effect of the subhalo is also detected in both bands individually. We also derive constraints on the abundance of dark matter (DM) subhalos down to M ∼ 2 × 10{sup 7} M {sub ⊙}, pushing down to the mass regime of the smallest detected satellites in the Local Group, where there are significant discrepancies between the observed population of luminous galaxies and predicted DM subhalos. We find hints of additional substructure, warranting further study using the full SDP.81 data set (including, for example, the spectroscopic imaging of the lensed carbon monoxide emission). We compare the results of this search to the predictions of ΛCDM halos, and find that given current uncertainties in the host halo properties of SDP.81, our measurements of substructure are consistent with theoretical expectations. Observations of larger samples of gravitational lenses with ALMA should be able to improve the constraints on the abundance of galactic substructure.

  2. Prototype Implementation of Web and Desktop Applications for ALMA Science Verification Data and the Lessons Learned

    Science.gov (United States)

    Eguchi, S.; Kawasaki, W.; Shirasaki, Y.; Komiya, Y.; Kosugi, G.; Ohishi, M.; Mizumoto, Y.

    2013-10-01

    ALMA is estimated to generate TB scale data during only one observation; astronomers need to identify which part of the data they are really interested in. We have been developing new GUI software for this purpose utilizing the VO interface: ALMA Web Quick Look System (ALMAWebQL) and ALMA Desktop Application (Vissage). The former is written in JavaScript and HTML5 generated from Java code by the Google Web Toolkit, and the latter is in pure Java. An essential point of our approach is how to reduce network traffic: we prepare, in advance, “compressed” FITS files of 2x2x1 (horizontal, vertical, and spectral directions, respectively) binning, 2 x 2 x 2 binning, 4 x 4 x 2 binning data, and so on. These files are hidden from users, and Web QL automatically chooses the proper one for each user operation. Through this work, we find that network traffic in our system is still a bottleneck towards TB scale data distribution. Hence we have to develop alternative data containers for much faster data processing. In this paper, we introduce our data analysis systems, and describe what we learned through the development.

  3. Centralized operations and maintenance planning at the Atacama Large Millimeter/submillimeter Array (ALMA)

    Science.gov (United States)

    Lopez, Bernhard; Whyborn, Nicholas D.; Guniat, Serge; Hernandez, Octavio; Gairing, Stefan

    2016-07-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) is a joint project between astronomical organizations in Europe, North America, and East Asia, in collaboration with the Republic of Chile. ALMA consists of 54 twelve-meter antennas and 12 seven-meter antennas operating as an aperture synthesis array in the (sub)millimeter wavelength range. Since the inauguration of the observatory back in March 2013 there has been a continuous effort to establish solid operations processes for effective and efficient management of technical and administrative tasks on site. Here a key aspect had been the centralized maintenance and operations planning: input is collected from science stakeholders, the computerized maintenance management system (CMMS) and from the technical teams spread around the world, then this information is analyzed and consolidated based on the established maintenance strategy, the observatory long-term plan and the short-term priorities definitions. This paper presents the high-level process that has been developed for the planning and scheduling of planned- and unplanned maintenance tasks, and for site operations like the telescope array reconfiguration campaigns. We focus on the centralized planning approach by presenting its genesis, its current implementation for the observatory operations including related planning products, and we explore the necessary next steps in order to fully achieve a comprehensive centralized planning approach for ALMA in steady-state operations.

  4. Alma y vida, el origen de un Fracaso Histórico

    Directory of Open Access Journals (Sweden)

    Raquel Arias Careaga

    1993-12-01

    Full Text Available El 9 de abril de 1902 se estrenaba en Madrid Alma y vida de don Benito Pérez Galdós. Es de suponer cierta expectación tras el éxito, y escándalo, de Electra. Pero Alma y vida no logró igualar la obra precedente. Algunos autores hablan de un rotundo fracasoI, otros de una buena acogida (Ángel Berenguer, p. 30. Lo cierto es que Galdós, en el prólogo a la edición de la obra, se queja del mal trato que le dio la crítica, aunque sin referirse a la acogida del público, cosa que sí había hecho en el prólogo de Los condenados. Más bien, el autor parece achacar el que su obra pasase bastante desapercibida ala labor descuidada de una crítica mal preparada. Cuáles fueron esas opiniones de los contemporáneos de Galdós acerca de su nueva obra es el primer acercamiento a Alma y vida que debemos hacer.

  5. Broadband MMIC LNAs for ALMA Band 2+3 With Noise Temperature Below 28 K

    Science.gov (United States)

    Cuadrado-Calle, David; George, Danielle; Fuller, Gary A.; Cleary, Kieran; Samoska, Lorene; Kangaslahti, Pekka; Kooi, Jacob W.; Soria, Mary; Varonen, Mikko; Lai, Richard; Mei, Xiaobing

    2017-05-01

    Recent advancements in transistor technology, such as the 35 nm InP HEMT, allow for the development of monolithic microwave integrated circuit (MMIC) low noise amplifiers (LNAs) with performance properties that challenge the hegemony of SIS mixers as leading radio astronomy detectors at frequencies as high as 116 GHz. In particular, for the Atacama Large Millimeter and Submillimeter Array (ALMA), this technical advancement allows the combination of two previously defined bands, 2 (67-90 GHz) and 3 (84-116 GHz), into a single ultra-broadband 2+3 (67-116 GHz) receiver. With this purpose, we present the design, implementation, and characterization of LNAs suitable for operation in this new ALMA band 2+3, and also a different set of LNAs for ALMA band 2. The best LNAs reported here show a noise temperature less than 250 K from 72 to 104 GHz at room temperature, and less than 28 K from 70 to 110 GHz at cryogenic ambient temperature of 20 K. To the best knowledge of the authors, this is the lowest wideband noise ever published in the 70-110 GHz frequency range, typically designated as W-band.

  6. Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): Fast-Scan Single-Dish Mapping

    Science.gov (United States)

    White, S. M.; Iwai, K.; Phillips, N. M.; Hills, R. E.; Hirota, A.; Yagoubov, P.; Siringo, G.; Shimojo, M.; Bastian, T. S.; Hales, A. S.; Sawada, T.; Asayama, S.; Sugimoto, M.; Marson, R. G.; Kawasaki, W.; Muller, E.; Nakazato, T.; Sugimoto, K.; Brajša, R.; Skokić, I.; Bárta, M.; Kim, S.; Remijan, A. J.; de Gregorio, I.; Corder, S. A.; Hudson, H. S.; Loukitcheva, M.; Chen, B.; De Pontieu, B.; Fleishmann, G. D.; Gary, D. E.; Kobelski, A.; Wedemeyer, S.; Yan, Y.

    2017-07-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope has commenced science observations of the Sun starting in late 2016. Since the Sun is much larger than the field of view of individual ALMA dishes, the ALMA interferometer is unable to measure the background level of solar emission when observing the solar disk. The absolute temperature scale is a critical measurement for much of ALMA solar science, including the understanding of energy transfer through the solar atmosphere, the properties of prominences, and the study of shock heating in the chromosphere. In order to provide an absolute temperature scale, ALMA solar observing will take advantage of the remarkable fast-scanning capabilities of the ALMA 12 m dishes to make single-dish maps of the full Sun. This article reports on the results of an extensive commissioning effort to optimize the mapping procedure, and it describes the nature of the resulting data. Amplitude calibration is discussed in detail: a path that uses the two loads in the ALMA calibration system as well as sky measurements is described and applied to commissioning data. Inspection of a large number of single-dish datasets shows significant variation in the resulting temperatures, and based on the temperature distributions, we derive quiet-Sun values at disk center of 7300 K at λ = 3 mm and 5900 K at λ = 1.3 mm. These values have statistical uncertainties of about 100 K, but systematic uncertainties in the temperature scale that may be significantly larger. Example images are presented from two periods with very different levels of solar activity. At a resolution of about 25'', the 1.3 mm wavelength images show temperatures on the disk that vary over about a 2000 K range. Active regions and plages are among the hotter features, while a large sunspot umbra shows up as a depression, and filament channels are relatively cool. Prominences above the solar limb are a common feature of the single-dish images.

  7. Revisiting Comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON) with ALMA Autocorrelations

    Science.gov (United States)

    Yukiko Palmer, Maureen; Cordiner, Martin; de Val-Borro, Miguel; Charnley, Steven B.; Mumma, Michael J.

    2017-10-01

    The Atacama Large Millimeter/submillimeter array (ALMA) is a powerful tool for high-resolution mapping, but as an interferometer it is insensitive to large-scale structures due to the lack of zero-spacing (autocorrelation/single-dish) measurements. This is especially limiting in studies of cometary comae, which can extend up to hundreds of arcseconds. In this work, we make use of ALMA autocorrelations, treating the entire ALMA array as a collection of single-dish telescopes, to study the large comae of comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON). This has significantly improved our spectral line sensitivity, allowing for the detection of new molecules in ISON's coma, including HCO+ and H(13C)N. We also present results from the combined use of ALMA autocorrelation (single dish) and cross-correlation (interferometric) data to create a more complete picture of the coma gas distribution in Lemmon. Since its initial detection in Hyakutake (Irvine et al. 1996), the origins of cometary HNC have been under investigation (Irvine et al. 1998; Rodgers & Charnley 2001, 2005; Lis et al. 2008). It might be produced from the degradation of a solid organic material. More measurements of the HNC parent scale length are needed to help understand the source of HNC. Using ALMA autocorrelation data, we follow up on the detection of HNC in comet Lemmon by Cordiner et al. (2014) and, assisted by newly-developed radiative transfer/excitation models, provide an analysis of its distribution in this comet.References: Irvine, W. M., Bockelee-Morvan, D., Lis, D. C., et al. 1996, Nature, 383, 418Irvine, W. M., Bergin, E. A., Dickens, J. E., et al. 1998, Nature, 393, 547; Rodgers, S. D., & Charnley, S. B. 2001, MNRAS, 323, 84; ---. 2005, MNRAS, 356, 1542; Lis, D. C., Bockelee-Morvan, D., Boissier, J., et al. 2008, ApJ, 675, 931; Cordiner, M. A., Remijan, A. J., Boissier, J., et al. 2014, ApJL, 792, L2Acknowledgments: NASA’s Astrobiology Program supported this work through the Goddard Center

  8. The complexity of Orion: an ALMA view. I. Data and first results

    Science.gov (United States)

    Pagani, L.; Favre, C.; Goldsmith, P. F.; Bergin, E. A.; Snell, R.; Melnick, G.

    2017-07-01

    Context. We wish to improve our understanding of the Orion central star formation region (Orion-KL) and disentangle its complexity. Aims: We collected data with ALMA during cycle 2 in 16 GHz of total bandwidth spread between 215.1 and 252.0 GHz with a typical sensitivity of 5 mJy/beam (2.3 mJy/beam from 233.4 to 234.4 GHz) and a typical beam size of 1.̋7 × 1.̋0 (average position angle of 89°). We produced a continuum map and studied the emission lines in nine remarkable infrared spots in the region including the hot core and the compact ridge, plus the recently discovered ethylene glycol peak. Methods: We present the data, and report the detection of several species not previously seen in Orion, including n- and I-propyl cyanide (C3H7CN), and the tentative detection of a number of other species including glycolaldehyde (CH2(OH)CHO). The first detections of gGg' ethylene glycol (gGg' (CH2OH)2) and of acetic acid (CH3COOH) in Orion are presented in a companion paper. We also report the possible detection of several vibrationally excited states of cyanoacetylene (HC3N), and of its 13C isotopologues. We were not able to detect the 16O18O line predicted by our detection of O2 with Herschel, due to blending with a nearby line of vibrationally excited ethyl cyanide. We do not confirm the tentative detection of hexatriynyl (C6H) and cyanohexatriyne (HC7N) reported previously, or of hydrogen peroxide (H2O2) emission. Results: We report a complex velocity structure only partially revealed before. Components as extreme as -7 and +19 km s-1 are detected inside the hot region. Thanks to different opacities of various velocity components, in some cases we can position these components along the line of sight. We propose that the systematically redshifted and blueshifted wings of several species observed in the northern part of the region are linked to the explosion that occurred 500 yr ago. The compact ridge, noticeably farther south displays extremely narrow lines ( 1 km s

  9. O De anima de Aristóteles e a concepção das faculdades da alma no Kitáb al-Nafs (Livro da Alma, de Anima de Ibn Sina (Avicena

    Directory of Open Access Journals (Sweden)

    Jamil Ibrahim Iskandar

    2011-01-01

    Full Text Available Este artigo apresenta uma comparação conceitual entre a obra De anima, de Aristóteles, e a concepção das faculdades da alma no Kitáb al-Nafs - edição árabe - (Livro da Alma, De anima, de Ibn Sina (Avicena, com o intuito de mostrar similitudes e influências de Aristóteles sobre o pensamento de Ibn Sina, nessa temática. Destaca, ainda, como e a época em que o estagirita foi recebido em terras do Islã, indicando o seu primeiro receptor, o filósofo Al-Kindi, assim como, de modo pormenorizado, uma comparação sobre a definição de alma dada pelos dois filósofos, e as três espécies de alma, com ênfase para o conceito de alma racional. Apresenta, também, a estrutura de cada uma das obras

  10. Urban quality of life and industrial project management: the case of Alcan aluminium smelter in Alma, Quebec, Canada

    International Nuclear Information System (INIS)

    Simard, M.

    2003-01-01

    This quality-of-life study involving the population of Alma (30 126 inhabitants) is part of a five-year, multidisciplinary research program entitled 'Modelisation du suivi des impacts sociaux de l'aluminerie Alma'. The goal of this research program is to document the social impacts arising from the establishment of the Alcan industrial mega-complex in Alma (see Map 1). The Alma smelter began operation in 2001. It employs 865 people and has a production capacity of 407 000 MT of aluminium ingots. The research program is being carried out in parallel with the project, rather than retroactively. Thus, various thematic reports have been published on topics such as the project's economic spin-off and changes in the housing and transportation sectors. More specifically, this study aims to gauge the perceptions of Alma residents regarding their quality of life as stakeholders. In order to ensure that the study produced a more accurate indication of the community's evolution and to tie the study in with the various phases of the implementation of this industrial mega-project, it was conducted in three parts, i.e., in 1998, 2000 and 2002, corresponding to the planning, construction and operation phases. (author)

  11. The Alma-Bacon County Story: A Model for Rural America. Committee Print, 92nd Congress, 2nd Session, July 24, 1972.

    Science.gov (United States)

    Nipp, Robert E.

    Designed to illustrate the revitalization process of a small rural community via use of the Model Cities Program, this case study of Alma-Bacon County, Georgia traces Alma-Bacon's: (1) historical background; (2) community development beginnings; (3) political development; (4) outstanding problems; and (5) development plans and accomplishments…

  12. The close circumstellar environment of Betelgeuse. V. Rotation velocity and molecular envelope properties from ALMA

    Science.gov (United States)

    Kervella, Pierre; Decin, Leen; Richards, Anita M. S.; Harper, Graham M.; McDonald, Iain; O'Gorman, Eamon; Montargès, Miguel; Homan, Ward; Ohnaka, Keiichi

    2018-01-01

    We observed Betelgeuse using ALMA's extended configuration in band 7 (f ≈ 340 GHz, λ ≈ 0.88 mm), resulting in a very high angular resolution of 18 mas. Using a solid body rotation model of the 28SiO(ν= 2, J = 8-7) line emission, we show that the supergiant is rotating with a projected equatorial velocity of νeqsini = 5.47 ± 0.25 km s-1 at the equivalent continuum angular radius Rstar = 29.50 ± 0.14 mas. This corresponds to an angular rotation velocity of ω sini = (5.6 ± 1.3) × 10-9 rad s-1. The position angle of its north pole is PA = 48.0 ± 3.5°. The rotation period of Betelgeuse is estimated to P/ sini = 36 ± 8 years. The combination of our velocity measurement with previous observations in the ultraviolet shows that the chromosphere is co-rotating with the star up to a radius of ≈ 10 au (45 mas or 1.5 × the ALMA continuum radius). The coincidence of the position angle of the polar axis of Betelgeuse with that of the major ALMA continuum hot spot, a molecular plume, and a partial dust shell (from previous observations) suggests that focused mass loss is currently taking place in the polar region of the star. We propose that this hot spot corresponds to the location of a particularly strong "rogue" convection cell, which emits a focused molecular plume that subsequently condenses into dust at a few stellar radii. Rogue convection cells therefore appear to be an important factor shaping the anisotropic mass loss of red supergiants.

  13. An ALMA [C II] Survey of 27 Quasars at z > 5.94

    Science.gov (United States)

    Decarli, Roberto; Walter, Fabian; Venemans, Bram P.; Bañados, Eduardo; Bertoldi, Frank; Carilli, Chris; Fan, Xiaohui; Farina, Emanuele Paolo; Mazzucchelli, Chiara; Riechers, Dominik; Rix, Hans-Walter; Strauss, Michael A.; Wang, Ran; Yang, Yujin

    2018-02-01

    We present a survey of the [C II] 158 μm line and underlying far-infrared (FIR) dust continuum emission in a sample of 27 z≳ 6 quasars using the Atacama Large Millimeter Array (ALMA) at ∼ 1\\prime\\prime resolution. The [C II] line was significantly detected (at > 5-σ) in 23 sources (85%). We find typical line luminosities of {L}[{{C}{{II}}]}={10}9-10 {L}ȯ , and an average line width of ∼385 {km} {{{s}}}-1. The [C II]-to-far-infrared luminosity ratios ([C II]/FIR) in our sources span one order of magnitude, highlighting a variety of conditions in the star-forming medium. Four quasar host galaxies are clearly resolved in their [C II] emission on a few kpc scales. Basic estimates of the dynamical masses of the host galaxies give masses between 2 × 1010 and 2 × 1011 {M}ȯ , i.e., more than an order of magnitude below what is expected from local scaling relations, given the available limits on the masses of the central black holes (> 3× {10}8 {M}ȯ , assuming Eddington-limited accretion). In stacked ALMA [C II] spectra of individual sources in our sample, we find no evidence of a deviation from a single Gaussian profile. The quasar luminosity does not strongly correlate with either the [C II] luminosity or equivalent width. This survey (with typical on-source integration times of 8 minutes) showcases the unparalleled sensitivity of ALMA at millimeter wavelengths, and offers a unique reference sample for the study of the first massive galaxies in the universe.

  14. A disrupted molecular torus around Eta Carinae as seen in 12CO with ALMA

    Science.gov (United States)

    Smith, Nathan; Ginsburg, Adam; Bally, John

    2018-03-01

    We present Atacama Large Millimeter Array (ALMA) observations of 12CO 2-1 emission from circumstellar material around the massive star Eta Carinae (η Car). These observations reveal new structural details about the cool equatorial torus located ˜4000 au from the star. The CO torus is not a complete azimuthal loop, but rather, is missing its near side, which appears to have been cleared away. The missing material matches the direction of apastron in the eccentric binary system, making it likely that η Car's companion played an important role in disrupting portions of the torus soon after ejection. Molecular gas seen in ALMA data aligns well with the cool dust around η Car previously observed in mid-infrared (IR) maps, whereas hot dust resides at the inner surface of the molecular torus. The CO also coincides with the spatial and velocity structure of near-IR H2 emission. Together, these suggest that the CO torus seen by ALMA is actually the pinched waist of the Homunculus polar lobes, which glows brightly because it is close to the star and warmer than the poles. The near side of the torus appears to be a blowout, associated with fragmented equatorial ejecta. We discuss implications for the origin of various features north-west of the star. CO emission from the main torus implies a total gas mass in the range of 0.2-1 M⊙ (possibly up to 5 M⊙ or more, although with questionable assumptions). Deeper observations are needed to constrain CO emission from the cool polar lobes.

  15. Kan strategien for primaer sundhedstjeneste genoplives 30 år efter Alma-Ata?

    DEFF Research Database (Denmark)

    Lund, Stine; Probst, Helene Bilsted; Bygbjerg, Ib

    2010-01-01

    Thirty years ago the Alma-Ata declaration on primary health care was developed. Implementation has been compounded by inadequate financing, changing disease patterns and immature health systems, and there is an ongoing discussion between selective and comprehensive primary health care supporters....... Globally, child mortality for under-five-year-olds has been reduced by 50%, but there are still large regional differences. This year the WHO development report is about revitalisation of the primary health care strategy. Recognition of this strategy may be the best instrument to improve health globally....

  16. Corpo e Alma em Foucault: Postulados para uma Metodologia da Psicologia

    OpenAIRE

    Fernando de Almeida Silveira; Reinaldo Furlan

    2003-01-01

    Michel Foucault destaca o corpo como expressão de poderes e de saberes que se articulam estrategicamente na história da sociedade ocidental. O corpo é, simultaneamente, agente e peça dentro de um jogo de forças presente em toda a rede social, que o torna depositário de marcas e de sinais que nele se inscrevem nesses embates, os quais, por sua vez, têm na corporeidade seu "campo de prova". E a alma surge como instrumento de atuação dos poderes/saberes sobre o corpo, no processo de constituição...

  17. ALMA observations of molecular absorption in four directions toward the Galactic bulge

    Science.gov (United States)

    Liszt, H.; Gerin, M.

    2018-02-01

    Context. Alma Cycle 3 observations serendipitously showed strong absorption from diffuse molecular gas in the Galactic bulge at -200 km s-1 51(3σ) for the bulge gas toward J1744 and 58 ± 9 and 64 ± 4 for the disk gas toward J1717 and J1744, respectively, all well above the value of 20-25 typical of the central molecular zone. Conclusions: The kinematics and chemistry of the bulge gas observed toward J1744 more nearly resemble that of gas in the Milky Way disk than in the central molecular zone.

  18. A young stellar cluster around a massive protostar revealed by ALMA

    OpenAIRE

    Girart, Josep Miquel; Carrasco-Gonzalez, C.; Anglada, G.; Curiel, S.

    2017-01-01

    Here we present 1.1 mm ALMA observations at a very high angular resolution of a high mass star forming region. The high angular resolution and high dynamic range allows to reveal a young stellar cluster of low mass YSO near a massive protostellar object. Most of the sources detected has no counterpart at other wavelengths (the IR is dominated by the bright emission of the massive/intermediate young stars, which mask the emission of the low mass YSO). A description of the properties of the low...

  19. Dos revistas similares pero distintas: “El Olivo” y “Alma100”

    Directory of Open Access Journals (Sweden)

    Carlos Arbelos

    2006-01-01

    Así aparecen dos revistas similares pero diferentes, si bien ambas se proponen la difusión y divulgación del flamenco, una El Olivo lo hace desde una perspectiva más tradicional y Alma100 lo aborda desde conceptos más ligados a lo que se ha denominado postmodernidad. La otra gran diferencia es que mientras la primera depende económicamente casi exclusivamente de una subvención institucional, la segunda lo hace desde los recursos propios que genera la publicidad que se inserta en la publicación

  20. U.S. and European ALMA Partners Sign Agreement Green Light for World's Most Powerful Radio Observatory

    Science.gov (United States)

    2003-02-01

    Dr. Rita Colwell, director of the U.S. National Science Foundation (NSF), and Dr. Catherine Cesarsky, director general of the European Southern Observatory (ESO), today signed a historic agreement jointly to construct and operate ALMA, the Atacama Large Millimeter Array, the world's largest and most powerful radio telescope operating at millimeter and sub-millimeter wavelengths. "With this agreement, we usher in a new age of research in astronomy," said Dr. Colwell. "By working together in this truly global partnership, the international astronomy community will be able to ensure the research capabilities needed to meet the long-term demands of our scientific enterprise, and we will be able to study and understand our Universe in ways that have previously been beyond our vision." ALMA Array Artist's Conception of ALMA Array in Compact Configuration (Click on Image for Larger Version) Other Images Available: Artist's conception of the antennas for the Atacama Large Millimeter Array Moonrise over ALMA test equipment near Cerro Chajnantor, Chile VertexRSI antenna at the VLA test site Dr. Cesarsky also commented, "This agreement signifies the start of a great project of contemporary astronomy and astrophysics. Representing Europe, and in collaboration with many laboratories and institutes on this continent, we together look forward toward wonderful research projects. With ALMA, we may learn how the earliest galaxies in the Universe really looked like, to mention but one of the many eagerly awaited opportunities with this marvelous facility." When complete in 2011, ALMA will be an array of 64, 12-meter radio antennas that will work together as one telescope to study millimeter and sub-millimeter wavelength light from space. These wavelengths of the electromagnetic spectrum, which cross the critical boundary between infrared and microwave radiation, hold the key to understanding such processes as planet and star formation, the formation of early galaxies and galaxy

  1. ALMA SCIENCE VERIFICATION DATA: MILLIMETER CONTINUUM POLARIMETRY OF THE BRIGHT RADIO QUASAR 3C 286

    International Nuclear Information System (INIS)

    Nagai, H.; Nakanishi, K.; Hada, K.; Paladino, R.; Hull, C. L. H.; Cortes, P.; Fomalont, E.; Moellenbrock, G.; Asada, K.

    2016-01-01

    We present full-polarization observations of the compact, steep-spectrum radio quasar 3C 286 made with the Atacama Large Millimeter and Submillimeter Array (ALMA) at 1.3 mm. These are the first full-polarization ALMA observations, which were obtained in the framework of Science Verification. A bright core and a south–west component are detected in the total intensity image, similar to previous centimeter images. Polarized emission is also detected toward both components. The fractional polarization of the core is about 17%; this is higher than the fractional polarization at centimeter wavelengths, suggesting that the magnetic field is even more ordered in the millimeter radio core than it is further downstream in the jet. The observed polarization position angle (or electric vector position angle (EVPA)) in the core is ∼39 ◦ , which confirms the trend that the EVPA slowly increases from centimeter to millimeter wavelengths. With the aid of multi-frequency VLBI observations, we argue that this EVPA change is associated with the frequency-dependent core position. We also report a serendipitous detection of a sub-mJy source in the field of view, which is likely to be a submillimeter galaxy.

  2. VizieR Online Data Catalog: ALMA 106GHz continuum observations in Chamaeleon I (Dunham+, 2016)

    Science.gov (United States)

    Dunham, M. M.; Offner, S. S. R.; Pineda, J. E.; Bourke, T. L.; Tobin, J. J.; Arce, H. G.; Chen, X.; di, Francesco J.; Johnstone, D.; Lee, K. I.; Myers, P. C.; Price, D.; Sadavoy, S. I.; Schnee, S.

    2018-02-01

    We obtained ALMA observations of every source in Chamaleon I detected in the single-dish 870 μm LABOCA survey by Belloche et al. (2011, J/A+A/527/A145), except for those listed as likely artifacts (1 source), residuals from bright sources (7 sources), or detections tentatively associated with YSOs (3 sources). We observed 73 sources from the initial list of 84 objects identified by Belloche et al. (2011, J/A+A/527/A145). We observed the 73 pointings using the ALMA Band 3 receivers during its Cycle 1 campaign between 2013 November 29 and 2014 March 08. Between 25 and 27 antennas were available for our observations, with the array configured in a relatively compact configuration to provide a resolution of approximately 2" FWHM (300 AU at the distance to Chamaeleon I). Each target was observed in a single pointing with approximately 1 minute of on-source integration time. Three out of the four available spectral windows were configured to measure the continuum at 101, 103, and 114 GHz, each with a bandwidth of 2 GHz, for a total continuum bandwidth of 6 GHz (2.8 mm) at a central frequency of 106 GHz. (2 data files).

  3. ALMA Observations of the Archetypal “Hot Core” That Is Not: Orion-KL

    Energy Technology Data Exchange (ETDEWEB)

    Orozco-Aguilera, M. T. [Instituto Nacional de Astrofísica, Óptica y Electrónica, Luis Enrique Erro 1, Tonantzintla, Puebla, México (Mexico); Zapata, Luis A. [Instituto de Radioastronomía y Astrofísica, UNAM, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacán, México (Mexico); Hirota, Tomoya [Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka-shi, Tokyo 181-8588 (Japan); Qin, Sheng-Li [Department of Astronomy, Yunnan University, and Key Laboratory of Astroparticle Physics of Yunnan Province, Kunming 650091 (China); Masqué, Josep M, E-mail: lzapata@crya.unam.mx [Departamento de Astronomía, Universidad de Guanajuato, Apdo. Postal 144, 36000 Guanajuato, México (Mexico)

    2017-09-20

    We present sensitive high angular resolution (∼0.″1–0.″3) continuum Atacama Large Millimeter/Submillimeter Array (ALMA) observations of the archetypal hot core located in the Orion Kleinmann-Low (KL) region. The observations were made in five different spectral bands (bands 3, 6, 7, 8, and 9) covering a very broad range of frequencies (149–658 GHz). Apart from the well-known millimeter emitting objects located in this region (Orion Source I and BN), we report the first submillimeter detection of three compact continuum sources (ALMA1–3) in the vicinities of the Orion-KL hot molecular core. These three continuum objects have spectral indices between 1.47 and 1.56, and brightness temperatures between 100 and 200 K at 658 GHz, suggesting that we are seeing moderate, optically thick dust emission with possible grain growth. However, as these objects are not associated with warm molecular gas, and some of them are farther out from the molecular core, we thus conclude that they cannot heat the molecular core. This result favors the hypothesis that the hot molecular core in Orion-KL core is heated externally.

  4. ALMA Observations of the Archetypal “Hot Core” That Is Not: Orion-KL

    International Nuclear Information System (INIS)

    Orozco-Aguilera, M. T.; Zapata, Luis A.; Hirota, Tomoya; Qin, Sheng-Li; Masqué, Josep M

    2017-01-01

    We present sensitive high angular resolution (∼0.″1–0.″3) continuum Atacama Large Millimeter/Submillimeter Array (ALMA) observations of the archetypal hot core located in the Orion Kleinmann-Low (KL) region. The observations were made in five different spectral bands (bands 3, 6, 7, 8, and 9) covering a very broad range of frequencies (149–658 GHz). Apart from the well-known millimeter emitting objects located in this region (Orion Source I and BN), we report the first submillimeter detection of three compact continuum sources (ALMA1–3) in the vicinities of the Orion-KL hot molecular core. These three continuum objects have spectral indices between 1.47 and 1.56, and brightness temperatures between 100 and 200 K at 658 GHz, suggesting that we are seeing moderate, optically thick dust emission with possible grain growth. However, as these objects are not associated with warm molecular gas, and some of them are farther out from the molecular core, we thus conclude that they cannot heat the molecular core. This result favors the hypothesis that the hot molecular core in Orion-KL core is heated externally.

  5. ALMA OBSERVATIONS OF THE OUTFLOW FROM SOURCE I IN THE ORION-KL REGION

    Energy Technology Data Exchange (ETDEWEB)

    Zapata, Luis A.; Rodriguez, Luis F.; Loinard, Laurent [Centro de Radioastronomia y Astrofisica, UNAM, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacan (Mexico); Schmid-Burgk, Johannes; Menten, Karl M. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, 53121 Bonn (Germany); Curiel, Salvador [Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Ap. 70-264, 04510 DF (Mexico)

    2012-07-20

    In this Letter, we present sensitive millimeter SiO (J = 5-4; {nu} = 0) line observations of the outflow arising from the enigmatic object Orion Source I made with the Atacama Large Millimeter/Submillimeter Array (ALMA). The observations reveal that at scales of a few thousand AU, the outflow has a marked 'butterfly' morphology along a northeast-southwest axis. However, contrary to what is found in the SiO and H{sub 2}O maser observations at scales of tens of AU, the blueshifted radial velocities of the moving gas are found to the northwest, while the redshifted velocities are in the southeast. The ALMA observations are complemented with SiO (J = 8-7; {nu} = 0) maps (with a similar spatial resolution) obtained with the Submillimeter Array. These observations also show a similar morphology and velocity structure in this outflow. We discuss some possibilities to explain these differences at small and large scales across the flow.

  6. Cross-polarization characterization of GORE—TEX© at ALMA band 9 frequencies

    Science.gov (United States)

    Candotti, M.; Baryshev, A. M.; Trappe, N. A.; Hesper, R.; Murphy, J. A.; Barkhol, J.

    2006-05-01

    GORE-TEX material, commonly used in radomes, is known to be transparent at microwave bands. In ALMA a thin GORE-TEX membrane will cover the aperture through which the RF beam enters the cabin at the primary vertex hole. Slabs of GORE-TEX are also generally employed in windows for intermediate temperature shields inside the cryostat. The purpose of these windows ideally is to allow the beam to pass through them without introducing any alteration to the beam properties. The main concern is RF loss, but also cross-polarization efficiency degradation. This paper will concentrate on the results we have obtained for ALMA band 9 (602-720 GHz), in relation of loss of cross-polarization efficiency of a linearly polarized beam passing through a GORE-TEX slab, depending on its orientation relative to the direction of polarization of the beam. In order to spot anisotropic behavior of the material under test, an ad hoc measurements set-up has been used. Systematic measurements of cross-polarization properties for different thicknesses of GORE-TEX slabs were undertaken. Cross-polarization information is given in relation of the relative angle between the incident beam polarization and the material under test.

  7. ALMA Maps of Dust and Warm Dense Gas Emission in the Starburst Galaxy IC 5179

    Energy Technology Data Exchange (ETDEWEB)

    Zhao Yinghe [Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011 (China); Lu, Nanyao; Xu, C. Kevin [National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing 100012 (China); Díaz-Santos, Tanio [Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago (Chile); Gao Yu [Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008 (China); Charmandaris, Vassilis [Department of Physics, University of Crete, GR-71003 Heraklion (Greece); Werf, Paul van der [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Zhang Zhi-Yu [Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Cao, Chen, E-mail: zhaoyinghe@ynao.ac.cn [School of Space Science and Physics, Shandong University at Weihai, Weihai, Shandong 264209 (China)

    2017-08-10

    We present our high-resolution (0.″15 × 0.″13, ∼34 pc) observations of the CO (6−5) line emission, which probes the warm and dense molecular gas, and the 434 μ m dust continuum emission in the nuclear region of the starburst galaxy IC 5179, conducted with the Atacama Large Millimeter Array (ALMA). The CO (6−5) emission is spatially distributed in filamentary structures with many dense cores and shows a velocity field that is characteristic of a circumnuclear rotating gas disk, with 90% of the rotation speed arising within a radius of ≲150 pc. At the scale of our spatial resolution, the CO (6−5) and dust emission peaks do not always coincide, with their surface brightness ratio varying by a factor of ∼10. This result suggests that their excitation mechanisms are likely different, as further evidenced by the southwest to northeast spatial gradient of both CO-to-dust continuum ratio and Pa- α equivalent width. Within the nuclear region (radius ∼ 300 pc) and with a resolution of ∼34 pc, the CO line flux (dust flux density) detected in our ALMA observations is 180 ± 18 Jy km s{sup −1} (71 ± 7 mJy), which accounts for 22% (2.4%) of the total value measured by Herschel .

  8. Probing the Gas Fueling and Outflows in Nearby AGN with ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Audibert, Anelise [Observatoire de Paris, LERMA, Centre National de la Recherche Scientifique, PSL University, Sorbonne University, UPMC, Paris (France); Combes, Françoise [Observatoire de Paris, LERMA, Centre National de la Recherche Scientifique, PSL University, Sorbonne University, UPMC, Paris (France); College de France, Paris (France); García-Burillo, Santiago [Observatorio Astronómico Nacional, Observatorio de Madrid, Madrid (Spain); Salomé, Philippe, E-mail: anelise.audibert@obspm.fr [Observatoire de Paris, LERMA, Centre National de la Recherche Scientifique, PSL University, Sorbonne University, UPMC, Paris (France)

    2017-12-12

    Feeding and feedback in AGN play a very important role to gain a proper understanding of galaxy formation and evolution. The interaction between activity mechanisms in the nucleus and its influence in the host galaxy are related to the physical processes involved in feedback and the gas fueling of the black hole. The discovery of many massive molecular outflows in the last few years have been promoting the idea that winds may be major actors in sweeping the gas out of galaxies. Also, the widely observed winds from the central regions of AGN are promising candidates to explain the scaling relations (e.g., the black hole-bulge mass relation, BH accretion rate tracking the star formation history) under the AGN feedback scenario. Out goal is to probe these phenomena through the kinematic and morphology of the gas inside the central kpc in nearby AGN. This has recently been possible due to the unprecedented ALMA spatial resolution and sensitivity. We present results on NGC7213 and NGC1808, the latter is part of a new ALMA follow-up of the NuGa project, a previous high-resolution (0.5–1″) CO survey of low luminosity AGN performed with the IRAM PdBI.

  9. Monitor and control system for ACA correlator based on PRIMERGY for ALMA project

    Science.gov (United States)

    Abe, Katsumi; Kawase, Sachiko; Moriya, Mitsuhiro

    2008-10-01

    The National Astronomical Observatory of Japan is constructing a large interferometer called the Atacama Large Millimeter/submillimeter Array (ALMA) ona plateau near the Atacama Desert in Chile at an elevation of about 5000 m, in cooperation with the National Radio Astronomy Observatory of the USA and the European Southern Observatory. In cooperation with FFC Limited, Fujitsu is taking charge of development of the Atacama Compact Array (ACA) correlator used in correlation processing of data collected with the interferometer. Fujitsu is also charged with developing the monitor and control system based on Fujitsu's Linux PRIMERGY servers. The PRIMERGY RX300 S3 used for this system must operate stably in a severe environment at an elevation of about 5000 m and under atmosperic pressure of about 0.5 atm. We employed a diskless system for stable operation, thus making the system reliable even at low atmospheric pressure. We also conducted long-time running tests in an environment similar to the Atacama high-altitude environment, and adopted a remote maintenance system in order to make error handling and recovery much easier. This paper briefly introduces the ALMA project, and then describes the means of stable monitor and control system operation.

  10. A união da alma e do intelecto na filosofia de Plotino

    Directory of Open Access Journals (Sweden)

    Bernardo G. S. L. Brandão

    2007-12-01

    Full Text Available Um dos aspectos mais importantes do sistema ético de Plotino é sua doutrina da união da alma e do Intelecto: essa união é o objetivo das práticas de purificação, o topo da prática dialética e a base da experiência mística. Mas, sendo inferior ao Intelecto, como é possível à alma alcançar essa união? Este artigo é uma tentativa de buscar a explicação plotiniana desse problema.One of the most important features of Plotinus' ethical system is his doctrine of the union between soul and Intellect: this union is the goal of purification procedures, the summit of dialectic practice and the basis of mystical experience. But, being inferior to Intellect, how is it possible for the soul to achieve this union? This paper is an attempt at searching for the plotinian explanation for this problem.

  11. RESOLVED IMAGES OF THE PROTOPLANETARY DISK AROUND HD 100546 WITH ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Pineda, Jaime E.; Quanz, Sascha P.; Meru, Farzana; Meyer, Michael R.; Avenhaus, Henning [Institute for Astronomy, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich (Switzerland); Mulders, Gijs D. [Lunar and Planetary Laboratory, The University of Arizona, 1629 E. University Blvd., Tucson, AZ 85721 (United States); Panić, Olja, E-mail: pjaime@phys.ethz.ch [Institute of Astronomy, Madingley Road, Cambridge CB3 0HA (United Kingdom)

    2014-06-20

    The disk around the Herbig Ae/Be star HD 100546 has been extensively studied and it is one of the systems for which there are observational indications of ongoing and/or recent planet formation. However, up until now, no resolved image of the millimeter dust emission or the gas has been published. We present the first resolved images of the disk around HD 100546 obtained in Band 7 with the ALMA observatory. The CO (3-2) image reveals a gas disk that extends out to 350 au radius at the 3σ level. Surprisingly, the 870 μm dust continuum emission is compact (radius <60 au) and asymmetric. The dust emission is well matched by a truncated disk with an outer radius of ≈50 au. The lack of millimeter-sized particles outside 60 au is consistent with radial drift of particles of this size. The protoplanet candidate, identified in previous high-contrast NACO/VLT L' observations, could be related to the sharp outer edge of the millimeter-sized particles. Future higher angular resolution ALMA observations are needed to determine the detailed properties of the millimeter emission and the gas kinematics in the inner region (<2''). Such observations could also reveal the presence of a planet through the detection of circumplanetary disk material.

  12. ALMA observation of the disruption of molecular gas in M87

    Science.gov (United States)

    Simionescu, A.; Tremblay, G.; Werner, N.; Canning, R. E. A.; Allen, S. W.; Oonk, J. B. R.

    2018-04-01

    We present the results from Atacama Large Millimeter Array (ALMA) observations centred 40 arcsec (3 kpc in projection) south-east of the nucleus of M87. We report the detection of extended CO (2-1) line emission with a total flux of (5.5 ± 0.6) × 10-18 erg s-1 cm-2 and corresponding molecular gas mass M_{H_2}=(4.7 ± 0.4) × 10^5 M_{⊙}, assuming a Galactic CO to H2 conversion factor. ALMA data indicate a line-of-sight velocity of -129 ± 3 km s-1, in good agreement with measurements based on the [C II] and H α+[N II] lines, and a velocity dispersion of σ = 27 ± 3 km s-1. The CO (2-1) emission originates only outside the radio lobe of the active galactic nucleus (AGN) seen in the 6 cm Very Large Array image, while the filament prolongs further inwards at other wavelengths. The molecular gas in M87 appears to be destroyed or excited by AGN activity, either by direct interaction with the radio plasma, or by the shock driven by the lobe into the X-ray emitting atmosphere. This is an important piece of the puzzle in understanding the impact of the central AGN on the amount of the coldest gas from which star formation can proceed.

  13. Interaction design challenges and solutions for ALMA operations monitoring and control

    Science.gov (United States)

    Pietriga, Emmanuel; Cubaud, Pierre; Schwarz, Joseph; Primet, Romain; Schilling, Marcus; Barkats, Denis; Barrios, Emilio; Vila Vilaro, Baltasar

    2012-09-01

    The ALMA radio-telescope, currently under construction in northern Chile, is a very advanced instrument that presents numerous challenges. From a software perspective, one critical issue is the design of graphical user interfaces for operations monitoring and control that scale to the complexity of the system and to the massive amounts of data users are faced with. Early experience operating the telescope with only a few antennas has shown that conventional user interface technologies are not adequate in this context. They consume too much screen real-estate, require many unnecessary interactions to access relevant information, and fail to provide operators and astronomers with a clear mental map of the instrument. They increase extraneous cognitive load, impeding tasks that call for quick diagnosis and action. To address this challenge, the ALMA software division adopted a user-centered design approach. For the last two years, astronomers, operators, software engineers and human-computer interaction researchers have been involved in participatory design workshops, with the aim of designing better user interfaces based on state-of-the-art visualization techniques. This paper describes the process that led to the development of those interface components and to a proposal for the science and operations console setup: brainstorming sessions, rapid prototyping, joint implementation work involving software engineers and human-computer interaction researchers, feedback collection from a broader range of users, further iterations and testing.

  14. ON THE NATURE OF THE TERTIARY COMPANION TO FW TAU: ALMA CO OBSERVATIONS AND SED MODELING

    Energy Technology Data Exchange (ETDEWEB)

    Caceres, Claudio; Hardy, Adam; Schreiber, Matthias R.; Cánovas, Héctor [Instituto de Física y Astronomía, Universidad de Valparaíso, Av. Gran Bretaña 1111, 2360102 Valparaíso (Chile); Cieza, Lucas A. [Núcleo de Astronomía, Universidad Diego Portales, Av. Ejército 441, Santiago (Chile); Williams, Jonathan P. [Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822 (United States); Hales, Antonio [Atacama Large Millimeter/Submillimeter Array, Joint ALMA Observatory, Alonso de Córdova 3107, Vitacura, 763-0355 Santiago (Chile); Pinte, Christophe [Univ. Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble (France); Ménard, Francois [UMI-FCA, CNRS/INSU, UMI 3386 (France); Wahhaj, Zahed [European Southern Observatory, Av. Alonso de Córdova 3107, Vitacura, 19001 Santiago (Chile)

    2015-06-20

    It is thought that planetary mass companions may form through gravitational disk instabilities or core accretion. Identifying such objects in the process of formation would provide the most direct test for the competing formation theories. One of the most promising candidates for a planetary mass object still in formation is the third object in the FW Tau system. We present here ALMA cycle 1 observations confirming the recently published 1.3 mm detection of a dust disk around this third object and present for the first time a clear detection of a single peak {sup 12}CO (2–1) line, providing direct evidence for the simultaneous existence of a gas disk. We perform radiative transfer modeling of the third object in FW Tau and find that current observations are consistent with either a brown dwarf embedded in an edge-on disk or a planet embedded in a low inclination disk, which is externally irradiated by the binary companion. Further observations with ALMA, aiming for high SNR detections of non-contaminated gas lines, are required to conclusively unveil the nature of the third object in FW Tau.

  15. Gas Cavities inside Dust Cavities in Disks Inferred from ALMA Observations

    Science.gov (United States)

    van der Marel, Nienke; van Dishoeck, Ewine F.; Bruderer, Simon; Pinilla, Paola; van Kempen, Tim; Perez, Laura; Isella, Andrea

    2016-01-01

    Protoplanetary disks with cavities in their dust distribution, also named transitional disks, are expected to be in the middle of active evolution and possibly planet formation. In recent years, millimeter-dust rings observed by ALMA have been suggested to have their origin in dust traps, caused by pressure bumps. One of the ways to generate these is by the presence of planets, which lower the gas density along their orbit and create pressure bumps at the edge. We present spatially resolved ALMA Cycle 0 and Cycle 1 observations of CO and CO isotopologues of several famous transitional disks. Gas is found to be present inside the dust cavities, but at a reduced level compared with the gas surface density profile of the outer disk. The dust and gas emission are quantified using the physical-chemical modeling code DALI. In the majority of these disks we find clear evidence for a drop in gas density of at least a factor of 10 inside the cavity, whereas the dust density drops by at least a factor 1000. The CO isotopologue observations reveal that the gas cavities are significantly smaller than the dust cavities. These gas structures suggest clearing by one or more planetary-mass companions.

  16. Probing the Gas Fueling and Outflows in Nearby AGN with ALMA

    Directory of Open Access Journals (Sweden)

    Anelise Audibert

    2017-12-01

    Full Text Available Feeding and feedback in AGN play a very important role to gain a proper understanding of galaxy formation and evolution. The interaction between activity mechanisms in the nucleus and its influence in the host galaxy are related to the physical processes involved in feedback and the gas fueling of the black hole. The discovery of many massive molecular outflows in the last few years have been promoting the idea that winds may be major actors in sweeping the gas out of galaxies. Also, the widely observed winds from the central regions of AGN are promising candidates to explain the scaling relations (e.g., the black hole-bulge mass relation, BH accretion rate tracking the star formation history under the AGN feedback scenario. Out goal is to probe these phenomena through the kinematic and morphology of the gas inside the central kpc in nearby AGN. This has recently been possible due to the unprecedented ALMA spatial resolution and sensitivity. We present results on NGC7213 and NGC1808, the latter is part of a new ALMA follow-up of the NuGa project, a previous high-resolution (0.5–1″ CO survey of low luminosity AGN performed with the IRAM PdBI.

  17. Not letting the perfect be the enemy of the good: steps toward science-ready ALMA images

    Science.gov (United States)

    Kepley, Amanda A.; Donovan Meyer, Jennifer; Brogan, Crystal; Moullet, Arielle; Hibbard, John; Indebetouw, Remy; Mason, Brian

    2016-07-01

    Historically, radio observatories have placed the onus of calibrating and imaging data on the observer, thus restricting their user base to those already initiated into the mysteries of radio data or those willing to develop these skills. To expand its user base, the Atacama Large Millimeter/submillimeter Array (ALMA) has a high- level directive to calibrate users' data and, ultimately, to deliver scientifically usable images or cubes to principle investigators (PIs). Although an ALMA calibration pipeline is in place, all delivered images continue to be produced for the PI by hand. In this talk, I will describe on-going efforts at the Northern American ALMA Science Center to produce more uniform imaging products that more closely meet the PI science goals and provide better archival value. As a first step, the NAASC imaging group produced a simple imaging template designed to help scientific staff produce uniform imaging products. This script allowed the NAASC to maximize the productivity of data analysts with relatively little guidance by the scientific staff by providing a step-by-step guide to best practices for ALMA imaging. Finally, I will describe the role of the manually produced images in verifying the imaging pipeline and the on-going development of said pipeline. The development of the imaging template, while technically simple, shows how small steps toward unifying processes and sharing knowledge can lead to large gains for science data products.

  18. Musica Alma

    Directory of Open Access Journals (Sweden)

    F. J. du Toit

    1960-03-01

    Full Text Available Dit is gesê dat musiek ’n uiting is van persoonlike, en dus geestelike en maatskaplike, gevoelens. Die kultivering van musiekwaardering en om met genot musiek te kan hoor van verskillende tydperke en skole, en van wisselendegrade van ingewikkeldheid, kan dus alleen verruimend werk. Dit bring die luisteraar in noue aanraking met die gees van verskillende volkere en tydperke.

  19. La inmortalidad del alma: historia de un argumento político

    Directory of Open Access Journals (Sweden)

    Miguel Saralegui

    2014-01-01

    Full Text Available Se examina una cuestión fundamental y poco estudiada de la teología política: la relación entre la defensa de la inmortalidad del alma y el mantenimiento del orden público. Se realiza un recorrido histórico por autores como Pietro Pomponazzi y Tomás Moro, que aceptan motivos políticos para defenderla, y David Hume, quien considera que no existe ningún motivo político para mantener dicha relación. Por último, se analizan los argumentos esgrimidos para mostrar que su eficacia está condicionada por la situación histórica.

  20. From Alma Ata to the Global Fund: The history of international health policy

    Directory of Open Access Journals (Sweden)

    Italian Global Health Watch

    2008-01-01

    Full Text Available “Global Funds are like stars in the sky, you can see them, admire them, appreciate their abundance… but fail to touch them.” - Ministry of Health Official, Malawi Abstract The paper traces the evolution of international health policies and international health institutions, starting from the birth of the World Health Organization, the setting up of the Health for All target at the Alma Ata conference in 1978 and the rise of neo-liberal policies promoted by international financial institutions from 1980 to the present. The paper looks at different issues surrounding public-private partnerships and the setting up of the Global Fund to fight AIDS, Tuberculosis and Malaria and the influence of these institutions on the health systems in poor countries.

  1. ORIGIN AND KINEMATICS OF THE ERUPTIVE FLOW FROM XZ TAU REVEALED BY ALMA

    International Nuclear Information System (INIS)

    Zapata, Luis A.; Galván-Madrid, Roberto; Carrasco-González, Carlos; Palau, Aina; Rodríguez, Luis F.; Kurtz, Stan E.; Tafoya, Daniel; Loinard, Laurent; Curiel, Salvador

    2015-01-01

    We present high angular resolution (∼0.″94) 12 CO(1-0) Atacama Large Millimeter/submillimeter Array (ALMA) observations obtained during the 2014 long baseline campaign from the eruptive bipolar flow from the multiple XZ Tau stellar system discovered by the Hubble Space Telescope (HST). These observations reveal, for the first time, the kinematics of the molecular flow. The kinematics of the different ejections close to XZ Tau reveal a rotating and expanding structure with a southeast–northwest velocity gradient. The youngest eruptive bubbles unveiled in the optical HST images are inside of this molecular expanding structure. Additionally, we report a very compact and collimated bipolar outflow emanating from XZ Tau A, which indicates that the eruptive outflow is indeed originating from this object. The mass (3 × 10 −7 M ⊙ ) and energetics (E kin = 3 × 10 37 erg) for the collimated outflow are comparable to those found in molecular outflows associated with young brown dwarfs

  2. A bela alma e a estética goethiana do símbolo

    Directory of Open Access Journals (Sweden)

    Wilma Patricia Maas

    2011-08-01

    Full Text Available Pretende-se acompanhar o desenvolvimento do pensamento estético de Goethe entre os anos de 1780 e 1790 paralelamente a sua expressão no livro VI do romance Os anos de aprendizado de Wilhelm Meister (1795-1796, no qual se narra a trajetória da Bela Alma em direção ao progressivo abandono dos símbolos religiosos como suporte sensível da fé. Entende-se que a convivência de Goethe com Karl Philipp Moritz foi decisiva para a concepção dos ensaios “Sobre os objetos das artes plásticas” (1797 e “Imitação simples, maneira, estilo” (1789, fundamentais para a constituição do pensamento estético de Goethe à época.

  3. Platão e a cidade justa: poetas ilusionistas e potências da alma

    Directory of Open Access Journals (Sweden)

    Rachel Gazolla

    2007-12-01

    Full Text Available A censura que Platão faz à poesia na República apresenta dois ângulos que serão investigados neste texto: de um lado, a relação com a mímesis, considerada como necessária para o conhecimento pela via da phantasía; de outro, a relação do gênero epithymético da alma, com a crítica mais específica exposta no livro X.The censorship Plato directs against poetry in the Republic is investigated from two points of view in this article: on one hand, the perspective of mimesis, which is seen as necessary to achieve knowledge, through phantasía; on the other, the issue of the epithymetic genre of soul, which is part of the more specific criticism developed in book X.

  4. An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic Redshifts

    Science.gov (United States)

    Danielson, A. L. R.; Swinbank, A. M.; Smail, Ian; Simpson, J. M.; Casey, C. M.; Chapman, S. C.; da Cunha, E.; Hodge, J. A.; Walter, F.; Wardlow, J. L.; Alexander, D. M.; Brandt, W. N.; de Breuck, C.; Coppin, K. E. K.; Dannerbauer, H.; Dickinson, M.; Edge, A. C.; Gawiser, E.; Ivison, R. J.; Karim, A.; Kovacs, A.; Lutz, D.; Menten, K.; Schinnerer, E.; Weiß, A.; van der Werf, P.

    2017-05-01

    We present spectroscopic redshifts of {\\text{}}{S}870μ {{m}} ≳ 2 mJy submillimeter galaxies (SMGs), which have been identified from the ALMA follow-up observations of 870 μm detected sources in the Extended Chandra Deep Field South (the ALMA-LESS survey). We derive spectroscopic redshifts for 52 SMGs, with a median of z = 2.4 ± 0.1. However, the distribution features a high-redshift tail, with ˜23% of the SMGs at z≥slant 3. Spectral diagnostics suggest that the SMGs are young starbursts, and the velocity offsets between the nebular emission and UV ISM absorption lines suggest that many are driving winds, with velocity offsets of up to 2000 km s-1. Using the spectroscopic redshifts and the extensive UV-to-radio photometry in this field, we produce optimized spectral energy distributions (SEDs) using Magphys, and use the SEDs to infer a median stellar mass of {M}\\star = (6 ± 1)× 1010 M {}⊙ for our SMGs with spectroscopic redshift. By combining these stellar masses with the star formation rates (measured from the far-infrared SEDs), we show that SMGs (on average) lie a factor of ˜5 above the so-called “main sequence” at z˜ 2. We provide this library of 52 template fits with robust and uniquely well-sampled SEDs as a resource for future studies of SMGs, and also release the spectroscopic catalog of ˜2000 (mostly infrared-selected) galaxies targeted as part of the spectroscopic campaign.

  5. The Taurus Boundary of Stellar/Substellar (TBOSS) Survey. II. Disk Masses from ALMA Continuum Observations

    Science.gov (United States)

    Ward-Duong, K.; Patience, J.; Bulger, J.; van der Plas, G.; Ménard, F.; Pinte, C.; Jackson, A. P.; Bryden, G.; Turner, N. J.; Harvey, P.; Hales, A.; De Rosa, R. J.

    2018-02-01

    We report 885 μm ALMA continuum flux densities for 24 Taurus members spanning the stellar/substellar boundary with spectral types from M4 to M7.75. Of the 24 systems, 22 are detected at levels ranging from 1.0 to 55.7 mJy. The two nondetections are transition disks, though other transition disks in the sample are detected. Converting ALMA continuum measurements to masses using standard scaling laws and radiative transfer modeling yields dust mass estimates ranging from ∼0.3 to 20 M ⊕. The dust mass shows a declining trend with central object mass when combined with results from submillimeter surveys of more massive Taurus members. The substellar disks appear as part of a continuous sequence and not a distinct population. Compared to older Upper Sco members with similar masses across the substellar limit, the Taurus disks are brighter and more massive. Both Taurus and Upper Sco populations are consistent with an approximately linear relationship in M dust to M star, although derived power-law slopes depend strongly upon choices of stellar evolutionary model and dust temperature relation. The median disk around early-M stars in Taurus contains a comparable amount of mass in small solids as the average amount of heavy elements in Kepler planetary systems on short-period orbits around M-dwarf stars, with an order of magnitude spread in disk dust mass about the median value. Assuming a gas-to-dust ratio of 100:1, only a small number of low-mass stars and brown dwarfs have a total disk mass amenable to giant planet formation, consistent with the low frequency of giant planets orbiting M dwarfs.

  6. Rings and gaps in the disc around Elias 24 revealed by ALMA

    Science.gov (United States)

    Dipierro, G.; Ricci, L.; Pérez, L.; Lodato, G.; Alexander, R. D.; Laibe, G.; Andrews, S.; Carpenter, J. M.; Chandler, C. J.; Greaves, J. A.; Hall, C.; Henning, T.; Kwon, W.; Linz, H.; Mundy, L.; Sargent, A.; Tazzari, M.; Testi, L.; Wilner, D.

    2018-04-01

    We present Atacama Large Millimeter/sub-millimeter Array (ALMA) Cycle 2 observations of the 1.3-mm dust continuum emission of the protoplanetary disc surrounding the T Tauri star Elias 24 with an angular resolution of ˜0.2 arcsec (˜28 au). The dust continuum emission map reveals a dark ring at a radial distance of 0.47 arcsec (˜65 au) from the central star, surrounded by a bright ring at 0.58 arcsec (˜81 au). In the outer disc, the radial intensity profile shows two inflection points at 0.71 and 0.87 arcsec (˜99 and 121 au, respectively). We perform global three-dimensional smoothed particle hydrodynamic gas/dust simulations of discs hosting a migrating and accreting planet. Combining the dust density maps of small and large grains with three-dimensional radiative transfer calculations, we produce synthetic ALMA observations of a variety of disc models in order to reproduce the gap- and ring-like features observed in Elias 24. We find that the dust emission across the disc is consistent with the presence of an embedded planet with a mass of ˜0.7 MJ at an orbital radius of ˜ 60 au. Our model suggests that the two inflection points in the radial intensity profile are due to the inward radial motion of large dust grains from the outer disc. The surface brightness map of our disc model provides a reasonable match to the gap- and ring-like structures observed in Elias 24, with an average discrepancy of ˜5 per cent of the observed fluxes around the gap region.

  7. Black hole mass measurement using molecular gas kinematics: what ALMA can do

    Science.gov (United States)

    Yoon, Ilsang

    2017-04-01

    We study the limits of the spatial and velocity resolution of radio interferometry to infer the mass of supermassive black holes (SMBHs) in galactic centres using the kinematics of circum-nuclear molecular gas, by considering the shapes of the galaxy surface brightness profile, signal-to-noise ratios (S/Ns) of the position-velocity diagram (PVD) and systematic errors due to the spatial and velocity structure of the molecular gas. We argue that for fixed galaxy stellar mass and SMBH mass, the spatial and velocity scales that need to be resolved increase and decrease, respectively, with decreasing Sérsic index of the galaxy surface brightness profile. We validate our arguments using simulated PVDs for varying beam size and velocity channel width. Furthermore, we consider the systematic effects on the inference of the SMBH mass by simulating PVDs including the spatial and velocity structure of the molecular gas, which demonstrates that their impacts are not significant for a PVD with good S/N unless the spatial and velocity scale associated with the systematic effects are comparable to or larger than the angular resolution and velocity channel width of the PVD from pure circular motion. Also, we caution that a bias in a galaxy surface brightness profile owing to the poor resolution of a galaxy photometric image can largely bias the SMBH mass by an order of magnitude. This study shows the promise and the limits of ALMA observations for measuring SMBH mass using molecular gas kinematics and provides a useful technical justification for an ALMA proposal with the science goal of measuring SMBH mass.

  8. ALMA IMAGING OF THE CO (6-5) LINE EMISSION IN NGC 7130

    Energy Technology Data Exchange (ETDEWEB)

    Zhao, Yinghe [Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011 (China); Lu, Nanyao [National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing 100012 (China); Xu, C. Kevin; Appleton, Philip; Murphy, Eric [Infrared Processing and Analysis Center, California Institute of Technology 100-22, Pasadena, CA 91125 (United States); Gao, Yu [Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008 (China); Barcos-Munõz, Loreto [Department of Astronomy, University of Virginia, 530 McCormick Road, Charlottesville, VA 22904 (United States); Díaz-Santos, Tanio [Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago (Chile); Charmandaris, Vassilis [Department of Physics, University of Crete, GR-71003 Heraklion (Greece); Armus, Lee [Spitzer Science Center, California Institute of Technology, MS 220-6, Pasadena, CA 91125 (United States); Van der Werf, Paul [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Evans, Aaron [National Radio Astronomy Observatory, Charlottesville, VA 22904 (United States); Cao, Chen [School of Space Science and Physics, Shandong University at Weihai, Weihai, Shandong 264209 (China); Inami, Hanae, E-mail: zhaoyinghe@gmail.com [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States)

    2016-04-01

    In this paper, we report our high-resolution (0.″20 × 0.″14 or ∼70 × 49 pc) observations of the CO(6-5) line emission, which probes warm and dense molecular gas, and the 434 μm dust continuum in the nuclear region of NGC 7130, obtained with the Atacama Large Millimeter Array (ALMA). The CO line and dust continuum fluxes detected in our ALMA observations are 1230 ± 74 Jy km s{sup −1} and 814 ± 52 mJy, respectively, which account for 100% and 51% of their total fluxes. We find that the CO(6-5) and dust emissions are generally spatially correlated, but their brightest peaks show an offset of ∼70 pc, suggesting that the gas and dust emissions may start decoupling at this physical scale. The brightest peak of the CO(6-5) emission does not spatially correspond to the radio continuum peak, which is likely dominated by an active galactic nucleus (AGN). This, together with our additional quantitative analysis, suggests that the heating contribution of the AGN to the CO(6-5) emission in NGC 7130 is negligible. The CO(6-5) and the extinction-corrected Pa-α maps display striking differences, suggestive of either a breakdown of the correlation between warm dense gas and star formation at linear scales of <100 pc or a large uncertainty in our extinction correction to the observed Pa-α image. Over a larger scale of ∼2.1 kpc, the double-lobed structure found in the CO(6-5) emission agrees well with the dust lanes in the optical/near-infrared images.

  9. Implementing the concurrent operation of sub-arrays in the ALMA correlator

    Science.gov (United States)

    Amestica, Rodrigo; Perez, Jesus; Lacasse, Richard; Saez, Alejandro

    2016-07-01

    The ALMA correlator processes the digitized signals from 64 individual antennas to produce a grand total of 2016 correlated base-lines, with runtime selectable lags resolution and integration time. The on-line software system can process a maximum of 125M visibilities per second, producing an archiving data rate close to one sixteenth of the former (7.8M visibilities per second with a network transfer limit of 60 MB/sec). Mechanisms in the correlator hardware design make it possible to split the total number of antennas in the array into smaller subsets, or sub-arrays, such that they can share correlator resources while executing independent observations. The software part of the sub-system is responsible for configuring and scheduling correlator resources in such a way that observations among independent subarrays occur simultaneously while internally sharing correlator resources under a cooperative arrangement. Configuration of correlator modes through its CAN-bus interface and periodic geometric delay updates are the most relevant activities to schedule concurrently while observations happen at the same time among a number of sub-arrays. For that to work correctly, the software interface to sub-arrays schedules shared correlator resources sequentially before observations actually start on each sub-array. Start times for specific observations are optimized and reported back to the higher level observing software. After that initial sequential phase has taken place then simultaneous executions and recording of correlated data across different sub-arrays move forward concurrently, sharing the local network to broadcast results to other software sub-systems. The present paper presents an overview of the different hardware and software actors within the correlator sub-system that implement some degree of concurrency and synchronization needed for seamless and simultaneous operation of multiple sub-arrays, limitations stemming from the resource-sharing nature of the

  10. ALMA Discovery of Solar Umbral Brightness Enhancement at λ = 3 mm

    Energy Technology Data Exchange (ETDEWEB)

    Iwai, Kazumasa [Institute for Space-Earth Environmental Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, 464-8601 (Japan); Loukitcheva, Maria [Center for Solar-Terrestrial Research, New Jersey Institute of Technology, 323 Martin Luther King Boulevard, Newark, NJ 07102 (United States); Shimojo, Masumi [Chile Observatory, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan); Solanki, Sami K. [Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, D-37073 Göttingen (Germany); White, Stephen M., E-mail: k.iwai@isee.nagoya-u.ac.jp [Space Vehicles Directorate, Air Force Research Laboratory, Albuquerque, NM (United States)

    2017-06-01

    We report the discovery of a brightness enhancement in the center of a large sunspot umbra at a wavelength of 3 mm using the Atacama Large Millimeter/sub-millimeter Array (ALMA). Sunspots are among the most prominent features on the solar surface, but many of their aspects are surprisingly poorly understood. We analyzed a λ = 3 mm (100 GHz) mosaic image obtained by ALMA that includes a large sunspot within the active region AR12470, on 2015 December 16. The 3 mm map has a 300″ × 300″ field of view and 4.″9 × 2.″2 spatial resolution, which is the highest spatial resolution map of an entire sunspot in this frequency range. We find a gradient of 3 mm brightness from a high value in the outer penumbra to a low value in the inner penumbra/outer umbra. Within the inner umbra, there is a marked increase in 3 mm brightness temperature, which we call an umbral brightness enhancement. This enhanced emission corresponds to a temperature excess of 800 K relative to the surrounding inner penumbral region and coincides with excess brightness in the 1330 and 1400 Å slit-jaw images of the Interface Region Imaging Spectrograph ( IRIS ), adjacent to a partial lightbridge. This λ = 3 mm brightness enhancement may be an intrinsic feature of the sunspot umbra at chromospheric heights, such as a manifestation of umbral flashes, or it could be related to a coronal plume, since the brightness enhancement was coincident with the footpoint of a coronal loop observed at 171 Å.

  11. Perder e recuperar a alma: tendências recentes na psicologia social da religião norte-americana e européia

    Directory of Open Access Journals (Sweden)

    Paiva Geraldo José de

    2002-01-01

    Full Text Available A palavra alma, do vocabulário religioso e psicológico, desapareceu da linha-mestra da psicologia. Com ela desapareceu o conceito de uma instância essencial da realidade humana. Ao contrário das denotações que identificam alma, espírito e mente e contrapõem alma a corpo, parece possível restituir a articulação originária dessas palavras nas fontes hebraicas da Bíblia, nas expressões idiomáticas das línguas ocidentais e no vocabulário psicológico fundador. Não é o uso da palavra alma, mas a recusa de seu desemprego, que torna interessante para o psicoterapeuta a serviço da alma, a atenção para estudos recentes, norte-americanos e europeus, que tentam restituir à alma sua posição estrutural e dinâmica na psique.

  12. A IMAGEM CONTRA A PURA REPRESENTAÇÃO: CORPOS, ALMAS E COSMOPOLÍTICA NA AMAZÔNIA

    Directory of Open Access Journals (Sweden)

    Leif Grunewald

    2011-12-01

    Full Text Available Um olhar sobre a noção de alma, conforme apresentada em um conjunto de etnografias sobre povos ameríndios, nos revela uma curiosa relação entre ‘alma’ e ‘imagem’, tratando-as como imagens corporais muito particulares dotadas da capacidade de se relacionar com variados centros de agência não humanos. Estas relações, como se sabe, são perigosas, uma vez que se corre eminente o risco da alma ser capturada ou agredida por formas de alteridade não humanas. Isso, claro, de um lado. De outro, as mesmas relações têm papel importante no xamanismo e na nominação. Este ensaio pretende, então, ampliar a compreensão sobre que tipo de imagem é esta chamada de alma nas paisagens amazônicas e como ela pode ser concebida como uma imagem que se furta à representação do corpo físico.

  13. almaBTE : A solver of the space-time dependent Boltzmann transport equation for phonons in structured materials

    Science.gov (United States)

    Carrete, Jesús; Vermeersch, Bjorn; Katre, Ankita; van Roekeghem, Ambroise; Wang, Tao; Madsen, Georg K. H.; Mingo, Natalio

    2017-11-01

    almaBTE is a software package that solves the space- and time-dependent Boltzmann transport equation for phonons, using only ab-initio calculated quantities as inputs. The program can predictively tackle phonon transport in bulk crystals and alloys, thin films, superlattices, and multiscale structures with size features in the nm- μm range. Among many other quantities, the program can output thermal conductances and effective thermal conductivities, space-resolved average temperature profiles, and heat-current distributions resolved in frequency and space. Its first-principles character makes almaBTE especially well suited to investigate novel materials and structures. This article gives an overview of the program structure and presents illustrative examples for some of its uses. PROGRAM SUMMARY Program Title:almaBTE Program Files doi:http://dx.doi.org/10.17632/8tfzwgtp73.1 Licensing provisions: Apache License, version 2.0 Programming language: C++ External routines/libraries: BOOST, MPI, Eigen, HDF5, spglib Nature of problem: Calculation of temperature profiles, thermal flux distributions and effective thermal conductivities in structured systems where heat is carried by phonons Solution method: Solution of linearized phonon Boltzmann transport equation, Variance-reduced Monte Carlo

  14. Direct Imaging of the Water Snow Line at the Time of Planet Formation using Two ALMA Continuum Bands

    Science.gov (United States)

    Banzatti, A.; Pinilla, P.; Ricci, L.; Pontoppidan, K. M.; Birnstiel, T.; Ciesla, F.

    2015-12-01

    Molecular snow lines in protoplanetary disks have been studied theoretically for decades because of their importance in shaping planetary architectures and compositions. The water snow line lies in the planet formation region at ≲10 AU, and so far its location has been estimated only indirectly from spatially unresolved spectroscopy. This work presents a proof-of-concept method to directly image the water snow line in protoplanetary disks through its physical and chemical imprint on the local dust properties. We adopt a physical disk model that includes dust coagulation, fragmentation, drift, and a change in fragmentation velocities of a factor of 10 between dry silicates and icy grains as found by laboratory work. We find that the presence of a water snow line leads to a sharp discontinuity in the radial profile of the dust emission spectral index αmm due to replenishment of small grains through fragmentation. We use the ALMA simulator to demonstrate that this effect can be observed in protoplanetary disks using spatially resolved ALMA images in two continuum bands. We explore the model dependence on the disk viscosity and find that the spectral index reveals the water snow line for a wide range of conditions, with opposite trends when the emission is optically thin rather than thick. If the disk viscosity is low (αvisc structure with a minimum at αmm ˜ 2 in the optically thick regime, possibly similar to what has been measured with ALMA in the innermost region of the HL Tau disk.

  15. Chandra and ALMA observations of the nuclear activity in two strongly lensed star-forming galaxies

    Science.gov (United States)

    Massardi, M.; Enia, A. F. M.; Negrello, M.; Mancuso, C.; Lapi, A.; Vignali, C.; Gilli, R.; Burkutean, S.; Danese, L.; Zotti, G. De

    2018-02-01

    Aim. According to coevolutionary scenarios, nuclear activity and star formation play relevant roles in the early stages of galaxy formation. We aim at identifying them in high-redshift galaxies by exploiting high-resolution and high-sensitivity X-ray and millimeter-wavelength data to confirm the presence or absence of star formation and nuclear activity and describe their relative roles in shaping the spectral energy distributions and in contributing to the energy budgets of the galaxies. Methods: We present the data, model, and analysis in the X-ray and millimeter (mm) bands for two strongly lensed galaxies, SDP.9 (HATLAS J090740.0-004200) and SDP.11 (HATLAS J091043.1-000322), which we selected in the Herschel-ATLAS catalogs for their excess emission in the mid-IR regime at redshift ≳1.5. This emission suggests nuclear activity in the early stages of galaxy formation. We observed both of them with Chandra ACIS-S in the X-ray regime and analyzed the high-resolution mm data that are available in the ALMA Science Archive for SDP.9. By combining the information available in mm, optical, and X-ray bands, we reconstructed the source morphology. Results: Both targets were detected in the X-ray, which strongly indicates highly obscured nuclear activity. ALMA observations for SDP.9 for the continuum and CO(6-5) spectral line with high resolution (0.02 arcsec corresponding to 65 pc at the distance of the galaxy) allowed us to estimate the lensed galaxy redshift to a better accuracy than pre-ALMA estimates (1.5753 ± 0.0003) and to model the emission of the optical, millimetric, and X-ray band for this galaxy. We demonstrate that the X-ray emission is generated in the nuclear environment, which strongly supports that this object has nuclear activity. On the basis of the X-ray data, we attempt an estimate of the black hole properties in these galaxies. Conclusions: By taking advantage of the lensing magnification, we identify weak nuclear activity associated with high

  16. ALMA imaging of C2H emission in the disk of NGC 1068

    Science.gov (United States)

    García-Burillo, S.; Viti, S.; Combes, F.; Fuente, A.; Usero, A.; Hunt, L. K.; Martín, S.; Krips, M.; Aalto, S.; Aladro, R.; Ramos Almeida, C.; Alonso-Herrero, A.; Casasola, V.; Henkel, C.; Querejeta, M.; Neri, R.; Costagliola, F.; Tacconi, L. J.; van der Werf, P. P.

    2017-12-01

    Aims: We study the feedback of star formation and nuclear activity on the chemistry of molecular gas in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy, by analyzing whether the abundances of key molecular species such as ethynyl (C2H), which is a classical tracer of photon dominated regions (PDR), change in the different environments of the disk of the galaxy. Methods: We used the Atacama Large Millimeter Array (ALMA) to map the emission of the hyperfine multiplet of C2H(N = 1-0) and its underlying continuum emission in the central r ≃ 35″ (2.5 kpc) region of the disk of NGC 1068 with a spatial resolution 1.̋0 × 0.̋7 (≃ 50-70 pc). We used maps of the dust continuum emission obtained at 349 GHz by ALMA to derive the H2 gas column densities and combined these with the C2H map at matched spatial resolution to estimate the fractional abundance of this species. We developed a set of time-dependent chemical models, which include shocks, gas-phase PDRs, and gas-grain chemical models to determine the origin of the C2H gas. Results: A sizeable fraction of the total C2H line emission is detected from the r ≃ 1.3 kpc starburst (SB) ring, which is a region that concentrates the bulk of the recent massive star formation in the disk traced by the Paα emission complexes imaged by the Hubble Space Telescope (HST). However, the brightest C2H emission originates from a r ≃ 200 pc off-centered circumnuclear disk (CND), where evidence of a molecular outflow has been previously found in other molecular tracers imaged by ALMA. We also detect significant emission that connects the CND with the outer disk in a region that probes the interface between the molecular disk and ionized gas outflow out to r ≃ 400 pc. We derived the fractional abundances of C2H (X(C2H)) assuming local thermodynamic equilibrium (LTE) conditions and a set of excitation temperatures (Tex) constrained by the previous multiline CO studies of the galaxy. Our estimates range from X(C2H) ≃ a

  17. Peri physeos psyches: sobre a natureza da alma no Fedro de Platão

    Directory of Open Access Journals (Sweden)

    Maria Aparecida de Paiva Montenegro

    2010-12-01

    Full Text Available No passo 245c do Fedro de Platão, no contexto do segundo discurso de Sócrates (no qual ele compõe sua palinodia dirigida a Eros, o filósofo chama atenção para a importância de "se tornar explícita a natureza da alma, dos seus estados e atos, assim como indagar se esta natureza é humana ou divina". Pretendo mostrar que Platão, nesse diálogo, tenta fundamentar a natureza mista da alma: em parte racional em parte passional. Essa ambiguidade constitutiva mostra-se diretamente correlacionada àquelas referentes às formas de Amor, Loucura e Retórica abordadas ao longo do diálogo, à medida que estas podem ser tanto perniciosas quanto prodigiosas, a depender do modo como se as conduz. Nessa perspectiva, meu propósito é defender a presença, na filosofia pensada por Platão, de elementos passionais imprescindíveis ao sucesso de sua atividade, cabendo ao filósofo alcançar, por meio de uma formação apropriada, a maestria para reverter aquilo que pode mergulhá-lo na ignorância e, consequentemente, na escravidão e na infelicidade, naquilo que justamente irá conduzi-lo na direção oposta: a do amor à Sabedoria.In Plato's Phaedrus 245-c, when Socrates delivers his second speech (in which he composes his palinodia addressed to Eros, the philosopher calls attention to the importance of "first understanding the truth about the nature of the soul, divine or human, by examining what it does and what is done to it". I intend to point out that in this dialogue, Plato tries to found the mixed composition of the soul: partly rational, partly passionate. This constitutive ambiguity seems to be directly related to those different kinds of Love, Madness and Rhetoric examined in the dialogue, inasmuch as they could be either beneficial or harmful, depending on the way they are managed. Therefore, my purpose is to point that regarding philosophy as conceived by Plato, the appealing of passionate elements are quite indispensable for its successful

  18. Porting the ALMA Correlator Data Processor from hard real-time to plain Linux

    Science.gov (United States)

    Amestica, Rodrigo; Perez, Jesus; Saez, Alejandro

    2016-07-01

    The ALMA correlator back-end consists of a cluster of 16 computing nodes and a master collector/packager node. The mission of the cluster is to process time domain lags into auto-correlations and complex visibilities, integrate them for some configurable amount of time and package them into a workable data product. Computers in the cluster are organized such that individual workloads per node are kept within achievable levels for different observing modes and antennas in the array. Over the course of an observation the master node transmits enough state information to each involved computing node to specify exactly how to process each set of lags received from the correlator. For that distributed mechanism to work, it is necessary to unequivocally identify each individual lag set arriving at each computing node. The original approach was based on a custom hardware interface to each node in the cluster plus a realtime version of the Linux Operating System. A modification recently introduced in the ALMA correlator consists of tagging each lag set with a time stamp before delivering them to the cluster. The time stamp identifies a precise 16- millisecond window during which that specific data set was streamed to the computing cluster. From the time stamp value a node is able to identify a centroid (in absolute time units), base-lines, and correlator mode during that hardware integration. That is, enough information to let the digital signal processing pipeline in each node to process time domain lags into frequency domain auto-correlations per antenna and visibilities per base-line. The scheme also means that a good degree of concurrency can be achieved in each node by having individual CPU cores process individual lag sets at the same time, thus rendering enough processing power to cope with a maximum 1 GiB/sec output from the correlator. The present paper describes how we time stamp lag sets within the correlator hardware, the implications to their on

  19. Terahertz Desorption Emission Spectroscopy (THz DES) - ‘ALMA in the Lab’

    Science.gov (United States)

    Emile Auriacombe, Olivier Bruno Jacques; Fraser, Helen; Ellison, Brian; Ioppolo, Sergio; Rea, Simon

    2016-06-01

    ALMA is revolutionising our scope to identify and locate molecules that have been desorbed from ices, particularly complex organic molecules (COMS), which provide a vital link between interstellar and prebiotic chemistry. Explaining the existence of these molecules in star-forming regions relies on an empirical understanding of the chemistry that underpins their formation:- do COMS form predominantly in the solid-phase and then desorb to the gas phase, or do only “smaller” species, radials or ions desorb and then undergo gas-phase chemical reactions to generate larger COMS?-are the rotational state populations in COMS only attributable to equilibrium chemistry, or could their formation mechanisms and desorption processes affect the rotational state occupancy of these molecules, thereby directly tying certain species to solid-state origins?We have developed a novel laboratory method - THz Desorption Emission Spectroscopy (THz-DES) that combines “traditional” laboratory astrophysics high-vacuum ice experiments with a sensitive high-spectral-resolution terahertz total-power heterodyne radiometer 1,2, partially mirroring the spectral range of ALMA band 7 (275- 373 GHz). Ices are grown in situ on a cold-plate, situated in a vacuum cell, then (thermally) desorbed. The sub-mm emission spectra of the resultant gas-phase molecules are detected as a function of time, temperature, or distance from the surface. Our first THz DES results will be shown for pure and binary ice systems including H2O, N2O and CH3OH. They show good correlation with established methods e.g. TPD, with the advantage of exploiting the molecular spectroscopy to unravel surface dynamics, state-occupancy, and unequivocal molecular identification, as well as concurrently measuring desorption barriers and molecular yields. We will extend our technique to a broader frequency range, enabling us to detect radical and ion desorption, to differentiate between A and E populations of CH3OH or ortho

  20. A Community-Engaged Research Approach to Improve Mental Health Among Latina Immigrants: ALMA Photovoice.

    Science.gov (United States)

    Perez, Georgina; Della Valle, Pamela; Paraghamian, Sarah; Page, Rachel; Ochoa, Janet; Palomo, Fabiana; Suarez, Emilia; Thrasher, Angela; Tran, Anh N; Corbie-Smith, Giselle

    2016-05-01

    Recent Latina immigrants are at increased risk of poor mental health due to stressors associated with adapting to life in the United States. Existing social and health care policies often do not adequately address the mental health concerns of new Latino populations. Amigas Latinas Motivando el Alma, a community-partnered research project, seeks to improve immigrant Latinas' mental health outcomes. Using Photovoice methodology, promotoras (lay health advisors) reflected on community factors affecting mental health through photography and guided discussion. Discussions were audio-recorded, transcribed, and coded using content analysis to identify salient themes. Promotoras reviewed codes to develop themes that they presented in community forums to reach local policy makers and to increase community awareness. These forums included an exhibit of the promotoras' photographs and discussion of action steps to address community concerns. Themes included transitioning to life in the United States, parenting, education, and combating racism. Nearly 150 stakeholders attended the community forums and proposed responses to promotoras' photographic themes. Our findings suggest that Photovoice provides an opportunity for Latinas and the larger community to identify issues that they find most important and to explore avenues for action and change by creating sustainable partnerships between the community and forum attendees. © 2015 Society for Public Health Education.

  1. PROTOPLANETARY DISKS IN THE ORION OMC1 REGION IMAGED WITH ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Eisner, J. A.; Sheehan, P. D. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Bally, J. M. [Department of Astrophysical and Planetary Sciences, University of Colorado, UCB 389, Boulder, CO 80309 (United States); Ginsburg, A., E-mail: jeisner@email.arizona.edu [ESO Headquarters, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei Munchen (Germany)

    2016-07-20

    We present ALMA observations of the Orion Nebula that cover the OMC1 outflow region. Our focus in this paper is on compact emission from protoplanetary disks. We mosaicked a field containing ∼600 near-IR-identified young stars, around which we can search for sub-millimeter emission tracing dusty disks. Approximately 100 sources are known proplyds identified with the Hubble Space Telescope . We detect continuum emission at 1 mm wavelengths toward ∼20% of the proplyd sample, and ∼8% of the larger sample of near-IR objects. The noise in our maps allows 4 σ detection of objects brighter than ∼1.5 mJy, corresponding to protoplanetary disk masses larger than 1.5 M {sub J} (using standard assumptions about dust opacities and gas-to-dust ratios). None of these disks are detected in contemporaneous CO(2-1) or C{sup 18}O(2-1) observations, suggesting that the gas-to-dust ratios may be substantially smaller than the canonical value of 100. Furthermore, since dust grains may already be sequestered in large bodies in Orion Nebula cluster (ONC) disks, the inferred masses of disk solids may be underestimated. Our results suggest that the distribution of disk masses in this region is compatible with the detection rate of massive planets around M dwarfs, which are the dominant stellar constituent in the ONC.

  2. VizieR Online Data Catalog: ALMA galaxy properties in the COSMOS survey field (Scoville+, 2016)

    Science.gov (United States)

    Scoville, N.; Sheth, K.; Aussel, H.; vanden Bout, P.; Capak, P.; Bongiorno, A.; Casey, C. M.; Murchikova, L.; Koda, J.; Alvarez-Marquez, J.; Lee, N.; Laigle, C.; McCracken, H. J.; Ilbert, O.; Pope, A.; Sanders, D.; Chu, J.; Toft, S.; Ivison, R. J.; Manohar, S.

    2018-02-01

    Our sample of 145 galaxies is taken from the COSMOS 2 deg2 (Scoville et al. 2007ApJS..172....1S). This survey field has excellent photometric redshifts (Ilbert et al. 2013, J/A+A/556/A55; Laigle 2016, A&A submitted) derived from deep 34-band (UV-Mid IR) photometry. The galaxies were selected to sample stellar masses Mstellar in the range 0.2-4x1011Mȯ and the range of SFRs at each stellar mass. The ALMA Cycle 2 observations (#2013.1.00034.S) were obtained in 2014-2015. The z=1.15 and 2.2 samples were observed in Band 7 (345 GHz) and the z=4.4 sample in Band 6 (240 GHz). On-source integration times were ~2 minutes per galaxy and average rms sensitivities were 0.152 (Band 7) and 0.065 mJy/beam (Band 6). Synthesized beam sizes were ~0.6"-1". Data were calibrated and imaged with natural weighting using CASA. (3 data files).

  3. İnternet üzerinden satın alma niyetinin belirleyicileri

    OpenAIRE

    MOITAL, Miguel; VAUGHAN, Roger; EDWARDS, Jonathan; PERES, Rita

    2014-01-01

    İnternetin kullanılmaya başlamasından beri 10 yıldan uzun bir süre geçmiş olmasına karşın, seyahat ürünü satın almalarında internetin kullanımı açısından ülkeler arasında belirgin farklılıklar olduğu göze çarpmaktadır. Portekiz gibi bazı ülkelerde, seyahat ürünü satın almalarının sadece küçük bir oranı internet üzerinden yapılmaktadır. Bu çalışma, seyahat ürününü internet üzerinden satın alma niyetinin belirleyicilerini değerlendirerek, satın almalarda internet kullanımının daha iyi anlaşılma...

  4. An ALMA continuum survey of circumstellar disks in the upper Scorpius OB association

    Energy Technology Data Exchange (ETDEWEB)

    Carpenter, John M.; Ricci, Luca; Isella, Andrea [Department of Astronomy, California Institute of Technology, MC 249-17, Pasadena, CA 91125 (United States)

    2014-05-20

    We present ALMA 880 μm continuum observations of 20 K- and M-type stars in the Upper Scorpius OB association (Upper Sco) that are surrounded by protoplanetary disks. These data are used to measure the dust content in disks around low-mass stars (0.1-1.6 M {sub ☉}) at a stellar age of 5-11 Myr. Thirteen sources were detected in the 880 μm dust continuum at ≥3σ with inferred dust masses between 0.3 and 52 M {sub ⊕}. The dust masses tend to be higher around the more massive stars, but the significance is marginal in that the probability of no correlation is p ≈ 0.03. The evolution in the dust content in disks was assessed by comparing the Upper Sco observations with published continuum measurements of disks around ∼1-2 Myr stars in the Class II stage in the Taurus molecular cloud. While the dust masses in the Upper Sco disks are on average lower than in Taurus, any difference in the dust mass distributions is significant at less than 3σ. For stellar masses between 0.49 M {sub ☉} and 1.6 M {sub ☉}, the mean dust mass in disks is lower in Upper Sco relative to Taurus by Δlog M {sub dust} = 0.44 ± 0.26.

  5. Relationships between nutrients and chlorophyll a concentration in the international Alma Gol Wetland, Iran

    Directory of Open Access Journals (Sweden)

    Saeed Balali

    2013-05-01

    Full Text Available This study investigated the relationships between nutrients and chlorophyll, a concentration in the International Alma Gol Wetland. Chlorophyll a is the major photosynthetic pigment in lots of phytoplanktons and has been used as a trophy index in aquatic ecosystems. Water samples were collected fortnightly from five stations in the wetland during summer and autumn. Chlorophyll-a ranged between 4.38 to 156.55 mg/m3, sulfate ranged between 138 to 190 mg/l, total alkalinity ranged between 80 to 280 mg/l, silica ranged between 3.80 to 35.00 mg/l, phosphate ranged between 0.02 to 3.70 mg/l, ammonia ranged between 0.10 to 11.90 mg/l, nitrate ranged between 0.01 to 2.75 mg/l and nitrite ranged between 0.01 to 0.39 mg/l. There was a significant correlation between chlorophyll a and nitrate, nitrite and ammonia but there was no significant correlation between chlorophyll a and silica, total alkalinity, sulfate and phosphorus.

  6. ORIGIN AND KINEMATICS OF THE ERUPTIVE FLOW FROM XZ TAU REVEALED BY ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Zapata, Luis A.; Galván-Madrid, Roberto; Carrasco-González, Carlos; Palau, Aina; Rodríguez, Luis F.; Kurtz, Stan E.; Tafoya, Daniel; Loinard, Laurent [Centro de Radioastronomía y Astrofísica, UNAM, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacán, México (Mexico); Curiel, Salvador [Instituto de Astronomía, Universidad Nacional Autónoma de México, Ap. 70-264, 04510 DF, México (Mexico)

    2015-09-20

    We present high angular resolution (∼0.″94) {sup 12}CO(1-0) Atacama Large Millimeter/submillimeter Array (ALMA) observations obtained during the 2014 long baseline campaign from the eruptive bipolar flow from the multiple XZ Tau stellar system discovered by the Hubble Space Telescope (HST). These observations reveal, for the first time, the kinematics of the molecular flow. The kinematics of the different ejections close to XZ Tau reveal a rotating and expanding structure with a southeast–northwest velocity gradient. The youngest eruptive bubbles unveiled in the optical HST images are inside of this molecular expanding structure. Additionally, we report a very compact and collimated bipolar outflow emanating from XZ Tau A, which indicates that the eruptive outflow is indeed originating from this object. The mass (3 × 10{sup −7} M{sub ⊙}) and energetics (E{sub kin} = 3 × 10{sup 37} erg) for the collimated outflow are comparable to those found in molecular outflows associated with young brown dwarfs.

  7. Implementing Kanban for agile process management within the ALMA Software Operations Group

    Science.gov (United States)

    Reveco, Johnny; Mora, Matias; Shen, Tzu-Chiang; Soto, Ruben; Sepulveda, Jorge; Ibsen, Jorge

    2014-07-01

    After the inauguration of the Atacama Large Millimeter/submillimeter Array (ALMA), the Software Operations Group in Chile has refocused its objectives to: (1) providing software support to tasks related to System Integration, Scientific Commissioning and Verification, as well as Early Science observations; (2) testing the remaining software features, still under development by the Integrated Computing Team across the world; and (3) designing and developing processes to optimize and increase the level of automation of operational tasks. Due to their different stakeholders, each of these tasks presents a wide diversity of importances, lifespans and complexities. Aiming to provide the proper priority and traceability for every task without stressing our engineers, we introduced the Kanban methodology in our processes in order to balance the demand on the team against the throughput of the delivered work. The aim of this paper is to share experiences gained during the implementation of Kanban in our processes, describing the difficulties we have found, solutions and adaptations that led us to our current but still evolving implementation, which has greatly improved our throughput, prioritization and problem traceability.

  8. Isotopic Ratios of Carbon and Oxygen in Titan's CO Using Alma

    Science.gov (United States)

    Serigano, Joseph; Nixon, C. A.; Cordiner, M. A.; Irwin, P. G. J.; Teanby, N. A.; Charnley, S. B.; Lindberg, J. E.

    2016-01-01

    We report interferometric observations of carbon monoxide (CO) and its isotopologues in Titan's atmosphere using the Atacama Large Millimeter/submillimeter Array (ALMA). The following transitions were detected: CO (J = 1-0, 2-1, 3-2, 6-5), C-13 O (J = 2-1, 3-2, 6-5), C-18 O (J = 2-1, 3-2), and C-17 O (J = 3-2). Molecular abundances and the vertical atmospheric temperature profile were derived by modeling the observed emission line profiles using NEMESIS, a line-by-line radiative transfer code. We present the first spectroscopic detection of O-17 in the outer solar system with C-17 O detected at greater than 8 sigma confidence. The abundance of CO was determined to be 49.6 +/- 1.8 ppm, assumed to be constant with altitude, with isotopic ratios C-12/C-13 = 89.9 +/- 3.4, O-16/O-18 = 486 +/- 22, and O-16/O-17 = 2917 +/- 359. The measurements of C-12/C-13 and O-16/O-18 ratios are the most precise values obtained in Titan's atmospheric CO to date. Our results are in good agreement with previous studies and suggest no significant deviations from standard terrestrial isotopic ratios.

  9. Migration to Alma/Primo: A Case Study of Central Washington University

    Directory of Open Access Journals (Sweden)

    Ping Fu

    2015-12-01

    Full Text Available This paper describes how Central Washington University Libraries (CWUL interacted and collaborated with the Orbis Cascade Alliance (OCA Shared Integrated Library System’s (SILS Implementation Team and Ex Libris to process systems and data migration from Innovative Interfaces Inc.’s Millennium integrated library system to Alma/Primo, Ex Libris’ next-generation library management solution and discovery and delivery solution. A chronological review method was used for this case study to provide an overall picture of key migration events, tasks, and implementation efforts, including pre-migration cleanup, migration forms, integration with external systems, testing, cutover, post-migration cleanup, and reporting and fixing outstanding issues. A three-phase migration model was studied, and a questionnaire was designed to collect data from functional leads to determine staff time spent on the migration tasks. Staff time spent on each phase was analyzed and quantitated, with some top essential elements for the success of the migration identified through the case review and data analysis. An analysis of the Ex Libris’ Salesforce cases created during the migration and post-migration was conducted to be used for identifying roles of key librarians and staff functional leads during the migration.

  10. THE MOLECULAR WIND IN THE NEAREST SEYFERT GALAXY CIRCINUS REVEALED BY ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Zschaechner, Laura K.; Walter, Fabian; Farina, Emanuele P.; Kruijssen, J. M. Diederik [Max Planck Institute für Astronomie—Königstuhl 17, D-69117 Heidelberg (Germany); Bolatto, Alberto; Veilleux, Sylvain [Department of Astronomy and Joint Space Science Institute, University of Maryland, College Park, MD 20642 (United States); Leroy, Adam [Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Meier, David S. [Department of Physics, New Mexico Institute of Mining and Technology, 801 Leroy Place, Socorro, NM 87801 (United States); Ott, Jürgen, E-mail: zschaechner@mpia.de [National Radio Astronomy Observatory—P.O. Box O, 1003 Lopezville Road, Socorro, NM 87801 (United States)

    2016-12-01

    We present ALMA observations of the inner 1′ (1.2 kpc) of the Circinus galaxy, the nearest Seyfert. We target CO (1–0) in the region associated with a well-known multiphase outflow driven by the central active galactic nucleus (AGN). While the geometry of Circinus and its outflow make disentangling the latter difficult, we see indications of outflowing molecular gas at velocities consistent with the ionized outflow. We constrain the mass of the outflowing molecular gas to be 1.5 × 10{sup 5}−5.1 × 10{sup 6} M {sub ⊙}, yielding a molecular outflow rate of 0.35–12.3 M {sub ⊙} yr{sup −1}. The values within this range are comparable to the star formation (SF) rate in Circinus, indicating that the outflow indeed regulates SF to some degree. The molecular outflow in Circinus is considerably lower in mass and energetics than previously studied AGN-driven outflows, especially given its high ratio of AGN luminosity to bolometric luminosity. The molecular outflow in Circinus is, however, consistent with some trends put forth by Cicone et al., including a linear relation between kinetic power and AGN luminosity, as well as its momentum rate versus bolometric luminosity (although the latter places Circinus among the starburst galaxies in that sample). We detect additional molecular species including CN and C{sup 17}O.

  11. Magnetically regulated collapse in the B335 protostar? I. ALMA observations of the polarized dust emission

    Science.gov (United States)

    Maury, A. J.; Girart, J. M.; Zhang, Q.; Hennebelle, P.; Keto, E.; Rao, R.; Lai, S.-P.; Ohashi, N.; Galametz, M.

    2018-03-01

    The role of the magnetic field during protostellar collapse is poorly constrained from an observational point of view, although it could be significant if we believe state-of-the-art models of protostellar formation. We present polarimetric observations of the 233 GHz thermal dust continuum emission obtained with ALMA in the B335 Class 0 protostar. Linearly polarized dust emission arising from the circumstellar material in the envelope of B335 is detected at all scales probed by our observations, from radii of 50 to 1000 au. The magnetic field structure producing the dust polarization has a very ordered topology in the inner envelope, with a transition from a large-scale poloidal magnetic field, in the outflow direction, to strongly pinched in the equatorial direction. This is probably due to magnetic field lines being dragged along the dominating infall direction since B335 does not exhibit prominent rotation. Our data and their qualitative comparison to a family of magnetized protostellar collapse models show that, during the magnetized collapse in B335, the magnetic field is maintaining a high level of organization from scales 1000 au to 50 au: this suggests the field is dynamically relevant and capable of influencing the typical outcome of protostellar collapse, such as regulating the disk size in B335.

  12. VizieR Online Data Catalog: ALMA survey of protoplanetary disks in sigma Ori (Ansdell+, 2017)

    Science.gov (United States)

    Ansdell, M.; Williams, J. P.; Manara, C. F.; Miotello, A.; Facchini, S.; van der Marel, N.; Testi, L.; van Dishoeck, E. F.

    2017-08-01

    Our sample consists of the 92 Young Stellar Objects (YSOs) in σ Orionis with infrared excesses consistent with the presence of a protoplanetary disk. hese sources are identified by cross-matching the Class II and transition disk (TD) candidates from the Spitzer survey of Hernandez et al. 2007 (Cat. J/ApJ/662/1067) with the Mayrit catalog (Caballero 2008, Cat. J/A+A/478/667). Both catalogs are expected to be complete down to the brown dwarf limit. Disk classifications are based on the Spitzer/Infrared Array Camera (IRAC) Spectral Energy Distribution (SED) slope, as described in Hernandez et al. 2007 (Cat. J/ApJ/662/1067). We also include in our sample a Class I disk (source 1153), as it is located near the Spitzer/IRAC color cutoff for Class II disks. Our Band 6 Atacama Large Millimeter/sub-millimeter Array (ALMA) observations were obtained on 2016 July 30 and 31 during Cycle 3 (Project ID: 2015.1.00089.S; PI: Williams). The array configuration used 36 and 37 12m antennas on July 30 and 31, respectively, with baselines of 15-1124m on both runs. The correlator setup included two broadband continuum windows centered on 234.293 and 216.484GHz with bandwidths of 2.000 and 1.875GHz and channel widths of 15.625 and 0.976MHz, respectively. The bandwidth-weighted mean continuum frequency was 225.676GHz (1.33mm). The spectral windows covered the 12CO (230.538GHz), 13CO (220.399GHz), and C18O (219.560GHz) J=2-1 transitions at velocity resolutions of 0.16-0.17km/s. These spectral windows were centered on 230.531, 220.392, and 219.554GHz with bandwidths of 11.719MHz and channel widths of 0.122MHz. On-source integration times were 1.2 minutes per object for an average continuum rms of 0.15mJy/beam (Table1). This sensitivity was based on the James Clerk Maxwell Telescope (JCMT)/Submillimeter Common User Bolometer Array (SCUBA)-2 survey of σ Orionis disks by Williams et al. 2013 (Cat. J/MNRAS/435/1671), who found that stacking their individual non-detections revealed a mean 850

  13. THE ANATOMY OF AN EXTREME STARBURST WITHIN 1.3 Gyr OF THE BIG BANG REVEALED BY ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Carilli, C. L. [National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801 (United States); Riechers, D. [Astronomy Department, California Institute of Technology, MC 249-17, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Walter, F. [Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, D-69117 Heidelberg (Germany); Maiolino, R.; Lentati, L. [Astrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue, Cambridge CB3 0HE (United Kingdom); Wagg, J. [European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19 (Chile); McMahon, R. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Wolfe, A., E-mail: ccarilli@aoc.nrao.edu [Department of Physics and Center for Astrophysics and Space Sciences, University of California, San Diego, La Jolla, CA 92093 (United States)

    2013-02-15

    We present further analysis of the [C II] 158 {mu}m fine structure line and thermal dust continuum emission from the archetype extreme starburst/active galactic nucleus (AGN) group of galaxies in the early universe, BRI 1202-0725 at z = 4.7, using the Atacama Large Millimeter Array. The group has long been noted for having a closely separated (26 kpc in projection) FIR-hyperluminous quasar host galaxy and an optically obscured submillimeter galaxy (SMG). A short ALMA test observation reveals a rich laboratory for the study of the myriad processes involved in clustered massive galaxy formation in the early universe. Strong [C II] emission from the SMG and the quasar have been reported earlier by Wagg et al. based on these observations. In this paper, we examine in more detail the imaging results from the ALMA observations, including velocity channel images, position-velocity plots, and line moment images. We present detections of [C II] emission from two Ly{alpha}-selected galaxies in the group, demonstrating the relative ease with which ALMA can detect the [C II] emission from lower star formation rate galaxies at high redshift. Imaging of the [C II] emission shows a clear velocity gradient across the SMG, possibly indicating rotation or a more complex dynamical system on a scale {approx}10 kpc. There is evidence in the quasar spectrum and images for a possible outflow toward the southwest, as well as more extended emission (a {sup b}ridge{sup )}, between the quasar and the SMG, although the latter could simply be emission from Ly{alpha}-1 blending with that of the quasar at the limited spatial resolution of the current observations. These results provide an unprecedented view of a major merger of gas-rich galaxies driving extreme starbursts and AGN accretion during the formation of massive galaxies and supermassive black holes within 1.3 Gyr of the big bang.

  14. Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA

    Science.gov (United States)

    Sharda, P.; Federrath, C.; da Cunha, E.; Swinbank, A. M.; Dye, S.

    2018-04-01

    Using high-resolution (sub-kiloparsec scale) data obtained by ALMA, we analyze the star formation rate (SFR), gas content and kinematics in SDP 81, a gravitationally-lensed starburst galaxy at redshift 3. We estimate the SFR surface density (ΣSFR) in the brightest clump of this galaxy to be 357^{+135}_{-85} {M_{⊙}} yr^{-1} kpc^{-2}, over an area of 0.07 ± 0.02 kpc2. Using the intensity-weighted velocity of CO (5-4), we measure the turbulent velocity dispersion in the plane-of-the-sky and find σv, turb = 37 ± 5 km s-1 for the clump, in good agreement with previous estimates along the line of sight, corrected for beam smearing. Our measurements of gas surface density, freefall time and turbulent Mach number allow us to compare the theoretical SFR from various star formation models with that observed, revealing that the role of turbulence is crucial to explaining the observed SFR in this clump. While the Kennicutt Schmidt (KS) relation predicts an SFR surface density of Σ _{SFR,KS} = 52± 17 {M_{⊙}} yr^{-1} kpc^{-2}, the single-freefall model by Krumholz, Dekel and McKee (KDM) predicts Σ _{SFR,KDM} = 106± 37 {M_{⊙ }} yr^{-1} kpc^{-2}. In contrast, the multi-freefall (turbulence) model by Salim, Federrath and Kewley (SFK) gives Σ _{SFR,SFK} = 491^{+139 }_{-194} {M_{⊙ }} yr^{-1} kpc^{-2}. Although the SFK relation overestimates the SFR in this clump (possibly due to the negligence of magnetic fields), it provides the best prediction among the available models. Finally, we compare the star formation and gas properties of this galaxy to local star-forming regions and find that the SFK relation provides the best estimates of SFR in both local and high-redshift galaxies.

  15. ALMA Multiple-transition Observations of High-density Molecular Tracers in Ultraluminous Infrared Galaxies

    Science.gov (United States)

    Imanishi, Masatoshi; Nakanishi, Kouichiro; Izumi, Takuma

    2018-04-01

    We present the results of our ALMA observations of 11 (ultra)luminous infrared galaxies ((U)LIRGs) at J = 4–3 of HCN, HCO+, and HNC and J = 3–2 of HNC. This is an extension of our previously published HCN and HCO+ J = 3–2 observations to multiple rotational J-transitions of multiple molecules, to investigate how molecular emission line flux ratios vary at different J-transitions. We confirm that ultraluminous infrared galaxies (ULIRGs) that contain or may contain luminous obscured active galactic nuclei (AGNs) tend to show higher HCN-to-HCO+ flux ratios than starburst galaxies, both at J = 4–3 and J = 3–2. For selected HCN-flux-enhanced AGN-important ULIRGs, our isotopologue H13CN, H13CO+, and HN13C J = 3–2 line observations suggest a higher abundance of HCN than HCO+ and HNC, which is interpreted to be primarily responsible for the elevated HCN flux in AGN-important galaxies. For such sources, the intrinsic HCN-to-HCO+ flux ratios after line opacity correction will be higher than the observed ratios, making the separation between AGNs and starbursts even larger. The signature of the vibrationally excited (v 2 = 1f) HCN J = 4–3 emission line is seen in one ULIRG, IRAS 12112‑0305 NE. P Cygni profiles are detected in the HCO+ J = 4–3 and J = 3–2 lines toward IRAS 15250+3609, with an estimated molecular outflow rate of ∼250–750 M ⊙ yr‑1. The SiO J = 6–5 line also exhibits a P Cygni profile in IRAS 12112+0305 NE, suggesting the presence of shocked outflow activity. Shock tracers are detected in many sources, suggesting ubiquitous shock activity in the nearby ULIRG population.

  16. The ALMA early science view of FUor/EXor objects - V. Continuum disc masses and sizes

    Science.gov (United States)

    Cieza, Lucas A.; Ruíz-Rodríguez, Dary; Perez, Sebastian; Casassus, Simon; Williams, Jonathan P.; Zurlo, Alice; Principe, David A.; Hales, Antonio; Prieto, Jose L.; Tobin, John J.; Zhu, Zhaohuan; Marino, Sebastian

    2018-03-01

    Low-mass stars build a significant fraction of their total mass during short outbursts of enhanced accretion known as FUor and EXor outbursts. FUor objects are characterized by a sudden brightening of ˜5 mag at visible wavelengths within 1 yr and remain bright for decades. EXor objects have lower amplitude outbursts on shorter time-scales. Here we discuss a 1.3 mm Atacama Large Millimeter/submillimeter Array (ALMA) mini-survey of eight outbursting sources (three FUors, four EXors, and the borderline object V1647 Ori) in the Orion Molecular Cloud. While previous papers in this series discuss the remarkable molecular outflows observed in the three FUor objects and V1647 Ori, here we focus on the continuum data and the differences and similarities between the FUor and EXor populations. We find that FUor discs are significantly more massive (˜80-600 MJup) than the EXor objects (˜0.5-40 MJup). We also report that the EXor sources lack the prominent outflows seen in the FUor population. Even though our sample is small, the large differences in disc masses and outflow activity suggest that the two types of objects represent different evolutionary stages. The FUor sources seem to be rather compact (Rc < 20-40 au) and to have a smaller characteristic radius for a given disc mass when compared to T Tauri stars. V1118 Ori, the only known close binary system in our sample, is shown to host a disc around each one of the stellar components. The disc around HBC 494 is asymmetric, hinting at a structure in the outer disc or the presence of a second disc.

  17. The complexity of Orion: an ALMA view. II. gGg'-ethylene glycol and acetic acid

    Science.gov (United States)

    Favre, C.; Pagani, L.; Goldsmith, P. F.; Bergin, E. A.; Carvajal, M.; Kleiner, I.; Melnick, G.; Snell, R.

    2017-07-01

    We report the first detection and high angular resolution (1.8″× 1.1″) imaging of acetic acid (CH3COOH) and gGg'-ethylene glycol (gGg'(CH2OH)2) toward the Orion Kleinmann-Low (Orion-KL) nebula. The observations were carried out at 1.3 mm with ALMA during Cycle 2. A notable result is that the spatial distribution of the acetic acid and ethylene glycol emission differs from that of the other O-bearing molecules within Orion-KL. While the typical emission of O-bearing species harbors a morphology associated with a V-shape linking the hot core region to the compact ridge (with an extension toward the BN object), the emission of acetic acid and ethylene glycol mainly peaks at about 2'' southwest from the hot core region (near sources I and n). We find that the measured CH3COOH:aGg'(CH2OH)2 and CH3COOH:gGg'(CH2OH)2 ratios differ from those measured toward the low-mass protostar IRAS 16293-2422 by more than one order of magnitude. Our best hypothesis to explain these findings is that CH3COOH, aGg'(CH2OH)2, and gGg'(CH2OH)2 are formed on the icy surface of grains and are then released into the gas-phase via co-desorption with water, by way of a bullet of matter ejected during the explosive event that occurred in the heart of the nebula about 500-700 yr ago.

  18. Matching user needs to technology in dementia care: experiences with the Alma Supervisor Educational Program

    Directory of Open Access Journals (Sweden)

    Torhild Holthe

    2016-12-01

    Full Text Available The number of individuals with dementia in Norway is more than 78,000, and, as in all other European countries, this figure is expected to rise over the coming decades. The Norwegian Health Directorate encourages municipalities to make use of ‘welfare technology’ in order to contribute to independent living and quality of life in older adults, to increase the quality of community health care, to save time when providing community health services and to reduce costs, e.g. admission to a nursing home. Introducing welfare technology to care recipients requires innovation on the part of the community health care service with regard to increasing the competency of the staff in the operation of the technologies, as well as in establishing an infrastructure for ‘digital communication’. Research has shown that access to assistive technology may support individuals with mild cognitive impairments, as well as in an early phase of dementia. However, it is crucial that the technology addresses an identified need, and that the device is tailored to the person’s preferences and context. Therefore, it is important to train health professionals to assess the user’s needs and preferences and to identify resources and limitations in the particular context. Alma’s House in Oslo is a demonstration site and education center for welfare technologies. The education program for the certification of Alma supervisors has become an important strategy in educating occupational therapists (OTs and nurses on how to assess user needs, identify appropriate technology and implement this into the care recipient’s home.

  19. ALMA observations of lensed Herschel sources: testing the dark matter halo paradigm

    Science.gov (United States)

    Amvrosiadis, A.; Eales, S. A.; Negrello, M.; Marchetti, L.; Smith, M. W. L.; Bourne, N.; Clements, D. L.; De Zotti, G.; Dunne, L.; Dye, S.; Furlanetto, C.; Ivison, R. J.; Maddox, S. J.; Valiante, E.; Baes, M.; Baker, A. J.; Cooray, A.; Crawford, S. M.; Frayer, D.; Harris, A.; Michałowski, M. J.; Nayyeri, H.; Oliver, S.; Riechers, D. A.; Serjeant, S.; Vaccari, M.

    2018-04-01

    With the advent of wide-area submillimetre surveys, a large number of high-redshift gravitationally lensed dusty star-forming galaxies have been revealed. Because of the simplicity of the selection criteria for candidate lensed sources in such surveys, identified as those with S500 μm > 100 mJy, uncertainties associated with the modelling of the selection function are expunged. The combination of these attributes makes submillimetre surveys ideal for the study of strong lens statistics. We carried out a pilot study of the lensing statistics of submillimetre-selected sources by making observations with the Atacama Large Millimeter Array (ALMA) of a sample of strongly lensed sources selected from surveys carried out with the Herschel Space Observatory. We attempted to reproduce the distribution of image separations for the lensed sources using a halo mass function taken from a numerical simulation that contains both dark matter and baryons. We used three different density distributions, one based on analytical fits to the haloes formed in the EAGLE simulation and two density distributions [Singular Isothermal Sphere (SIS) and SISSA] that have been used before in lensing studies. We found that we could reproduce the observed distribution with all three density distributions, as long as we imposed an upper mass transition of ˜1013 M⊙ for the SIS and SISSA models, above which we assumed that the density distribution could be represented by a Navarro-Frenk-White profile. We show that we would need a sample of ˜500 lensed sources to distinguish between the density distributions, which is practical given the predicted number of lensed sources in the Herschel surveys.

  20. ALMA IMAGING OF HCN, CS, AND DUST IN ARP 220 AND NGC 6240

    Energy Technology Data Exchange (ETDEWEB)

    Scoville, Nick; Manohar, Swarnima; Murchikova, Lena [California Institute of Technology, MC 249-17, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Sheth, Kartik [North American ALMA Science Center, National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22901 (United States); Walter, Fabian; Zschaechner, Laura [Max-Planck-Institut fur Astronomie, Konigstuhl 17, D-69117 Heidelberg (Germany); Yun, Min [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Koda, Jin [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 (United States); Sanders, David; Barnes, Joshua [Institute for Astronomy, 2680 Woodlawn Drive, University of Hawaii, Honolulu, Hawaii, HI 96822 (United States); Thompson, Todd [Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Robertson, Brant; Tacconi, Linda; Narayanan, Desika [Department of Astronomy and Steward Observatory, University of Arizona, Tucson AZ 85721 (United States); Genzel, Reinhard; Davies, Richard [Max-Planck-Institut fur extraterrestrische Physik (MPE), Giessenbachstrasse, D-85748 Garching (Germany); Hernquist, Lars [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Brown, Robert [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22901 (United States); Hayward, Christopher C. [TAPIR 350-17, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Kartaltepe, Jeyhan [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); and others

    2015-02-10

    We report ALMA Band 7 (350 GHz) imaging at 0.''4-0.''6 resolution and Band 9 (696 GHz) at ∼0.''25 resolution of the luminous IR galaxies Arp 220 and NGC 6240. The long wavelength dust continuum is used to estimate interstellar medium masses for Arp 220 east and west and NGC 6240 of 1.9, 4.2, and 1.6 × 10{sup 9} M {sub ☉}within radii of 69, 65, and 190 pc. The HCN emission was modeled to derive the emissivity distribution as a function of radius and the kinematics of each nuclear disk, yielding dynamical masses consistent with the masses and sizes derived from the dust emission. In Arp 220, the major dust and gas concentrations are at radii less than 50 pc in both counter-rotating nuclear disks. The thickness of the disks in Arp 220 estimated from the velocity dispersion and rotation velocities are 10-20 pc and the mean gas densities are n{sub H{sub 2}}∼10{sup 5} cm{sup –3} at R <50 pc. We develop an analytic treatment for the molecular excitation (including photon trapping), yielding volume densities for both the HCN and CS emission with n {sub H2} ∼ 2 × 10{sup 5} cm{sup –3}. The agreement of the mean density from the total mass and size with that required for excitation suggests that the volume is essentially filled with dense gas, i.e., it is not cloudy or like swiss cheese.

  1. ALMA View of the Galactic Center Minispiral: Ionized Gas Flows around Sagittarius A∗

    Science.gov (United States)

    Tsuboi, Masato; Kitamura, Yoshimi; Uehara, Kenta; Miyawaki, Ryosuke; Tsutsumi, Takahiro; Miyazaki, Atsushi; Miyoshi, Makoto

    2017-06-01

    We have observed the “Galactic center minispiral (GCMS)” in the H42α recombination line as a part of the first large-scale mosaic observation in the Sagittarius A complex using Atacama Millimeter/submillimeter Array (ALMA). We revealed the kinematics of the ionized gas streamers of the GCMS. We found that the ionized gas streamers of the Northern Arm (NA) and Eastern Arm (EA) in their outer regions somewhat deviate from the Keplerian orbits that were derived previously from the trajectories in the inner regions. In addition, we found that the streamer corresponding to the Bar of the GCMS has a Keplerian orbit with an eccentricity of e∼ 0.8, which is independent from the Keplerian orbits of the other streamers of the GCMS. We estimated the LTE electron temperature and electron density in the ionized gas streamers. We confirmed the previously claimed tendency that the electron temperatures increase toward Sgr A*. We found that the electron density in the NA and EA also increases with approaching Sgr A* without the lateral expansion of the gas streamers. This suggests that there is some external pressure around the GCMS. The ambient ionized gas may cause the confinement and/or the perturbation of the orbits. There is a good positional correlation between the protostar candidates detected by JVLA at 34 GHz and the ionized gas streamer, the Northeastern Arm, newly found by our H42α recombination line observation. This suggests that the candidates had formed in the streamer and they were brought to near Sgr A* as the streamer falls.

  2. An ALMA Survey of CO Isotopologue Emission from Protoplanetary Disks in Chamaeleon I

    Energy Technology Data Exchange (ETDEWEB)

    Long Feng; Herczeg, Gregory J. [Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, Haidian Qu, 100871 Beijing (China); Pascucci, Ilaria; Apai, Daniel; Hendler, Nathan; Mulders, Gijs D. [Lunar and Planetary Laboratory, The University of Arizona, Tucson, AZ 85721 (United States); Drabek-Maunder, Emily; Mohanty, Subhanjoy [Imperial College London, London SW7 2AZ (United Kingdom); Testi, Leonardo [ESO/European Southern Observatory, Garching bei München (Germany); Henning, Thomas [Max Planck Institute for Astronomy, Heidelberg (Germany); Manara, Carlo F., E-mail: longfeng@pku.edu.cn [Scientific Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Noordwijk (Netherlands)

    2017-08-01

    The mass of a protoplanetary disk limits the formation and future growth of any planet. Masses of protoplanetary disks are usually calculated from measurements of the dust continuum emission by assuming an interstellar gas-to-dust ratio. To investigate the utility of CO as an alternate probe of disk mass, we use ALMA to survey {sup 13}CO and C{sup 18}O J = 3–2 line emission from a sample of 93 protoplanetary disks around stars and brown dwarfs with masses from in the nearby Chamaeleon I star-forming region. We detect {sup 13}CO emission from 17 sources and C{sup 18}O from only one source. Gas masses for disks are then estimated by comparing the CO line luminosities to results from published disk models that include CO freeze-out and isotope-selective photodissociation. Under the assumption of a typical interstellar medium CO-to-H{sub 2} ratio of 10{sup −4}, the resulting gas masses are implausibly low, with an average gas mass of ∼0.05 M {sub Jup} as inferred from the average flux of stacked {sup 13}CO lines. The low gas masses and gas-to-dust ratios for Cha I disks are both consistent with similar results from disks in the Lupus star-forming region. The faint CO line emission may instead be explained if disks have much higher gas masses, but freeze-out of CO or complex C-bearing molecules is underestimated in disk models. The conversion of CO flux to CO gas mass also suffers from uncertainties in disk structures, which could affect gas temperatures. CO emission lines will only be a good tracer of the disk mass when models for C and CO depletion are confirmed to be accurate.

  3. ALMA observations of lensed Herschel sources : Testing the dark-matter halo paradigm

    Science.gov (United States)

    Amvrosiadis, A.; Eales, S. A.; Negrello, M.; Marchetti, L.; Smith, M. W. L.; Bourne, N.; Clements, D. L.; De Zotti, G.; Dunne, L.; Dye, S.; Furlanetto, C.; Ivison, R. J.; Maddox, S.; Valiante, E.; Baes, M.; Baker, A. J.; Cooray, A.; Crawford, S. M.; Frayer, D.; Harris, A.; Michałowski, M. J.; Nayyeri, H.; Oliver, S.; Riechers, D. A.; Serjeant, S.; Vaccari, M.

    2018-01-01

    With the advent of wide-area submillimeter surveys, a large number of high-redshift gravitationally lensed dusty star-forming galaxies (DSFGs) has been revealed. Due to the simplicity of the selection criteria for candidate lensed sources in such surveys, identified as those with S500μm > 100 mJy, uncertainties associated with the modelling of the selection function are expunged. The combination of these attributes makes submillimeter surveys ideal for the study of strong lens statistics. We carried out a pilot study of the lensing statistics of submillimetre-selected sources by making observations with the Atacama Large Millimetre Array (ALMA) of a sample of strongly-lensed sources selected from surveys carried out with the Herschel Space Observatory. We attempted to reproduce the distribution of image separations for the lensed sources using a halo mass function taken from a numerical simulation which contains both dark matter and baryons. We used three different density distributions, one based on analytical fits to the halos formed in the EAGLE simulation and two density distributions (Singular Isothermal Sphere (SIS) and SISSA) that have been used before in lensing studies. We found that we could reproduce the observed distribution with all three density distributions, as long as we imposed an upper mass transition of ˜1013M⊙ for the SIS and SISSA models, above which we assumed that the density distribution could be represented by an NFW profile. We show that we would need a sample of ˜500 lensed sources to distinguish between the density distributions, which is practical given the predicted number of lensed sources in the Herschel surveys.

  4. Treinta años de Alma-Ata: Interpretaciones y consecuencias para el bienestar psicosocial y la salud comunitaria

    OpenAIRE

    Aguilar-Palacio, Isabel; Instituto Aragonés de Ciencias de la Salud (España)

    2009-01-01

    En este artículo se discute la experiencia de treinta años, desde que se presentó, en 1978, en la Conferencia Internacional de Alma-Ata, la nueva estrategia de la OMS de Atención Primaria de Salud. En esta, la OMS apostaba por un sistema integral basado en la equidad y en la participación comunitaria. Esta estrategia fue tachada de utópica, desarrollándose distintas interpretaciones de un mismo concepto, entre ellas, la Atención Primaria de Salud (APS) y la Atención Primaria Selectiva de Salu...

  5. Using ALMA to Resolve the Nature of the Early Star-Forming Large-Scale Structure G073

    Science.gov (United States)

    Hill, R.; Kneissl, R.; Polletta, M.; Clarenc, B.; Dole, H. A.; Nesvadba, N. P. H.; Scott, D.; Béthermin, M.; Lagache, G.; Montier, L.

    2017-07-01

    Galaxy clusters at large redshift are key targets for understanding the nature of the early Universe, yet locating them has proven to be very challenging. Recently, a large sample of over 2000 high-z candidate structures have been found using Planck's all-sky submillimetre maps, and a subset of 234 have been followed up with Herschel-SPIRE, which showed that the emission can be attributed to large far-infrared overdensities. However, the individual galaxies giving rise to the emission seen by Planck and Herschel have not yet been resolved nor characterized, so we do not yet know whether these sources are the progenitors of present-day, massive galaxy clusters. In an attempt to address this, we targeted the eight brightest Herschel-SPIRE peaks in the centre of the Planck peak G073.4-57.5 using ALMA at 1.3 mm, and complemented these observations with multi-wavelength data from Spitzer-IRAC at 3.6 and 4.5 μm and from CFHT-WIRCam at 1.2 and 2.2 μm. We also utilize data on G073.4-57.5 at 850 μm from JCMT's SCUBA-2 instrument. We detect a total of 18 millimetre galaxies brighter than 0.3mJy in 2.4arcmin2. In every case we are able to match these to their NIR counterparts, and while the most significant SCUBA-2 sources are not included in the ALMA pointings, we find an 8σ detection when stacking the ALMA source positions in the 850 μm data. We derive photometric redshifts, IR luminosities, star-formation rates, stellar masses, dust temperatures, and dust masses; the photometric redshifts are concentrated around z ≃ 1 and z ≃ 2 and the NIR colours show a "red" sequence, while the star-formation rates indicate that three of the galaxies are "starbursts". Serendipitous CO line detections of two of the galaxies appear to match their photometric redshifts with z = 2.05. We find that the ALMA source density is 8-30 times higher than average background estimates, and thus also larger than seen in typical "proto-cluster" fields. The evidence seems to be indicating the

  6. Kan strategien for primær sundhedstjeneste genoplives 30 år efter Alma-Ata?

    DEFF Research Database (Denmark)

    Lund, Stine; Probst, Helene Bilsted; Bygbjerg, Ib Christian

    2010-01-01

    Thirty years ago the Alma-Ata declaration on primary health care was developed. Implementation has been compounded by inadequate financing, changing disease patterns and immature health systems, and there is an ongoing discussion between selective and comprehensive primary health care supporters....... Globally, child mortality for under-five-year-olds has been reduced by 50%, but there are still large regional differences. This year the WHO development report is about revitalisation of the primary health care strategy. Recognition of this strategy may be the best instrument to improve health globally....

  7. Leibniz acerca de almas, corpos, agregados e substâncias na discussão com Fardella (1690

    Directory of Open Access Journals (Sweden)

    Edgar Marques

    2010-06-01

    Full Text Available Defendo neste artigo, contra a interpretação de Robert Adams, a tese de que, na discussão com Fardella (1690, Leibniz adota uma ontologia realista, segundo a qual seres vivos, e não almas, são substâncias.In this article, I sustain, against Robert Adam's interpretation, the thesis that Leibniz, in the discussion with Fardella (1690, adopts a realistic ontology, according to which live beings, instead of souls, are substances.

  8. Elefante asiático sometido al turismo: ¿Cuál es el precio por romper su alma?

    OpenAIRE

    García de Lorenzo, Maria; Iglesias Rodríguez, Carmen María

    2016-01-01

    El trabajo expuesto tiene como finalidad conocer el proceso de domesticación del elefante asiático para su uso en el turismo y ocio, así como las consecuencias físicas y etológicas que supone esta práctica sobre el animal. Se centra en el método ancestral utilizado en el sudeste asiático, “khedda”, que “rompe” su alma. Se hace una descripción breve de sus características físicas y su comportamiento para conocerlo un poco mejor

  9. O estatuto político da amizade: A Alma do Osso, de Cao Guimarães

    Directory of Open Access Journals (Sweden)

    Rafael de Almeida

    2013-06-01

    Full Text Available A partir do conceito de amizade proposto por Giorgio Agamben, este ensaio reflete, em uma interface entre estética e política, acerca das relações de poder presentes em A Alma do Osso (Cao Guimarães, 2004. O maior relevo é dado ao modo que o cineasta partilha, por meio do filme, sua existência com o ermitão Dominguinhos da Pedra, bem como as reverberações que isso garante à forma do documentário.

  10. The Anatomy of an Extreme Starburst within 1.3 Gyr of the Big Bang Revealed by ALMA

    Science.gov (United States)

    Carilli, C. L.; Riechers, D.; Walter, F.; Maiolino, R.; Wagg, J.; Lentati, L.; McMahon, R.; Wolfe, A.

    2013-02-01

    We present further analysis of the [C II] 158 μm fine structure line and thermal dust continuum emission from the archetype extreme starburst/active galactic nucleus (AGN) group of galaxies in the early universe, BRI 1202-0725 at z = 4.7, using the Atacama Large Millimeter Array. The group has long been noted for having a closely separated (26 kpc in projection) FIR-hyperluminous quasar host galaxy and an optically obscured submillimeter galaxy (SMG). A short ALMA test observation reveals a rich laboratory for the study of the myriad processes involved in clustered massive galaxy formation in the early universe. Strong [C II] emission from the SMG and the quasar have been reported earlier by Wagg et al. based on these observations. In this paper, we examine in more detail the imaging results from the ALMA observations, including velocity channel images, position-velocity plots, and line moment images. We present detections of [C II] emission from two Lyα-selected galaxies in the group, demonstrating the relative ease with which ALMA can detect the [C II] emission from lower star formation rate galaxies at high redshift. Imaging of the [C II] emission shows a clear velocity gradient across the SMG, possibly indicating rotation or a more complex dynamical system on a scale ~10 kpc. There is evidence in the quasar spectrum and images for a possible outflow toward the southwest, as well as more extended emission (a "bridge"), between the quasar and the SMG, although the latter could simply be emission from Lyα-1 blending with that of the quasar at the limited spatial resolution of the current observations. These results provide an unprecedented view of a major merger of gas-rich galaxies driving extreme starbursts and AGN accretion during the formation of massive galaxies and supermassive black holes within 1.3 Gyr of the big bang. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA

  11. ALMA 1.3 Millimeter Map of the HD 95086 System -- A Young Analog of the HR 8799 System

    Science.gov (United States)

    Su, Kate; MacGregor, Meredith Ann; Booth, Mark; Wilner, David; Malhotra, Renu; Morrison, Sarah; OST STDT

    2018-01-01

    Planets and minor bodies such as asteroids, Kuiper-belt objects and comets are integral components of a planetary system. Interactions among them leave clues about the formation process of a planetary system. The signature of such interactions is best illustrated through resolved observations of its debris disk. Here we present ALMA 1.3 mm observations of HD 95086, a young analog of the HR 8799 system, that hosts a directly imaged giant planet b and a massive debris disk with both asteroid- and Kuiper-belt analogs. The location of the Kuiper-belt analog is resolved for the first time. Our deep ALMA map also reveals a bright source located near the edge of the ring. The properties of the source, based on limited data, are consistent with it being a luminous star-forming galaxy at high redshift. We will discuss future, resolved observations of debris disks, highlighting the potential of the Origins Space Telescope (OST), one of the four science and technology definition studies commissioned by NASA Headquarters for the 2020 Astronomy and Astrophysics Decadal survey.

  12. ALMA FOLLOWS STREAMING OF DENSE GAS DOWN TO 40 pc FROM THE SUPERMASSIVE BLACK HOLE IN NGC 1097

    International Nuclear Information System (INIS)

    Fathi, Kambiz; Piñol-Ferrer, Nuria; Lundgren, Andreas A.; Wiklind, Tommy; Kohno, Kotaro; Izumi, Takuma; Martín, Sergio; Espada, Daniel; Hatziminaoglou, Evanthia; Imanishi, Masatoshi; Krips, Melanie; Matsushita, Satoki; Meier, David S.; Nakai, Naomasa; Sheth, Kartik; Turner, Jean; Van de Ven, Glenn

    2013-01-01

    We present a kinematic analysis of the dense molecular gas in the central 200 pc of the nearby galaxy NGC 1097, based on Cycle 0 observations with the Atacama Large Millimeter/submillimeter Array (ALMA). We use the HCN(4-3) line to trace the densest interstellar molecular gas (n H 2 ∼10 8 cm –3 ), and quantify its kinematics, and estimate an inflow rate for the molecular gas. We find a striking similarity between the ALMA kinematic data and the analytic spiral inflow model that we have previously constructed based on ionized gas velocity fields on larger scales. We are able to follow dense gas streaming down to 40 pc distance from the supermassive black hole in this Seyfert 1 galaxy. In order to fulfill marginal stability, we deduce that the dense gas is confined to a very thin disk, and we derive a dense gas inflow rate of 0.09 M ☉ yr –1 at 40 pc radius. Combined with previous values from the Hα and CO gas, we calculate a combined molecular and ionized gas inflow rate of ∼0.2 M ☉ yr –1 at 40 pc distance from the central supermassive black hole of NGC 1097.

  13. The ALMA view of the Antennae galaxy collision: How galaxy interaction triggers the formation of super star clusters

    Science.gov (United States)

    Herrera, Cinthya N.; Boulanger, François; Falgarone, Edith G.; Pineau Des Forêts, Guillaume; García-Burillo, Santiago; Iono, Daisuke; Guillard, Pierre

    The Antennae galaxies are a spectacular example of a burst of star formation triggered by the encounter of two galaxies, being an ideal source to understand how the dynamics of galaxy mergers drives star formation. We present archive ALMA CO(3-2) and VLT near-IR H2 spectro-imaging observations, and new ALMA 13CO(2-1) and dust continuum observations, at ~50 pc resolution. Combining tracers of density and velocity structure of the gas and its energetics, we demonstrate that star formation involves a complex interplay of merger-driven gas dynamics and turbulence, and the dissipation of the gas kinetic energy. We focus on a compact, bright H2 source, associated with cold molecular gas and dust continuum emission, located where the velocity gradient in the interaction region is observed to be the largest. The characteristics of this source suggest that we are witnessing the formation, initiated by turbulent dissipation, of a cloud massive enough (~4×106M⊙) to form a super star cluster within 1 Myr.

  14. DUYGUSAL ZEKA VE DÜRTÜSEL SATIN ALMA DAVRANIŞI İLİŞKİSİ

    OpenAIRE

    BÜYÜKER İŞLER, Didar; ATİLLA, Gaye

    2013-01-01

    Bireylerin kişilik özelliklerinin farklı olması tüketicilerin satın alma davranışında birbirinden farklı olmasında etkindir. İnsan davranışını yönlendiren biyolojik ve psikolojik etmenler de sürece eklendiğinde satın alma davranışı pekçok faktörün bombardımanı altında gerçekleşmektedir denilebilir. Fiziksel ve işlevsel faydaların ötesinde “duygu” son yıllarda pek çok alanda olduğu gibi tüketici davranışları konusunda önem kazanmaya başlamıştır. Duyguya hitap etmeyen bir ürünün satın alınabili...

  15. Gas density drops inside dust cavities of transitional disks around young stars observed with ALMA

    Science.gov (United States)

    van der Marel, N.; van Dishoeck, E. F.; Bruderer, S.; Pérez, L.; Isella, A.

    2015-07-01

    Context. Transitional disks with large dust cavities are important laboratories in which to study planet formation and disk evolution. Cold gas may still be present inside these cavities, but quantying this gas is challenging. The gas content is important for constraining the origin of the dust cavity. Aims: We use Atacama Large Millimeter/submillimeter Array (ALMA) observations of 12CO 6-5 and 690 GHz (Band 9) continuum of five well-studied transitional disks. In addition, we analyze previously published Band 7 observations of a disk in the 12CO 3-2 line and 345 GHz continuum. The observations are used to set constraints on the gas and dust surface density profiles, in particular, the drop δgas of the gas density inside the dust cavity. Methods: The physical-chemical modeling code DALI was used to simultaneously analyze the gas and dust images. We modeled SR21, HD 135344B, LkCa15, SR24S, and RX J1615-3255 (Band 9) and J1604-2130 (Band 7). The spectral energy distribution and continuum visibility curve constrain the dust surface density. Then we used the same model to calculate the 12CO emission, which we compared with the observations through spectra and intensity cuts. The amount of gas inside the cavity was quantified by varying the δgas parameter. Results: Model fits to the dust and gas indicate that gas is still present inside the dust cavity for all disks, but at a reduced level. The gas surface density drops inside the cavity by at least a factor 10, while the dust density drops by at least a factor 1000. Disk masses are comparable with previous estimates from the literature, cavity radii are found to be smaller than in the data obtained with the 345 GHz SubMillimeter Array. Conclusions: The derived gas surface density profiles suggest that the cavity was cleared by one or more companions in all cases, which trapped the millimeter-sized dust at the edge of the cavity. Appendix is available in electronic form at http://www.aanda.org

  16. Chemical segregation in hot cores with disk candidates. An investigation with ALMA

    Science.gov (United States)

    Allen, V.; van der Tak, F. F. S.; Sánchez-Monge, Á.; Cesaroni, R.; Beltrán, M. T.

    2017-07-01

    Context. In the study of high-mass star formation, hot cores are empirically defined stages where chemically rich emission is detected toward a massive YSO. It is unknown whether the physical origin of this emission is a disk, inner envelope, or outflow cavity wall and whether the hot core stage is common to all massive stars. Aims: We investigate the chemical makeup of several hot molecular cores to determine physical and chemical structure. We use high spectral and spatial resolution submillimeter observations to determine how this stage fits into the formation sequence of a high-mass star. Methods: The submillimeter interferometer ALMA (Atacama Large Millimeter Array) was used to observe the G35.20-0.74N and G35.03+0.35 hot cores at 350 GHz in Cycle 0. We analyzed spectra and maps from four continuum peaks (A, B1, B2 and B3) in G35.20-0.74N, separated by 1000-2000 AU, and one continuum peak in G35.03+0.35. We made all possible line identifications across 8 GHz of spectral windows of molecular emission lines down to a 3σ line flux of 0.5 K and determined column densities and temperatures for as many as 35 species assuming local thermodynamic equilibrium (LTE). Results: In comparing the spectra of the four continuum peaks, we find each has a distinct chemical composition expressed in over 400 different transitions. In G35.20, B1 and B2 contain oxygen- and sulfur-bearing organic and inorganic species but few nitrogen-bearing species whereas A and B3 are strong sources of O-, S-, and N-bearing organic and inorganic species (especially those with the CN bond). Column densities of vibrationally excited states are observed to be equal to or greater than the ground state for a number of species. Deuterated methyl cyanide is clearly detected in A and B3 with D/H ratios of 8 and 13%, respectively, but is much weaker at B1 and undetected at B2. No deuterated species are detected in G35.03, but similar molecular abundances to G35.20 were found in other species. We also

  17. De la definición de alma a las tesis sobre la diversidad de sus funciones con relación al cuerpo en Avicena

    Directory of Open Access Journals (Sweden)

    Miguel Alfredo Del Aguila

    2015-12-01

    Full Text Available En el presente trabajo nos detenemos en la relación alma-cuerpo en el contexto del Avicenna latinus, prestando especial atención a la definición de alma y a la diversificación de sus funciones en su relación con el cuerpo. Así, en la primera parte analizamos el dictamen de alma del pensador árabe en tanto y en cuanto nos la permita considerar -como bien Avicena lo hace remitiéndose a Aristóteles- elemento común a todos los niveles de vida; no a la manera de una realidad no-accidental añadida a un cuerpo constituido orgánicamente, sino como principio de organización del mismo, de sus funciones o potencias. Luego, exponemos la división y clasificación de las facultades y de las actividades del alma, gracias a las cuales podemos establecer un marco epistemológico que explique precisamente en parte lo que entiende por abstracción.

  18. ALMA observations of the nearby AGB star L2 Puppis : II. Gas disk properties derived from 12CO and 13CO J = 3-2 emission

    NARCIS (Netherlands)

    Homan, W.; Richards, A.; Decin, L.; Kervella, P.; de Koter, A.; McDonald, I.; Ohnaka, K.

    The circumstellar environment of the AGB star L2 Puppis was observed with ALMA in cycle 3, with a resolution of 15 × 18 mas. The molecular emission shows a differentially rotating disk, inclined to a nearly edge-on position. In the first paper in this series (Paper I) the molecular emission was

  19. Dualidade Corpo/Alma E A Exploração Do Trabalho No Modo De Produção Capitalista / Duality Body/Soul And Labor Exploitation In The Capitalist Production Mode

    OpenAIRE

    Vilas Boas, Lucas Guedes; Mestrando em Geografia - Universidade Federal de Juiz de Fora; Mourão Júnior, Carlos Alberto

    2015-01-01

    Por muitos séculos, o homem possuiu a crença que corpo e alma eram indissociáveis. Contudo, a tese dualística já apontada por Santo Agostinho e consolidada séculos depois com Descartes rompe com essa ideia da inseparabilidade do corpo e da alma. Inicialmente, tratar-se-á de como estes dois autores conceberam a dualidade corpo e mente em seus escritos. O presente trabalho almeja mostrar algumas das implicações da aceitação da teoria dualística entre corpo e alma no contexto científico-metafísi...

  20. Composição florística da floresta estacional decídua montana de Serra das Almas, CE, Brasil Flora of seasonal deciduous montane forest at Serra das Almas, Ceará State, Brazil

    Directory of Open Access Journals (Sweden)

    Jacira Rabelo Lima

    2009-09-01

    Full Text Available No domínio semi-árido brasileiro, a flora das bacias sedimentares ainda é pouco conhecida, mas os levantamentos já existentes indicam que há grande heterogeneidade florística e fisionômica. Mesmo áreas geográficas próximas podem apresentar dissimilaridade florística. Visando testar esta hipótese, a composição florística e o espectro biológico da floresta estacional decídua de Serra das Almas, estado do Ceará, foram analisados e comparados com os de 14 áreas sedimentares no Nordeste. Foram encontradas 104 espécies e 39 famílias em 1 ha analisado. Fabaceae, Euphorbiaceae, Erythroxylaceae e Myrtaceae foram as famílias com maior riqueza e fanerófitos a forma de vida predominante (87%. Arbóreas e arbustivas representaram 72% das espécies, trepadeiras 15%, subarbustos 6% e herbáceas 7%. A análise de agrupamento da composição dos fanerófitos, usando o índice de Jaccard e as médias de grupo a posteriori, indicou a formação de grupos florísticos entre áreas geográficas mais próximas. Porém, não foi significativo pelo teste de Mantel, o que demonstra a ocorrência de alta heterogeneidade florística mesmo entre áreas geográficas próximas. A flora da floresta da Serra das Almas apresentou maior semelhança com as formações encontradas no planalto da Ibiapaba.In the Brazilian semi-arid region, the flora in the sedimentary basins has been poorly studied, but the few surveys already done indicate great floristic and physiognomic heterogeneity. Even neighboring sites may be floristically different. To test this hypothesis, the floristic composition and the biological spectrum of the seasonal deciduous forest at Serra das Almas, Ceará, was analyzed and compared to those of 14 other northeastern Brazil sedimentary areas. A total of 104 species belonging to 40 families were found at the 1 ha site. Fabaceae, Euphorbiaceae, Erythroxylaceae and Myrtaceae were the families with the most species and phanerophytes the main

  1. Legados da consciência: estratégias para livrar a alma do "fogo do Purgatório"

    Directory of Open Access Journals (Sweden)

    Carlos Leonardo Kelmer Mathias

    2015-06-01

    Full Text Available O objetivo do presente artigo consiste em demonstrar como vários legados testamentários encerravam a estratégia, por parte do testador, de aliviar a consciência com vistas a obter a salvação da alma. O texto se valeu da análise qualitativa de testamentos de homens, mulheres, forros, forras, ricos, pobres e senhores de escravos arrolados a partir da pesquisa de 116 processos testamentários registrados no cartório do termo de Vila do Carmo, capitania de Minas Gerais, entre 1715 e 1778. Acerca dos legados, foram estudados os seguintes aspectos: heranças, paternidade, hierarquias, esmolas e créditos. Por fim, o texto conclui que, na medida em que tinham a finalidade de promover a paz do testador consigo mesmo, tais destinações podem ser definidas como legados da consciência.

  2. Histórias de almas e milagres: a religião nos filmes silenciosos pernambucanos

    Directory of Open Access Journals (Sweden)

    Luciana Sá Leitão Corrêa de Araújo

    2008-12-01

    Full Text Available A produção cinematográfica pernambucana ao longo da década de 1920 inclui alguns títulos nos quais a religião tem especial relevância. Neste artigo, analisamos os filmes História de uma alma (Eustórgio Wanderley, 1926, Revezes... (Chagas Ribeiro, 1927 e Destino das rosas (Ary Severo, 1930, procurando compreender como neles se insere o elemento religioso, o porquê dessa  recorrência e de que maneira está relacionada às particularidades do meio cinematográfico local, no que diz respeito à realização de filmes de enredo.

  3. Health for all beyond 2000: the demise of the Alma-Ata Declaration and primary health care in developing countries.

    Science.gov (United States)

    Hall, John J; Taylor, Richard

    2003-01-06

    Access to basic health services was affirmed as a fundamental human right in the Declaration of Alma-Ata in 1978. The model formally adopted for providing healthcare services was "primary health care" (PHC), which involved universal, community-based preventive and curative services, with substantial community involvement. PHC did not achieve its goals for several reasons, including the refusal of experts and politicians in developed countries to accept the principle that communities should plan and implement their own healthcare services. Changes in economic philosophy led to the replacement of PHC by "Health Sector Reform", based on market forces and the economic benefits of better health. It is time to abandon economic ideology and determine the methods that will provide access to basic healthcare services for all people.

  4. Inefficient jet-induced star formation in Centaurus A. High resolution ALMA observations of the northern filaments

    Science.gov (United States)

    Salomé, Q.; Salomé, P.; Miville-Deschênes, M.-A.; Combes, F.; Hamer, S.

    2017-12-01

    NGC 5128 (Centaurus A) is one of the best targets to study AGN feedback in the local Universe. At 13.5 kpc from the galaxy, optical filaments with recent star formation lie along the radio jet direction. This region is a testbed for positive feedback, here through jet-induced star formation. Atacama Pathfinder EXperiment (APEX) observations have revealed strong CO emission in star-forming regions and in regions with no detected tracers of star formation activity. In cases where star formation is observed, this activity appears to be inefficient compared to the Kennicutt-Schmidt relation. We used the Atacama Large Millimeter/submillimeter Array (ALMA) to map the 12CO(1-0) emission all along the filaments of NGC 5128 at a resolution of 1.3'' 23.8pc. We find that the CO emission is clumpy and is distributed in two main structures: (i) the Horseshoe complex, located outside the HI cloud, where gas is mostly excited by shocks and where no star formation is observed, and (ii) the Vertical filament, located at the edge of the HI shell, which is a region of moderate star formation. We identified 140 molecular clouds using a clustering method applied to the CO data cube. A statistical study reveals that these clouds have very similar physical properties, such as size, velocity dispersion, and mass, as in the inner Milky Way. However, the range of radius available with the present ALMA observations does not enable us to investigate whether or not the clouds follow the Larson relation. The large virial parameter αvir of the clouds suggests that gravity is not dominant and clouds are not gravitationally unstable. Finally, the total energy injection in the northern filaments of Centaurus A is of the same order as in the inner part of the Milky Way. The strong CO emission detected in the northern filaments is an indication that the energy injected by the jet acts positively in the formation of dense molecular gas. The relatively high virial parameter of the molecular clouds

  5. ESTUDO DE MANIFESTAÇÕES PATOLÓGICAS DO TERMINAL RODOVIÁRIO DE CRUZ DAS ALMAS - BA

    OpenAIRE

    Henrique Almeida Santana; Edvaldo Nascimento Conceição; Fernanda Nepomuceno Costa

    2016-01-01

    Patologia para a construção civil é entendido como a parte de engenharia que estuda os sintomas, causas e origens das lesões nas edificações. O Terminal Rodoviário da cidade de Cruz das Almas foi construído na década de oitenta, apresentando constante fluxo de veículos, com alta emissão de gás carbônico. Devido à aparência degradada da edificação, o presente trabalho teve como objetivo estudar as manifestações patológicas e determinar um prognóstico através de visita na edificação e revisão l...

  6. Gravitationally Unstable Condensations Revealed by ALMA in the TUKH122 Prestellar Core in the Orion A Cloud

    Science.gov (United States)

    Ohashi, Satoshi; Sanhueza, Patricio; Sakai, Nami; Kandori, Ryo; Choi, Minho; Hirota, Tomoya; Nguyễn-Lu’o’ng, Quang; Tatematsu, Ken’ichi

    2018-04-01

    We have investigated the TUKH122 prestellar core in the Orion A cloud using ALMA 3 mm dust continuum, N2H+ (J = 1‑0), and CH3OH ({J}K={2}K-{1}K) molecular-line observations. Previous studies showed that TUKH122 is likely on the verge of star formation because the turbulence is almost dissipated and chemically evolved among other starless cores in the Orion A cloud. By combining ALMA 12 m and ACA data, we recover extended emission with a resolution of ∼5″ corresponding to 0.01 pc and identify six condensations with a mass range of 0.1–0.4 M ⊙ and a radius of ≲0.01 pc. These condensations are gravitationally bound following a virial analysis and are embedded in the filament, including the elongated core with a mass of ∼29 M ⊙ and a radial density profile of r ‑1.6 derived by Herschel. The separation of these condensations is ∼0.035 pc, consistent with the thermal Jeans length at a density of 4.4 × 105 cm‑3. This density is similar to the central part of the core. We also find a tendency for the N2H+ molecule to deplete at the dust peak condensation. This condensation may be beginning to collapse because the line width becomes broader. Therefore, the fragmentation still occurs in the prestellar core by thermal Jeans instability, and multiple stars are formed within the TUKH122 prestellar core. The CH3OH emission shows a large shell-like distribution and surrounds these condensations, suggesting that the CH3OH molecule formed on dust grains is released into the gas phase by nonthermal desorption such as photoevaporation caused by cosmic-ray-induced UV radiation.

  7. VizieR Online Data Catalog: Redshift survey of ALMA-identified SMGs in ECDFS (Danielson+, 2017)

    Science.gov (United States)

    Danielson, A. L. R.; Swinbank, A. M.; Smail, I.; Simpson, J. M.; Casey, C. M.; Chapman, S. C.; da Cunha, E.; Hodge, J. A.; Walter, F.; Wardlow, J. L.; Alexander, D. M.; Brandt, W. N.; De Breuck, C.; Coppin, K. E. K.; Dannerbauer, H.; Dickinson, M.; Edge, A. C.; Gawiser, E.; Ivison, R. J.; Karim, A.; Kovacs, A.; Lutz, D.; Menten, K.; Schinnerer, E.; Weiss, A.; van der Werf, P.

    2017-11-01

    The 870um LESS survey (Weiss+ 2009, J/ApJ/707/1201) was undertaken using the LABOCA camera on APEX, covering an area of 0.5°x0.5° centered on the ECDFS. Follow-up observations of the LESS sources were carried out with ALMA (Hodge+ 2013, J/ApJ/768/91). In summary, observations for each source were taken between 2011 October and November in the Cycle 0 Project #2011.1.00294.S. To search for spectroscopic redshifts, we initiated an observing campaign using the the FOcal Reducer and low dispersion Spectrograph (FORS2) and VIsible MultiObject Spectrograph (VIMOS) on VLT (program 183.A-0666), but to supplement these observations, we also obtained observations with XSHOOTER on VLT (program 090.A-0927(A) from 2012 December 7-10), the Gemini Near-Infrared Spectrograph (GNIRS; program GN-2012B-Q-90) and the Multi-Object Spectrometer for Infra-Red Exploration (MOSFIRE) on the Keck I telescope (2012B_H251M, 2013BU039M, and 2013BN114M), all of which cover the near-infrared. As part of a spectroscopic campaign targeting Herschel-selected galaxies in the ECDFS, ALESS submillimeter galaxies (SMGs) were included on DEep Imaging Multi-Object Spectrograph (DEIMOS) slit masks on Keck II (program 2012B_H251). In total, we observed 109 out of the 131 ALESS SMGs in the combined main and supp samples. Spectroscopic redshifts for two of our SMGs, ALESS61.1 and ALESS65.1, were determined from serendipitous detections of the [CII]λ158um line in the ALMA band. See section 2.7. (2 data files).

  8. ALMA Reveals Sequential High-mass Star Formation in the G9.62+0.19 Complex

    Energy Technology Data Exchange (ETDEWEB)

    Liu, Tie; Kim, Kee-Tae [Korea Astronomy and Space Science Institute 776, Daedeokdae-ro, Yuseong-gu, Daejeon, Korea 34055 (Korea, Republic of); Lacy, John [Department of Astronomy, University of Texas at Austin, Austin, TX 78712 (United States); Li, Pak Shing [Astronomy Department, University of California, Berkeley, CA 94720 (United States); Wang, Ke [European Southern Observatory, Karl-Schwarzschild-Str.2, D-85748 Garching bei München (Germany); Qin, Sheng-Li [Department of Astronomy, Yunnan University, and Key Laboratory of Astroparticle Physics of Yunnan Province, Kunming, 650091 (China); Zhang, Qizhou [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Garay, Guido; Mardones, Diego [Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago (Chile); Wu, Yuefang [Department of Astronomy, Peking University, Beijing 100871 (China); Zhu, Qingfeng [Astronomy Department, University of Science and Technology, Chinese Academy of Sciences, Hefei 210008 (China); Tatematsu, Ken’ichi; Hirota, Tomoya [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Ren, Zhiyuan; Li, Di [National Astronomical Observatories, Chinese Academy of Science, A20 Datun Road, Chaoyang District, Beijing 100012 (China); Liu, Sheng-Yuan; Chen, Huei-Ru; Su, Yu-Nung, E-mail: liutiepku@gmail.com [Academia Sinica, Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 106, Taiwan (China)

    2017-11-01

    Stellar feedback from high-mass stars (e.g., H ii regions) can strongly influence the surrounding interstellar medium and regulate star formation. Our new ALMA observations reveal sequential high-mass star formation taking place within one subvirial filamentary clump (the G9.62 clump) in the G9.62+0.19 complex. The 12 dense cores (MM1–MM12) detected by ALMA are at very different evolutionary stages, from the starless core phase to the UC H ii region phase. Three dense cores (MM6, MM7/G, MM8/F) are associated with outflows. The mass–velocity diagrams of the outflows associated with MM7/G and MM8/F can be well-fit by broken power laws. The mass–velocity diagram of the SiO outflow associated with MM8/F breaks much earlier than other outflow tracers (e.g., CO, SO, CS, HCN), suggesting that SiO traces newly shocked gas, while the other molecular lines (e.g., CO, SO, CS, HCN) mainly trace the ambient gas continuously entrained by outflow jets. Five cores (MM1, MM3, MM5, MM9, MM10) are massive starless core candidates whose masses are estimated to be larger than 25 M {sub ☉}, assuming a dust temperature of ≤20 K. The shocks from the expanding H ii regions (“B” and “C”) to the west may have a great impact on the G9.62 clump by compressing it into a filament and inducing core collapse successively, leading to sequential star formation. Our findings suggest that stellar feedback from H ii regions may enhance the star formation efficiency and suppress low-mass star formation in adjacent pre-existing massive clumps.

  9. Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations

    Science.gov (United States)

    Scholtz, J.; Alexander, D. M.; Harrison, C. M.; Rosario, D. J.; McAlpine, S.; Mullaney, J. R.; Stanley, F.; Simpson, J.; Theuns, T.; Bower, R. G.; Hickox, R. C.; Santini, P.; Swinbank, A. M.

    2018-03-01

    We present sensitive 870 μm continuum measurements from our ALMA programmes of 114 X-ray selected active galactic nuclei (AGN) in the Chandra Deep Field-South and Cosmic Evolution Survey fields. We use these observations in combination with data from Spitzer and Herschel to construct a sample of 86 X-ray selected AGN, 63 with ALMA constraints at z = 1.5-3.2 with stellar mass >2 × 1010 M⊙. We constructed broad-band spectral energy distributions in the infrared band (8-1000 μm) and constrain star-formation rates (SFRs) uncontaminated by the AGN. Using a hierarchical Bayesian method that takes into account the information from upper limits, we fit SFR and specific SFR (sSFR) distributions. We explore these distributions as a function of both X-ray luminosity and stellar mass. We compare our measurements to two versions of the Evolution and Assembly of GaLaxies and their Environments (EAGLE) hydrodynamical simulations: the reference model with AGN feedback and the model without AGN. We find good agreement between the observations and that predicted by the EAGLE reference model for the modes and widths of the sSFR distributions as a function of both X-ray luminosity and stellar mass; however, we found that the EAGLE model without AGN feedback predicts a significantly narrower width when compared to the data. Overall, from the combination of the observations with the model predictions, we conclude that (1) even with AGN feedback, we expect no strong relationship between the sSFR distribution parameters and instantaneous AGN luminosity and (2) a signature of AGN feedback is a broad distribution of sSFRs for all galaxies (not just those hosting an AGN) with stellar masses above ≈1010 M⊙.

  10. Mapping jet-ISM interactions in X-ray binaries with ALMA: a GRS 1915+105 case study

    Science.gov (United States)

    Tetarenko, A. J.; Freeman, P.; Rosolowsky, E. W.; Miller-Jones, J. C. A.; Sivakoff, G. R.

    2018-03-01

    We present Atacama Large Millimetre/Sub-Millimetre Array (ALMA) observations of IRAS 19132+1035, a candidate jet-interstellar medium (ISM) interaction zone near the black hole X-ray binary (BHXB) GRS 1915+105. With these ALMA observations (combining data from the 12 m array and the Atacama Compact Array), we map the molecular line emission across the IRAS 19132+1035 region. We detect emission from the 12CO [J = 2 - 1], 13CO [ν = 0, J = 2 - 1], C18O [J = 2 - 1], H2CO [J = 30, 3 - 20, 2], H2CO [J = 32, 2 - 22, 1], H2CO [J = 32, 1 - 22, 0], SiO [ν = 0, J = 5 - 4], CH3OH [J = 42, 2 - 31, 2], and CS [ν = 0, J = 5 - 4] transitions. Given the morphological, spectral, and kinematic properties of this molecular emission, we present several lines of evidence that support the presence of a jet-ISM interaction at this site, including a jet-blown cavity in the molecular gas. This compelling new evidence identifies this site as a jet-ISM interaction zone, making GRS 1915+105, the third Galactic BHXB with at least one conclusive jet-ISM interaction zone. However, we find that this interaction occurs on much smaller scales than was postulated by previous work, where the BHXB jet does not appear to be dominantly powering the entire IRAS 19132+1035 region. Using estimates of the ISM conditions in the region, we utilize the detected cavity as a calorimeter to estimate the time-averaged power carried in the GRS 1915+105 jets of (8.4^{+7.7}_{-8.1})× 10^{32} erg s^{-1}. Overall, our analysis demonstrates that molecular lines are excellent diagnostic tools to identify and probe jet-ISM interaction zones near Galactic BHXBs.

  11. ALMA Observations of the IRDC Clump G34.43+00.24 MM3: DNC/HNC Ratio

    Science.gov (United States)

    Sakai, Takeshi; Sakai, Nami; Furuya, Kenji; Aikawa, Yuri; Hirota, Tomoya; Foster, Jonathan B.; Sanhueza, Patricio; Jackson, James M.; Yamamoto, Satoshi

    2015-04-01

    We have observed the clump G34.43+00.24 MM3 associated with an infrared dark cloud in DNC J = 3-2, HN13C J = 3-2, and N2H+ J = 3-2 with the Atacama Large Millimeter/submillimeter Array (ALMA). The N2H+ emission is found to be relatively weak near the hot core and the outflows, and its distribution is clearly anti-correlated with the CS emission. This result indicates that a young outflow is interacting with cold ambient gas. The HN13C emission is compact and mostly emanates from the hot core, whereas the DNC emission is extended around the hot core. Thus, the DNC and HN13C emission traces warm regions near the protostar differently. The DNC emission is stronger than the HN13C emission toward most parts of this clump. The DNC/HNC abundance ratio averaged within a 15\\prime\\prime × 15\\prime\\prime area around the phase center is higher than 0.06. This ratio is much higher than the value obtained by the previous single-dish observations of DNC and HN13C J = 1-0 (˜0.003). It seems likely that the DNC and HNC emission observed with the single-dish telescope traces lower density envelopes, while that observed with ALMA traces higher density and highly deuterated regions. We have compared the observational results with chemical-model results in order to investigate the behavior of DNC and HNC in the dense cores. Taking these results into account, we suggest that the low DNC/HNC ratio in the high-mass sources obtained by the single-dish observations are at least partly due to the low filling factor of the high density regions.

  12. Menón el politikos. Política y unidad del alma en el Menón de Platón

    OpenAIRE

    Sergio Ariza

    2012-01-01

    Se analizan algunos usos del tópico de la política en el Menón, para mostrar que la virtud discutida es política, no sólo porque los interlocutores están interesados exclusivamente en la cualidad que debe poseer el gobernante, sino también porque tal cualidad consiste en una forma de autogobierno del alma. El alma es vista así como una entidad política cuya excelencia depende del tipo de gobierno impuesto. Se relaciona esta propuesta con la psicología implícita en la primera sección del diálo...

  13. Software as a Service: Herausforderungen bei der Einführung des Bibliothekssystems Alma in der Freien Universität Berlin

    Directory of Open Access Journals (Sweden)

    Jiri Kende

    2015-12-01

    Full Text Available Moderne Bibliothekssysteme werden zunehmend als Software as a Service (SaaS angeboten. Die Berliner Bibliotheken der Freien Universität Berlin, der Humboldt Universität, der Technischen Universität und der Universität der Künste haben für 2016 gemeinsam den Umstieg auf das cloudbasierte Bibliothekssystem Alma beschlossen. Der Aufsatz berichtet über die Herausforderungen während der zweijährigen Vertragsverhandlungen mit besonderem Augenmerk auf den Datenschutz.  Modern library management systems are increasingly offered as Software as a Service (SaaS.The libraries of the Free University Berlin, the Humboldt university, the Technical university and the University of Arts decided concertedly to move in 2016 to the cloud based next generation library management system Alma. The article reviews the challenges during the contract negotiations with a special focus on data protection.

  14. AlmaDL Journals: servizi di qualità per l’editoria scientifica ad accesso aperto dell’Università di Bologna

    Directory of Open Access Journals (Sweden)

    Marialaura Vignocchi

    2012-12-01

    Full Text Available The article illustrates AlmaDL Journals, the open access e-publishing service supporting scientific peer reviewed journals edited by Departments and research groups of the University of Bologna. Digital technologies and the Internet have deeply changed the way researchers and scholars access and share information. Moreover new technologies challenge professionals involved in the publishing value chain and publication life cycle at various levels. The traditional scholarly communication model fails to meet researchers’ needs and expectations. Initiatives such as the AlmaDL Journals seeks to provide alternative models that take full advantage of the digital environment and new media while ensuring quality requirements and the traditional functions of scientific serial publications.

  15. ALMA Observations of the Host Galaxy of GRB 090423 at z = 8.23: Deep Limits on Obscured Star Formation 630 Million Years after the Big Bang

    Science.gov (United States)

    Berger, E.; Zauderer, B. A.; Chary, R.-R.; Laskar, T.; Chornock, R.; Tanvir, N. R.; Stanway, E. R.; Levan, A. J.; Levesque, E. M.; Davies, J. E.

    2014-12-01

    We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F ν(222 GHz) Space Telescope rest-frame ultraviolet (UV) observations is SFRUV ~ 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z >~ 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.

  16. VizieR Online Data Catalog: Orion Integral Filament ALMA+IRAM30m N2H+(1-0) data (Hacar+, 2018)

    Science.gov (United States)

    Hacar, A.; Tafalla, M.; Forbrich, J.; Alves, J.; Meingast, S.; Grossschedl, J.; Teixeira, P. S.

    2018-01-01

    Combined ALMA+IRAM30m large-scale N2H+(1-0) emission in the Orion ISF. Two datasets are presented here in FITS format: 1.- Full data cube: spectral resolution = 0.1 kms-1 2.- Total integrated line intensity (moment 0) map Units are in Jy/beam See also: https://sites.google.com/site/orion4dproject/home (2 data files).

  17. Fast-Growing SMBHs in Fast-Growing Galaxies, at High Redshifts: The Role of Major Mergers As Revealed by ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Trakhtenbrot, Benny [Department of Physics, ETH Zurich, Zurich (Switzerland); Lira, Paulina [Departamento de Astronomia, Universidad de Chile, Santiago (Chile); Netzer, Hagai [Raymond and Beverly Sackler Faculty of Exact Sciences, School of Physics and Astronomy and the Wise Observatory, Tel-Aviv University, Tel-Aviv (Israel); Cicone, Claudia [Department of Physics, ETH Zurich, Zurich (Switzerland); INAF-Osservatorio Astronomico di Brera, Milan (Italy); Maiolino, Roberto [Cavendish Laboratory, University of Cambridge, Cambridge (United Kingdom); Kavli Institute for Cosmology, University of Cambridge, Cambridge (United Kingdom); Shemmer, Ohad, E-mail: benny.trakhtenbrot@phys.ethz.ch [Department of Physics, University of North Texas, Denton, TX (United States)

    2017-11-30

    We present a long-term, multi-wavelength project to understand the epoch of fastest growth of the most massive black holes by using a sample of 40 luminous quasars at z ≃ 4.8. These quasars have rather uniform properties, with typical accretion rates and black hole masses of L/L{sub Edd} ≃ 0.7 and M{sub BH} ≃ 10{sup 9}M{sub ⊙}. The sample consists of “FIR-bright” sources with a previous Herschel/SPIRE detection, suggesting SFR > 1,000 M{sub ⊙} yr−1, as well as of “FIR-faint” sources for which Herschel stacking analysis implies a typical SFR of ~400 M{sub ⊙} yr−1. Six of the quasars have been observed by ALMA in [C ii] λ157.74μm line emission and adjacent rest-frame 150μm continuum, to study the dusty cold ISM. ALMA detected companion, spectroscopically confirmed sub-mm galaxies (SMGs) for three sources—one FIR-bright and two FIR-faint. The companions are separated by ~14–45 kpc from the quasar hosts, and we interpret them as major galaxy interactions. Our ALMA data therefore clearly support the idea that major mergers may be important drivers for rapid, early SMBH growth. However, the fact that not all high-SFR quasar hosts are accompanied by interacting SMGs, and their ordered gas kinematics observed by ALMA, suggest that other processes may be fueling these systems. Our analysis thus demonstrates the diversity of host galaxy properties and gas accretion mechanisms associated with early and rapid SMBH growth.

  18. Exploring molecular complexity with ALMA (EMoCA): Detection of three new hot cores in Sagittarius B2(N)

    Science.gov (United States)

    Bonfand, M.; Belloche, A.; Menten, K. M.; Garrod, R. T.; Müller, H. S. P.

    2017-08-01

    Context. The Sagittarius B2 molecular cloud contains several sites forming high-mass stars. Sgr B2(N) is one of its main centers of activity. It hosts several compact and ultra-compact HII regions, as well as two known hot molecular cores (Sgr B2(N1) and Sgr B2(N2)) in the early stage of the high-mass star formation process, where complex organic molecules (COMs) are detected in the gas phase. Aims: Our goal is to use the high sensitivity of the Atacama Large Millimeter/submillimeter Array (ALMA) to characterize the hot core population in Sgr B2(N) and thereby shed new light on the star formation process in this star-forming region. Methods: We use a complete 3 mm spectral line survey conducted with ALMA to search for faint hot cores in the Sgr B2(N) region. The chemical composition of the detected sources and the column densities are derived by modeling the whole spectra under the assumption of local thermodynamic equilibrium. Population diagrams are constructed to fit rotational temperatures. Integrated intensity maps are produced to derive the peak position and fit the size of each molecule's emission distribution. The kinematic structure of the hot cores is investigated by analyzing the line wing emission of typical outflow tracers. The H2 column densities are computed from ALMA and SMA continuum emission maps. Results: We report the discovery of three new hot cores in Sgr B2(N) that we call Sgr B2(N3), Sgr B2(N4), and Sgr B2(N5). The three sources are associated with class II methanol masers, well known tracers of high-mass star formation, and Sgr B2(N5), also with a UCHII region. Their H2 column densities are found to be between approximately 16 and 36 times lower than the one of the main hot core Sgr B2(N1). The spectra of these new hot cores have spectral line densities of 11 up to 31 emission lines per GHz above the 7σ level, assigned to 22-25 molecules plus 13-20 less abundant isotopologs. We derive rotational temperatures of approximately 140-180 K for

  19. Hygienic sanitary conditions of sun dried meat marketed in Cruz das Almas, Bahia and detection of strains with antimicrobial resistance

    Directory of Open Access Journals (Sweden)

    Norma Suely Evangelista-Barreto

    2014-06-01

    Full Text Available This study aimed to evaluate the microbiological, physical and chemical qualities of sun dried meat marketed in Cruz das Almas, Bahia, as well as trace the resistance profile of the isolated strains against different commercial pharmacos. There were collected and analysed 36 samples of sun dried meat, acquired in 12 different establishment (supermarkets, mini-markets, butchers and a municipal market, and quantified mesophilic aerobic bacteria, coliforms, Staphylococcus coagulase positive, E. coli and presence of Salmonella spp., as well as specific content humidity, water activity (Aw and chloride. In 83% of the establishments, mesophilic bacteria counted > 105 CFU.g-1 and 58% coliforms at 35º C > 105 NMP.g- 1 and coliforms at 45ºC > 103 NMP.g-1. Escherichia coli was isolated in 75% of the establishments. Staphylococcus spp. ranged from 4.8 x 104 to 9.0 x 108 UFC.g-1, not being isolated Staphylococcus coagulase positive. Salmonella was found in 25% of the establishments. The humidity in the sun dried meat samples ranged from 52.37% to 74.69%, the Aw from 0.87 to 0.95 and the chloride from 3.16% to 5.98%. Salmonella was 100% resistant to tetracycline, acid nalidixic, cephalothin and erythromycin, with intermediate resistance to ampicillin and gentamicin. Escherichia coli was resistant to erythromycin (100%, ampicillin (68.7%, cephalothin (71.4%, tetracycline (64.2%, nalidixic acid (35.7% and gentamicin (12.5%. Multiresistant strains of E. coli were observed in 87.5% of the isolates, and it happened that in 28.6% of the resistance it was mediated by plasmids. Multidrug resistance profile was observed in all Salmonella, with a strain showing plasmid resistance. The marketing of sun dried meat in Cruz das Almas presents hygienic and sanitary failures due to it’s high microbial loads. This fact undermines the safety and product lifetime, and may also pose risk to public health since it markets strains with antimicrobial.

  20. An ALMA study of the Orion Integral Filament. I. Evidence for narrow fibers in a massive cloud

    Science.gov (United States)

    Hacar, A.; Tafalla, M.; Forbrich, J.; Alves, J.; Meingast, S.; Grossschedl, J.; Teixeira, P. S.

    2018-03-01

    Aim. We have investigated the gas organization within the paradigmatic Integral Shape Filament (ISF) in Orion in order to decipher whether or not all filaments are bundles of fibers. Methods: We combined two new ALMA Cycle 3 mosaics with previous IRAM 30m observations to produce a high-dynamic range N2H+ (1-0) emission map of the ISF tracing its high-density material and velocity structure down to scales of 0.009 pc (or 2000 AU). Results: From the analysis of the gas kinematics, we identify a total of 55 dense fibers in the central region of the ISF. Independently of their location in the cloud, these fibers are characterized by transonic internal motions, lengths of 0.15 pc, and masses per unit length close to those expected in hydrostatic equilibrium. The ISF fibers are spatially organized forming a dense bundle with multiple hub-like associations likely shaped by the local gravitational potential. Within this complex network, the ISF fibers show a compact radial emission profile with a median FWHM of 0.035 pc systematically narrower than the previously proposed universal 0.1 pc filament width. Conclusions: Our ALMA observations reveal complex bundles of fibers in the ISF, suggesting strong similarities between the internal substructure of this massive filament and previously studied lower-mass objects. The fibers show identical dynamic properties in both low- and high-mass regions, and their widespread detection in nearby clouds suggests a preferred organizational mechanism of gas in which the physical fiber dimensions (width and length) are self-regulated depending on their intrinsic gas density. Combining these results with previous works in Musca, Taurus, and Perseus, we identify a systematic increase of the surface density of fibers as a function of the total mass per-unit-length in filamentary clouds. Based on this empirical correlation, we propose a unified star-formation scenario where the observed differences between low- and high-mass clouds, and the

  1. Malaria control in the African Region: perceptions and viewspoints on proceedings of the Africa Leaders Malaria Alliance (ALMA

    Directory of Open Access Journals (Sweden)

    Sambo Luis

    2011-06-01

    Full Text Available Abstract Background In 2009 a total of 153,408 malaria deaths were reported in Africa. Eleven countries showed a reduction of more than 50% in either confirmed malaria cases or malaria admissions and deaths in recent years. However, many African countries are not on track to achieve the malaria component of the Millennium Development Goal (MDG 6. The African Leaders Malaria Alliance (ALMA working session at the 15th African Union Summit discussed the bottlenecks to achieving MDG 6 (specifically halting and beginning to reverse the incidence of malaria by 2015, success factors, and what countries needed to do to accelerate achievement of the MDG. The purpose of this article is to reflect on the proceedings of the ALMA working session. Methods Working methods of the session included speeches and statements by invited speakers and high-level panel discussions. Discussion The main bottlenecks identified related to the capacity of the health systems to deliver quality care and accessibility issues; need for strong, decentralized malaria-control programmes with linkages with other health and development sectors, the civil society and private sector entities; benefits of co-implementation of malaria control programmes with child survival or other public health interventions; systematic application of integrated promotive, preventive, diagnostic and case management interventions with full community participation; adapting approaches to local political, socio-cultural and administrative environments. The following prerequisites for success were identified: a clear vision and effective leadership of national malaria control programmes; high level political commitment to ensure adequate capacity in expertise, skill mix and number of managers, technicians and service providers; national ownership, intersectoral collaboration and accountability, as well as strong civil society and private sector involvement; functional epidemiological surveillance systems

  2. DA RELAÇÃO CORPO-ALMA À MENTE-CÉREBRO: A ANTROPOLOGIA CRISTÃ E AS NOVAS ANTROPOLOGIAS

    Directory of Open Access Journals (Sweden)

    Renato Alves de Oliveira

    2014-01-01

    Full Text Available O objetivo deste artigo é mostrar que a questão referente aos dois princípios metafísicos constitutivos da antropologia cristã, o corpo/matéria e a alma/espírito, e a forma de conceber a relação entre eles encontra-se presentes no subsolo das novas antropologias materialistas, mas com um novo verniz através da relação entre a mente e o cérebro. Para a antropologia cristã, a existência do binômio corpo-alma é uma questão resolvida. As discussões se concentram na forma de conceber a relação entre ambos os princípios. Analogamente, para algumas antropologias materialistas atuais, a existência da mente e do cérebro é uma questão fechada. Os confrontos encontram-se na forma de conceber as relações entre a mente e o cérebro: há uma identificação ou distinção entres ambas as realidades? A mente seria uma qualidade emergente do cérebro?   ABSTRACT: The purpose of this article is to show that the question concerning the two constituent metaphysical principles of Christian anthropology, body/matter and soul/spirit, and the way of conceiving the relationship between them is presente in the basement of the new materialist anthropologies, but with a new varnish through the relationship between mind and brain. For Christian anthropology, the existence of the binomial soul/body is a settled issue. The discussions focus on how to design the relationship between the two principles. Similarly, for some current materialistic anthropologies, the existence of the mind and the brain is a closed question. The clashes are the way of conceiving the relationship between mind and brain: Is there an identification or a distinction between the two realities? Would be the mind an emergent quality of the brain?

  3. ALMA OBSERVATIONS OF THE SUBMILLIMETER DENSE MOLECULAR GAS TRACERS IN THE LUMINOUS TYPE-1 ACTIVE NUCLEUS OF NGC 7469

    International Nuclear Information System (INIS)

    Izumi, Takuma; Kohno, Kotaro; Ikarashi, Soh; Aalto, Susanne; Doi, Akihiro; Espada, Daniel; Fathi, Kambiz; Harada, Nanase; Hsieh, Pei-Ying; Matsushita, Satoki; Hatsukade, Bunyo; Hattori, Takashi; Imanishi, Masatoshi; Iono, Daisuke; Ishizuki, Sumio; Nagai, Hiroshi; Krips, Melanie; Martín, Sergio; Meier, David S.; Nakai, Naomasa

    2015-01-01

    We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 1 observations of the central kiloparsec region of the luminous type 1 Seyfert galaxy NGC 7469 with unprecedented high resolution (0.″5 ×0.″4 = 165 × 132 pc) at submillimeter wavelengths. Utilizing the wide bandwidth of ALMA, we simultaneously obtained HCN(4–3), HCO + (4–3), CS(7–6), and partially CO(3–2) line maps, as well as the 860 μm continuum. The region consists of the central ∼1″ component and the surrounding starburst ring with a radius of ∼1.″5–2.″5. Several structures connect these components. Except for CO(3–2), these dense gas tracers are significantly concentrated toward the central ∼1″, suggesting their suitability to probe the nuclear regions of galaxies. Their spatial distribution resembles well those of centimeter and mid-infrared continuum emissions, but it is anticorrelated with the optical one, indicating the existence of dust-obscured star formation. The integrated intensity ratios of HCN(4–3)/HCO + (4–3) and HCN(4–3)/CS(7–6) are higher at the active galactic nucleus (AGN) position than at the starburst ring, which is consistent with our previous findings (submillimeter-HCN enhancement). However, the HCN(4–3)/HCO + (4–3) ratio at the AGN position of NGC 7469 (1.11 ± 0.06) is almost half of the corresponding value of the low-luminosity type 1 Seyfert galaxy NGC 1097 (2.0 ± 0.2), despite the more than two orders of magnitude higher X-ray luminosity of NGC 7469. But the ratio is comparable to that of the close vicinity of the AGN of NGC 1068 (∼1.5). Based on these results, we speculate that some heating mechanisms other than X-ray (e.g., mechanical heating due to an AGN jet) can contribute significantly for shaping the chemical composition in NGC 1097

  4. ALMA OBSERVATIONS OF THE SUBMILLIMETER DENSE MOLECULAR GAS TRACERS IN THE LUMINOUS TYPE-1 ACTIVE NUCLEUS OF NGC 7469

    Energy Technology Data Exchange (ETDEWEB)

    Izumi, Takuma; Kohno, Kotaro; Ikarashi, Soh [Institute of Astronomy, School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Aalto, Susanne [Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Observatory, SE-439 94 Onsala (Sweden); Doi, Akihiro [Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara 252-5210 (Japan); Espada, Daniel [Joint ALMA Observatory, Alonso de Córdova, 3107, Vitacura, Santiago 763-0355 (Chile); Fathi, Kambiz [Stockholm Observatory, Department of Astronomy, Stockholm University, AlbaNova Centre, SE-106 91 Stockholm (Sweden); Harada, Nanase; Hsieh, Pei-Ying; Matsushita, Satoki [Academia Sinica, Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 10617, Taiwan (China); Hatsukade, Bunyo; Hattori, Takashi; Imanishi, Masatoshi; Iono, Daisuke; Ishizuki, Sumio; Nagai, Hiroshi [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Krips, Melanie; Martín, Sergio [Institut de Radio Astronomie Millimétrique, 300 rue de la Piscine, Domaine Universitaire, F-38406 St. Martin d’Hères (France); Meier, David S. [Department of Physics, New Mexico Institute of Mining and Technology, 801 Leroy Place, Soccoro, NM 87801 (United States); Nakai, Naomasa, E-mail: takumaizumi@ioa.s.u-tokyo.ac.jp [Department of Physics, Faculty of Pure and Applied Sciences, University of Tsukuba, 1-1-1 Ten-nodai, Tsukuba, Ibaraki 305-8571 (Japan); and others

    2015-09-20

    We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 1 observations of the central kiloparsec region of the luminous type 1 Seyfert galaxy NGC 7469 with unprecedented high resolution (0.″5 ×0.″4 = 165 × 132 pc) at submillimeter wavelengths. Utilizing the wide bandwidth of ALMA, we simultaneously obtained HCN(4–3), HCO{sup +}(4–3), CS(7–6), and partially CO(3–2) line maps, as well as the 860 μm continuum. The region consists of the central ∼1″ component and the surrounding starburst ring with a radius of ∼1.″5–2.″5. Several structures connect these components. Except for CO(3–2), these dense gas tracers are significantly concentrated toward the central ∼1″, suggesting their suitability to probe the nuclear regions of galaxies. Their spatial distribution resembles well those of centimeter and mid-infrared continuum emissions, but it is anticorrelated with the optical one, indicating the existence of dust-obscured star formation. The integrated intensity ratios of HCN(4–3)/HCO{sup +}(4–3) and HCN(4–3)/CS(7–6) are higher at the active galactic nucleus (AGN) position than at the starburst ring, which is consistent with our previous findings (submillimeter-HCN enhancement). However, the HCN(4–3)/HCO{sup +}(4–3) ratio at the AGN position of NGC 7469 (1.11 ± 0.06) is almost half of the corresponding value of the low-luminosity type 1 Seyfert galaxy NGC 1097 (2.0 ± 0.2), despite the more than two orders of magnitude higher X-ray luminosity of NGC 7469. But the ratio is comparable to that of the close vicinity of the AGN of NGC 1068 (∼1.5). Based on these results, we speculate that some heating mechanisms other than X-ray (e.g., mechanical heating due to an AGN jet) can contribute significantly for shaping the chemical composition in NGC 1097.

  5. Malaria control in the African Region: perceptions and viewspoints on proceedings of the Africa Leaders Malaria Alliance (ALMA).

    Science.gov (United States)

    Sambo, Luis Gomes; Ki-Zerbo, Georges; Kirigia, Joses Muthuri

    2011-06-13

    In 2009 a total of 153,408 malaria deaths were reported in Africa. Eleven countries showed a reduction of more than 50% in either confirmed malaria cases or malaria admissions and deaths in recent years. However, many African countries are not on track to achieve the malaria component of the Millennium Development Goal (MDG) 6. The African Leaders Malaria Alliance (ALMA) working session at the 15th African Union Summit discussed the bottlenecks to achieving MDG 6 (specifically halting and beginning to reverse the incidence of malaria by 2015), success factors, and what countries needed to do to accelerate achievement of the MDG. The purpose of this article is to reflect on the proceedings of the ALMA working session. Working methods of the session included speeches and statements by invited speakers and high-level panel discussions. The main bottlenecks identified related to the capacity of the health systems to deliver quality care and accessibility issues; need for strong, decentralized malaria-control programmes with linkages with other health and development sectors, the civil society and private sector entities; benefits of co-implementation of malaria control programmes with child survival or other public health interventions; systematic application of integrated promotive, preventive, diagnostic and case management interventions with full community participation; adapting approaches to local political, socio-cultural and administrative environments.The following prerequisites for success were identified: a clear vision and effective leadership of national malaria control programmes; high level political commitment to ensure adequate capacity in expertise, skill mix and number of managers, technicians and service providers; national ownership, intersectoral collaboration and accountability, as well as strong civil society and private sector involvement; functional epidemiological surveillance systems; and levering of African Union and regional economic

  6. Real life experience with frontline azacitidine in a large series of older adults with acute myeloid leukemia stratified by MRC/LRF score: results from the expanded international E-ALMA series (E-ALMA+).

    Science.gov (United States)

    Falantes, José; Pleyer, Lisa; Thépot, Sylvain; Almeida, António M; Maurillo, Luca; Martínez-Robles, Violeta; Stauder, Reinhard; Itzykson, Raphael; Pinto, Ricardo; Venditti, Adriano; Bargay, Joan; Burgstaller, Sonja; Martínez, María Pilar; Seegers, Valerie; Cortesão, Emilia; Foncillas, María Ángeles; Gardin, Claude; Montesinos, Pau; Musto, Pellegrino; Fenaux, Pierre; Greil, Richard; Sanz, Miguel Angel; Ramos, Fernando

    2018-05-01

    Azacitidine (AZA) prolonged overall survival (OS) in the AZA-AML-001 trial. However, few subjects were randomized to AZA or intensive chemotherapy (IC). The Medical Research Council (MRC) and the Leukemia Research Foundation (LRF) developed a score for older AML patients receiving IC or non-intensive regimens, whereas the E-ALMA study validated a score for survival and response in elderly patients receiving AZA in daily practice. Both identified three groups with different risk estimates. This analysis evaluates the efficacy of frontline AZA in older AML patients (N = 710) unfit for IC from different national registries (E-ALMA + series) stratified by the MRC/LRF risk score. Median OS of patients categorized as good, standard and poor-risk groups by the MRC/LRF score was 13.4 (95% CI, 10.8-16), 12.4 (95% CI, 9.9-14.8), and 8.1 months (95% CI, 7-9.1), respectively (p = .0001). In conclusion, this is the largest retrospective cohort of older AML patients treated with AZA.

  7. Star-Formation History in Early Universe Revealed by Blind Line-Search Using AtLAST and ALMA

    Science.gov (United States)

    Hayatsu, H.; Natsuki

    2018-01-01

    Using blind line searches to understand the cosmic star-formation history is one of the strategies that will be pursued by AtLAST, which will have high sensitivity and mapping speed. Before moving into the 'AtLAST era', it is essential to develop a method to efficiently detect faint sources considering the completeness of source detection and contamination by false detections. Furthermore, in order to propose strategies for blind line searching using AtLAST, it is necessary to know to what extent we can constrain the luminosity function using existing ALMA archival data. In this presentation, we report the current status of tests using a blind line-searching method and show preliminary results. We plan to apply our final results to various science cases for future AtLAST observations e.g. cross-checking the luminosity density using an intensity-mapping technique or estimating the redshift evolution of ionization state or metallicity by combining with JWST or SPICA data. We plan to release our code as a CASA task.

  8. MODA ODAKLI İÇGÜDÜSEL SATIN ALMA DAVRANIŞINA ETKİ EDEN FAKTÖRLER

    Directory of Open Access Journals (Sweden)

    İlknur TÜFEKÇİ

    2014-10-01

    Full Text Available ÖZ: Günümüzde geleneksel birçok moda perakendecisi, esnek olmayan tedarik zinciri, onun yarattığı aşırı stok ve kâr kayıplarıyla mücadele ederken, hızlı moda perakendecileri esnek tedarik zinciri yönetimi ve yeni trendlere hızla uyum sağlayarak bu problemi avantaja dönüştürmüşlerdir. Bu sayede hızlı moda pazarını oluşturma ve geliştirmede büyük başarı sağlamışlardır. Dolayısıyla çalışma, bu pazarda yer alan tüketicilerin algı ve tutumlarının satın alma davranışlarına etkisini belirlemek amacıyla düzenlenmiştir. Çalışma Atatürk Üniversitesi’nde okuyan kız öğrencilere 387 adet anket uygulaması yoluyla gerçekleştirilmiştir. Araştırmanın amaçları doğrultusunda öncelikle hızlı moda perakendeciliğine yönelik tutum, kıtlık algısı, düşük fiyat algısı ve tükenebilir algısının moda odaklı içgüdüsel satın alma davranışı üzerine etkisini belirlemek için çoklu regresyon analizi yapılmıştır. Sonrasında ise çok kriterli karar verme tekniklerinden TOPSIS yöntemi ile bu değişkenlerin önem sıralaması belirlenmiştir. Söz konusu değişkenlerin moda odaklı içgüdüsel satın alma üzerinde anlamlı bir etkiye sahip olduğu ve kriterler arasında en önemi etkiyi “tükenebilir algısı”nın taşıdığı belirlenmiştir. Anahtar Kelimeler: Hızlı Moda, Moda Odaklı İçgüdüsel Satın Alma, TOPSIS. ABSTRACT: Many traditional fashion retailer are struggling with inflexible supply chain and the excess inventory and profit loss due to this inflexibility. But, these problems have been converted into advantages by fast fashion retailers, via adapting quickly to new trends and flexible supply chain management. In this way, they have achieved great success which is the creation of the fast fashion market and development. Therefore, the aim of this study is to determine consumers' perceptions and attitudes effect on purchase behavior in this market

  9. Molecular Outflow and Feedback in an Obscured Quasar at z˜1.5 Revealed by ALMA

    Science.gov (United States)

    Brusa, Marcella

    2017-11-01

    We imaged with ALMA and ARGOS/LUCI the molecular gas and the dust and stellar continuum in XID2028, an obscured QSO at z=1.593, where the presence of a massive outflow in the ionized gas component traced by the [O III]5007 emission has been resolved up to 10 kpc. This target does represent a unique test case to study QSO 'feedback in action' at the peak epoch of AGN- galaxy coevolution. The QSO has been detected both in the CO(5-4) transition and in the 1.3mm continuum, with emissions confined in the central ( consumption conditions in XID2028, possibly due to feedback effects on the host galaxy. Finally, we observe an asymmetric profile of the CO(5-4) line, which suggests the presence of high velocity gas up to 700 km/s. An image of the blueshfited and redshifted CO wings provides the first detection of a spatially resolved, galaxy-scale molecular outflow at high-z, extended in opposite directions with the approaching component spatially coincident with the ionised gas outflow. The resolved, molecular outflow appear to be cospatial with the component observed int the ionised gas. XID2028 therefore represents the first example of molecular and ionised kpc scales outflows at high-z.

  10. Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [C I

    Science.gov (United States)

    Emonts, B. H. C.; Lehnert, M. D.; Dannerbauer, H.; De Breuck, C.; Villar-Martín, M.; Miley, G. K.; Allison, J. R.; Gullberg, B.; Hatch, N. A.; Guillard, P.; Mao, M. Y.; Norris, R. P.

    2018-03-01

    The circumgalactic medium (CGM) of the massive Spiderweb Galaxy, a conglomerate of merging proto-cluster galaxies at z=2.2, forms an enriched interface where feedback and recycling act on accreted gas. This is shown by observations of [C I], CO(1-0) and CO(4-3) performed with the Atacama Large Millimeter Array (ALMA) and Australia Telescope Compact Array (ATCA). [C I] and CO(4-3) are detected across ˜50 kpc, following the distribution of previously detected low-surface-brightness CO(1-0) across the CGM. This confirms our previous results on the presence of a cold molecular halo. The central radio galaxy MRC 1138-262 shows a very high global L΄CO(4-3)/L΄CO(1-0) ˜ 1, suggesting that mechanisms other than FUV-heating by star formation prevail at the heart of the Spiderweb Galaxy. Contrary, the CGM has L΄CO(4-3)/L΄CO(1-0) and L΄[CI]/L΄CO(1-0) similar to the ISM of five galaxies in the wider proto-cluster, and its carbon abundance, X[CI]/XH2, resembles that of the Milky Way and starforming galaxies. The molecular CGM is thus metal-rich and not diffuse, confirming a link between the cold gas and in-situ star formation. Thus, the Spiderweb Galaxy grows not directly through accretion of gas from the cosmic web, but from recycled gas in the GCM.

  11. ESTUDO DE MANIFESTAÇÕES PATOLÓGICAS DO TERMINAL RODOVIÁRIO DE CRUZ DAS ALMAS - BA

    Directory of Open Access Journals (Sweden)

    Henrique Almeida Santana

    2016-11-01

    Full Text Available Patologia para a construção civil é entendido como a parte de engenharia que estuda os sintomas, causas e origens das lesões nas edificações. O Terminal Rodoviário da cidade de Cruz das Almas foi construído na década de oitenta, apresentando constante fluxo de veículos, com alta emissão de gás carbônico. Devido à aparência degradada da edificação, o presente trabalho teve como objetivo estudar as manifestações patológicas e determinar um prognóstico através de visita na edificação e revisão literária. As manifestações que predominam são as fissuras, manchas de umidade, segregação em peças de concreto e recalques. Os estudos mostraram que a edificação necessita de intervenções terapêuticas pertinente a manifestações patológicas, acompanhadas de profissionais habilitados.

  12. Evolução da temperatura ambiente em construções sujeitas ao fogo

    OpenAIRE

    Inácio, Pedro Jorge Rita Ledo

    2011-01-01

    Dissertação para a obtenção do Grau de Mestre em Engenharia Civil A perda de bens materiais e de vidas humanas em situações de incêndio tem sido ao longo dos tempos uma preocupação crescente, promovendo assim o conceito de segurança contra incêndio e de diversos mecanismos associados à sua prevenção ou limitação dos danos causados. Um incêndio é algo difícil de prever, assim como a sua consequência nos elementos de construção. Dessa forma, ao longo das ultimas décadas, os elementos d...

  13. Microbiological quality and antimicrobial susceptibility of informally traded milk in Cruz das Almas county, Bahia Qualidade microbiológica e suscetibilidade antimicrobiana do leite in natura comercializado em Cruz das Almas, Bahia

    Directory of Open Access Journals (Sweden)

    Norma Suely Evangelista Barreto

    2012-12-01

    Full Text Available The microbiological quality as well as the antimicrobial susceptibility of bacteria isolated from raw milk obtained from 25 food stores in Cruz das Almas, Bahia were evaluated. The analysis included counts of mesophilic and psicrotrophic microorganisms, molds and yeast, Staphylococcus spp., coagulase-positive Staphylococcus, coliforms (at 35ºC and 45ºC, and the presence of Salmonella spp. and Escherichia coli. The average count for mesophilic and psicrotrophic microorganisms, molds and yeast, and coliforms at 35°C and 45°C were 1.6 x 109 CFU.mL-1, 9.6 x 104 CFU.mL-1, 3.8 x 108 CFU. mL-1, 4.0 x 105 MPN.mL-1 and 3.8 x 105 MPN.mL-1, respectively. Coagulase positive Staphylococcus was found in 44% of the samples (mean value of 7.3 x 105 CFU.mL-1, and E. coli was present in 76% of them. Salmonella was not detected in any of the samples tested. E. coli showed resistance (57.9% to tetracycline, to ampicillin and chloramphenicol (10.5%, and cephalotin (5.3%, while coagulase-positive Staphylococcus strains were resistant to amicacin (18% and vancomicin (18%. The raw milk besides to present poor microbiological quality, becoming a health risk of the consumers, it may contribute to the dissemination of resistant bacteria to various antimicrobial agents. Para a avaliação da qualidade microbiológica do leite in natura, bem como a suscetibilidade antimicrobiana das bactérias isoladas, foram analisados 25 estabelecimentos comerciais em Cruz das Almas, Ba. Para isso realizou-se a quantificação de micro-organismos heterotróficos mesófilos e psicrotróficos aeróbios, bolores e leveduras, Staphylococcus spp., Staphylococcus coagulase positiva, coliformes (35ºC e 45ºC e presença de Salmonella spp. e Escherichia coli. A contagem média de micro-organismos heterotróficos mesófilos foi de 1,6 x 109 UFC.mL-1, psicrotróficos 9,6 x 104 UFC. mL-1, bolores e leveduras 3,8 x 108 UFC.mL-1, coliformes a 35°C 4 x 105 NMP.mL-1 e a 45°C 3,8 x 105 NMP.mL-1

  14. La metáfora de la luz como expresión del alma en “Livia y los sueños” de Jesús Gardea

    Directory of Open Access Journals (Sweden)

    María del Rosario Lara

    2014-01-01

    Full Text Available En el presente artículo exploramos la expresión artística de la idea de alma a través de la metáfora de la luz tal y como aparece en “Livia y los sueños” . Para ello, nos basare - mos en los postulados filosóficos de María Zambrano referentes a las concepciones de alma, ser humano y destino. En nuestra investigación también abordaremos la forma como tiempo y espacio en la obra de Gardea integran un cronotopo específico, como base donde la idea de alma puede desplegarse en toda su plenitud.

  15. An intensely star-forming galaxy at z ∼ 7 with low dust and metal content revealed by deep ALMA and HST observations

    Energy Technology Data Exchange (ETDEWEB)

    Ouchi, Masami; Ono, Yoshiaki; Momose, Rieko [Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8582 (Japan); Ellis, Richard [Department of Astrophysics, California Institute of Technology, MS 249-17, Pasadena, CA 91125 (United States); Nakanishi, Kouichiro [The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Kohno, Kotaro; Tamura, Yoichi [Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Kurono, Yasutaka [Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago 763-0355 (Chile); Ashby, M. L. N.; Willner, S. P.; Fazio, G. G. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Shimasaku, Kazuhiro [Research Center for the Early Universe (WPI), University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033 (Japan); Iono, Daisuke, E-mail: ouchims@icrr.u-tokyo.ac.jp [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)

    2013-12-01

    We report deep ALMA observations complemented by associated Hubble Space Telescope (HST) imaging for a luminous (m {sub UV} = 25) galaxy, 'Himiko', at a redshift of z = 6.595. The galaxy is remarkable for its high star formation rate, 100 M {sub ☉} yr{sup –1}, which has been securely estimated from our deep HST and Spitzer photometry, and the absence of any evidence for strong active galactic nucleus activity or gravitational lensing magnification. Our ALMA observations probe an order of magnitude deeper than previous IRAM observations, yet fail to detect a 1.2 mm dust continuum, indicating a flux of <52 μJy, which is comparable to or weaker than that of local dwarf irregulars with much lower star formation rates. We likewise provide a strong upper limit for the flux of [C II] 158 μm, L{sub [C} {sub II]}<5.4×10{sup 7} L{sub ⊙}, which is a diagnostic of the hot interstellar gas that is often described as a valuable probe for early galaxies. In fact, our observations indicate that Himiko lies off the local L{sub [C} {sub II]}-star formation rate scaling relation by a factor of more than 30. Both aspects of our ALMA observations suggest that Himiko is a unique object with a very low dust content and perhaps nearly primordial interstellar gas. Our HST images provide unique insight into the morphology of this remarkable source, highlighting an extremely blue core of activity and two less extreme associated clumps. Himiko is undergoing a triple major merger event whose extensive ionized nebula of Lyα emitting gas, discovered in our earlier work with Subaru, is powered by star formation and the dense circumgalactic gas. We are likely witnessing an early massive galaxy during a key period of its mass assembly close to the end of the reionization era.

  16. ALMA INVESTIGATION OF VIBRATIONALLY EXCITED HCN/HCO{sup +}/HNC EMISSION LINES IN THE AGN-HOSTING ULTRALUMINOUS INFRARED GALAXY IRAS 20551−4250

    Energy Technology Data Exchange (ETDEWEB)

    Imanishi, Masatoshi [Subaru Telescope, 650 North A’ohoku Place, Hilo, HI 96720 (United States); Nakanishi, Kouichiro [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Izumi, Takuma, E-mail: masa.imanishi@nao.ac.jp [Institute of Astronomy, School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan)

    2016-07-01

    We present the results of ALMA Cycle 2 observations of the ultraluminous infrared galaxy IRAS 20551−4250 at HCN/HCO{sup +}/HNC J = 3–2 lines at both vibrational ground ( v = 0) and vibrationally excited ( v {sub 2} = 1) levels. This galaxy contains a luminous buried active galactic nucleus (AGN), in addition to starburst activity, and our ALMA Cycle 0 data revealed a tentatively detected vibrationally excited HCN v {sub 2} = 1f J = 4–3 emission line. In our ALMA Cycle 2 data, the HCN/HCO{sup +}/HNC J = 3–2 emission lines at v = 0 are clearly detected. The HCN and HNC v {sub 2} = 1f J = 3–2 emission lines are also detected, but the HCO{sup +} v {sub 2} = 1f J = 3–2 emission line is not. Given the high energy level of v {sub 2} = 1 and the resulting difficulty of collisional excitation, we compared these results with those of the calculation of infrared radiative pumping, using the available infrared 5–35 μ m spectrum. We found that all of the observational results were reproduced if the HCN abundance was significantly higher than that of HCO{sup +} and HNC. The flux ratio and excitation temperature between v {sub 2} = 1f and v = 0, after correction for possible line opacity, suggests that infrared radiative pumping affects rotational ( J -level) excitation at v = 0 at least for HCN and HNC. The HCN-to-HCO{sup +} v = 0 flux ratio is higher than those of starburst-dominated regions, and will increase even more when the derived high HCN opacity is corrected. The enhanced HCN-to-HCO{sup +} flux ratio in this AGN-hosting galaxy can be explained by the high HCN-to-HCO{sup +} abundance ratio and sufficient HCN excitation at up to J = 4, rather than the significantly higher efficiency of infrared radiative pumping for HCN than HCO{sup +}.

  17. ALMACAL - III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H I-absorption-selected system

    Science.gov (United States)

    Klitsch, A.; Péroux, C.; Zwaan, M. A.; Smail, I.; Oteo, I.; Biggs, A. D.; Popping, G.; Swinbank, A. M.

    2018-03-01

    Studying the flow of baryons into and out of galaxies is an important part of understanding the evolution of galaxies over time. We present a detailed case study of the environment around an intervening Ly α absorption line system at zabs = 0.633, seen towards the quasar J0423-0130 (zQSO = 0.915). We detect with ALMA the 12CO(2-1), 12CO(3-2), and 1.2 mm continuum emission from a galaxy at the redshift of the Ly α absorber at a projected distance of 135 kpc. From the ALMA detections, we infer interstellar medium conditions similar to those in low-redshift luminous infrared galaxies. Director's Discretionary Time (DDT) Multi-Unit Spectroscopic Explorer (MUSE) integral field unit observations reveal the optical counterpart of the 12CO emission line source and three additional emission line galaxies at the absorber redshift, which together form a galaxy group. The 12CO emission line detections originate from the most massive galaxy in this group. While we cannot exclude that we miss a fainter host, we reach a dust-uncorrected star formation rate (SFR) limit of >0.3 M⊙yr-1 within 100 kpc from the sightline to the background quasar. We measure the dust-corrected SFR (ranging from 3 to 50 M⊙ yr-1), the morpho-kinematics and the metallicities of the four group galaxies to understand the relation between the group and the neutral gas probed in absorption. We find that the Ly α absorber traces either an outflow from the most massive galaxy or intragroup gas. This case study illustrates the power of combining ALMA and MUSE to obtain a census of the cool baryons in a bounded structure at intermediate redshift.

  18. ALMA Observations of the Galactic Center: SiO Outflows and High Mass Star Formation Near Sgr A

    Science.gov (United States)

    Yusef-Zadeh, F.; Royster, M.; Wardle, M.; Arendt, R.; Bushouse, H.; Gillessen, S.; Lis, D.; Pound, M. W.; Roberts, D. A.; Whitney, B.; hide

    2013-01-01

    Using ALMA observations of the Galactic center with a spatial resolution of 2.61" x 0.97 ", we detected 11 SiO (5-4) clumps of molecular gas in the within 0.6pc (15") of Sgr A*, interior of the 2-pc circumnuclear molecular ring. Three SiO (5-4) clumps closest to Sgr A* show the largest central velocities of approximately 150 kilometers per second and broadest asymmetric linewidths with total linewidths FWZI approximately 110-147 kilometers per second. Other clumps are distributed mainly to the NE of the ionized minispiral with narrow linewidths of FWHM approximately 11-27 kilometers per second. Using CARMA data, LVG modeling of the broad velocity clumps, the SiO (5-4) and (2-1) line ratios constrain the column density N(SiO) approximately 10(exp 14) per square centimeter, and the H2 gas density n(sub H2) = (3-9) x 10(exp 5) per cubic centimeter for an assumed kinetic temperature 100-200K. The SiO (5-4) clumps with broad and narrow linewidths are interpreted as highly embedded protostellar outflows, signifying an early stage of massive star formation near Sgr A* in the last 104 years. Additional support for the presence of YSO outflows is that the luminosities and velocity widths lie in the range detected from protostellar outflows in star forming regions in the Galaxy. Furthermore, SED modeling of stellar sources along the N arm show two YSO candidates near SiO clumps supporting in-situ star formation near Sgr A*. We discuss the nature of star formation where the gravitational potential of the black hole dominates. In particular, we suggest that external radiative pressure exerted on self-shielded molecular clouds enhance the gas density, before the gas cloud become gravitationally unstable near Sgr A*.

  19. The evolution of interstellar medium mass probed by dust emission: Alma observations at z = 0.3-2

    International Nuclear Information System (INIS)

    Scoville, N.; Manohar, S.; Aussel, H.; Sheth, K.; Scott, K. S.; Sanders, D.; Ivison, R.; Pope, A.; Capak, P.; Vanden Bout, P.; Kartaltepe, J.; Robertson, B.; Lilly, S.

    2014-01-01

    The use of submillimeter dust continuum emission to probe the mass of interstellar dust and gas in galaxies is empirically calibrated using samples of local star-forming galaxies, Planck observations of the Milky Way, and high-redshift submillimeter galaxies. All of these objects suggest a similar calibration, strongly supporting the view that the Rayleigh-Jeans tail of the dust emission can be used as an accurate and very fast probe of the interstellar medium (ISM) in galaxies. We present ALMA Cycle 0 observations of the Band 7 (350 GHz) dust emission in 107 galaxies from z = 0.2 to 2.5. Three samples of galaxies with a total of 101 galaxies were stellar-mass-selected from COSMOS to have M * ≅ 10 11 M ☉ : 37 at z ∼ 0.4, 33 at z ∼ 0.9, and 31 at z = 2. A fourth sample with six infrared-luminous galaxies at z = 2 was observed for comparison with the purely mass-selected samples. From the fluxes detected in the stacked images for each sample, we find that the ISM content has decreased by a factor ∼6 from 1 to 2 × 10 10 M ☉ at both z = 2 and 0.9 down to ∼2 × 10 9 M ☉ at z = 0.4. The infrared-luminous sample at z = 2 shows a further ∼4 times increase in M ISM compared with the equivalent non-infrared-bright sample at the same redshift. The gas mass fractions are ∼2% ± 0.5%, 12% ± 3%, 14% ± 2%, and 53% ± 3% for the four subsamples (z = 0.4, 0.9, and 2 and infrared-bright galaxies).

  20. ALMA Observations of Elias 2–24: A Protoplanetary Disk with Multiple Gaps in the Ophiuchus Molecular Cloud

    Science.gov (United States)

    Cieza, Lucas A.; Casassus, Simon; Pérez, Sebastian; Hales, Antonio; Cárcamo, Miguel; Ansdell, Megan; Avenhaus, Henning; Bayo, Amelia; Bertrang, Gesa H.-M.; Cánovas, Hector; Christiaens, Valentin; Dent, William; Ferrero, Gabriel; Gamen, Roberto; Olofsson, Johan; Orcajo, Santiago; Osses, Axel; Peña-Ramirez, Karla; Principe, David; Ruíz-Rodríguez, Dary; Schreiber, Matthias R.; van der Plas, Gerrit; Williams, Jonathan P.; Zurlo, Alice

    2017-12-01

    We present ALMA 1.3 mm continuum observations at 0\\buildrel{\\prime\\prime}\\over{.} 2 (25 au) resolution of Elias 2–24, one of the largest and brightest protoplanetary disks in the Ophiuchus Molecular Cloud, and we report the presence of three partially resolved concentric gaps located at ∼20, 52, and 87 au from the star. We perform radiative transfer modeling of the disk to constrain its surface density and temperature radial profile and place the disk structure in the context of mechanisms capable of forming narrow gaps such as condensation fronts and dynamical clearing by actively forming planets. In particular, we estimate the disk temperature at the locations of the gaps to be 23, 15, and 12 K (at 20, 52, and 87 au, respectively), very close to the expected snowlines of CO (23–28 K) and N2 (12–15 K). Similarly, by assuming that the widths of the gaps correspond to 4–8× the Hill radii of forming planets (as suggested by numerical simulations), we estimate planet masses in the range of 0.2{--}1.5 {M}{Jup}, 1.0{--}8.0 {M}{Jup}, and 0.02{--}0.15 {M}{Jup} for the inner, middle, and outer gap, respectively. Given the surface density profile of the disk, the amount of “missing mass” at the location of each one of these gaps (between 4 and 20 {M}{Jup}) is more than sufficient to account for the formation of such planets.

  1. Diverse Nuclear Star-forming Activities in the Heart of NGC 253 Resolved with 10-pc-scale ALMA Images

    Science.gov (United States)

    Ando, Ryo; Nakanishi, Kouichiro; Kohno, Kotaro; Izumi, Takuma; Martín, Sergio; Harada, Nanase; Takano, Shuro; Kuno, Nario; Nakai, Naomasa; Sugai, Hajime; Sorai, Kazuo; Tosaki, Tomoka; Matsubayashi, Kazuya; Nakajima, Taku; Nishimura, Yuri; Tamura, Yoichi

    2017-11-01

    We present an 8 pc × 5 pc resolution view of the central ˜200 pc region of the nearby starburst galaxy NGC 253, based on ALMA Band 7 (λ ≃ 0.85 {mm} or ν ˜ 350 GHz) observations covering 11 GHz. We resolve the nuclear starburst of NGC 253 into eight dusty star-forming clumps, 10 pc in scale, for the first time. These clumps, each of which contains (4-10) × {10}4 {M}⊙ of dust (assuming that the dust temperature is 25 K) and up to 6× {10}2 massive (O5V) stars, appear to be aligned in two parallel ridges, while they have been blended in previous studies. Despite the similarities in sizes and dust masses of these clumps, their line spectra vary drastically from clump to clump, although they are separated by only ˜10 pc. Specifically, one of the clumps, Clump 1, exhibits line-confusion-limited spectra with at least 36 emission lines from 19 molecules (including CH3OH, HNCO, H2CO, CH3CCH, H2CS, and H3O+) and a hydrogen recombination line (H26α), while far fewer kinds of molecular lines are detected in some other clumps where fragile species, such as complex organic molecules and HNCO, completely disappear from their spectra. We demonstrate the existence of hot molecular gas ({T}{rot}({{SO}}2)=90+/- 11 K) in the former clump, which suggests that the hot and chemically rich environments are localized within a 10-pc-scale star-forming clump.

  2. The ALMA Frontier Fields Survey. I. 1.1 mm continuum detections in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223

    Science.gov (United States)

    González-López, J.; Bauer, F. E.; Romero-Cañizales, C.; Kneissl, R.; Villard, E.; Carvajal, R.; Kim, S.; Laporte, N.; Anguita, T.; Aravena, M.; Bouwens, R. J.; Bradley, L.; Carrasco, M.; Demarco, R.; Ford, H.; Ibar, E.; Infante, L.; Messias, H.; Muñoz Arancibia, A. M.; Nagar, N.; Padilla, N.; Treister, E.; Troncoso, P.; Zitrin, A.

    2017-01-01

    Context. Dusty star-forming galaxies are among the most prodigious systems at high redshift (z > 1), characterized by high star-formation rates and huge dust reservoirs. The bright end of this population has been well characterized in recent years, but considerable uncertainties remain for fainter dusty star-forming galaxies, which are responsible for the bulk of star formation at high redshift and thus play a key role in galaxy growth and evolution. Aims: In this first paper of our series, we describe our methods for finding high redshift faint dusty galaxies using millimeter observations with ALMA. Methods: We obtained ALMA 1.1 mm mosaic images for three strong-lensing galaxy clusters from the Frontier Fields Survey, which constitute some of the best studied gravitational lenses to date. The ≈2' × 2' mosaics overlap with the deep HST WFC3/IR footprints and encompass the high magnification regions of each cluster for maximum intrinsic source sensitivity. The combination of extremely high ALMA sensitivity and the magnification power of these clusters allows us to systematically probe the sub-mJy population of dusty star-forming galaxies over a large surveyed area. Results: We present a description of the reduction and analysis of the ALMA continuum observations for the galaxy clusters Abell 2744 (z = 0.308), MACS J0416.1-2403 (z = 0.396) and MACS J1149.5+2223 (z = 0.543), for which we reach observed rms sensitivities of 55, 59 and 71 μJy beam-1 respectively. We detect 12 dusty star-forming galaxies at S/N ≥ 5.0 across the three clusters, all of them presenting coincidence with near-infrared detected counterparts in the HST images. None of the sources fall close to the lensing caustics, thus they are not strongly lensed. The observed 1.1 mm flux densities for the total sample of galaxies range from 0.41 to 2.82 mJy, with observed effective radii spanning ≲0.̋05 to 0.̋37 ± 0.̋21 . The lensing-corrected sizes of the detected sources appear to be in the

  3. First Results from the $Herschel$ and ALMA Spectroscopic Surveys of the SMC: The Relationship Between [CII]-bright Gas and CO-bright Gas at Low Metallicity

    OpenAIRE

    Jameson, Katherine E.; Bolatto, Alberto D.; Wolfire, Mark; Warren, Steven R.; Herrera-Camus, Rodrigo; Croxall, Kevin; Pellegrini, Eric; Smith, John-David; Rubio, Monica; Indebetouw, Remy; Israel, Frank P.; Meixner, Margaret; Roman-Duval, Julia; van Loon, Jacco Th.; Muller, Erik

    2018-01-01

    The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present results from the Herschel Spectroscopic Survey of the SMC (HS$^{3}$), which mapped the key far-IR cooling lines [CII], [OI], [NII], and [OIII] in five star-forming regions, and new ALMA 7m-array maps of $^{12}$CO and $^{13}$CO $(2-1)$ with coverage overlapping four of the five HS$^{3}$ regions. We detect [CII] and [OI] throughout all of the r...

  4. ALMA observations of the nearby AGB star L2 Puppis II. Gas disk properties derived from 12CO and 13CO J = 3–2 emission

    OpenAIRE

    Homan, Ward; Richards, Anita; Decin, Leen; Kervella , Pierre; de Koter, Alex; Mcdonald, Iain; Ohnaka, Keiichi

    2017-01-01

    The circumstellar environment of the AGB star L2 Puppis was observed with ALMA in cycle 3, with a resolution of 15 × 18 mas. The molecular emission shows a differentially rotating disk, inclined to a nearly edge-on position. In the first paper in this series (Paper I) the molecular emission was analysed to accurately deduce the motion of the gas in the equatorial regions of the disk. In this work we model the optically thick 12CO J = 3-2 and the optically thin 13CO J = 3-2 rotational transiti...

  5. As potencialidades da personalidade-alma na reabilitação da linguagem e do pensamento: um estudo transdisciplinar de caso no SUS

    OpenAIRE

    Renata Paes de Barros

    2012-01-01

    Introdução: A clínica fonoaudiológica dentro do SUS, no interior paulista, é ainda muito pautada por um referencial reducionista, próprio da medicina convencional. A Antiga e Mística Ordem Rosae Crucis, AMORC, é uma escola do esoterismo ocidental, que veicula a Tradição Rosacruz. Nesta Tradição, “personalidade-alma” é a identidade psíquica da pessoa, uma “manifestação objetiva da reação individual à parte integrante da Alma Universal”. Este “Eu Interior” é dotado de grande potencial que pode ...

  6. MOLECULAR GAS ALONG A BRIGHT H α FILAMENT IN 2A 0335+096 REVEALED BY ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Vantyghem, A. N.; McNamara, B. R.; Hogan, M. T. [Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1 (Canada); Russell, H. R.; Fabian, A. C. [Institute of Astronomy, Madingley Road, Cambridge CB3 0HA (United Kingdom); Edge, A. C. [Department of Physics, Durham University, Durham DH1 3LE (United Kingdom); Nulsen, P. E. J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Combes, F.; Salomé, P. [LERMA, Observatoire de Paris, CNRS, UPMC, PSL Univ., 61 avenue de l’Observatoire, 75014 Paris (France); Baum, S. A.; O’Dea, C. P. [Department of Physics and Astronomy, University of Manitoba, Winnipeg, MB R3T 2N2 (Canada); Donahue, M.; Voit, G. M. [Department of Physics and Astronomy, Michigan State University, 567 Wilson Road, East Lansing, MI 48824 (United States); Main, R. A.; Murray, N. W.; Parrish, I. J [Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8 (Canada); O’Connell, R. W. [Department of Astronomy, University of Virginia, P.O. Box 400235, Charlottesville, VA 22904 (United States); Oonk, J. B. R. [ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, NL-7990 AA Dwingeloo (Netherlands); Sanders, J. S. [Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching (Germany); Tremblay, G., E-mail: a2vantyg@uwaterloo.ca [Department of Physics and Yale Center for Astronomy and Astrophysics, Yale University, 217 Prospect Street, New Haven, CT 06511 (United States)

    2016-12-01

    We present ALMA CO(1–0) and CO(3–2) observations of the brightest cluster galaxy (BCG) in the 2A 0335+096 galaxy cluster ( z  = 0.0346). The total molecular gas mass of 1.13 ± 0.15 × 10{sup 9} M {sub ⊙} is divided into two components: a nuclear region and a 7 kpc long dusty filament. The central molecular gas component accounts for 3.2 ± 0.4 × 10{sup 8} M {sub ⊙} of the total supply of cold gas. Instead of forming a rotationally supported ring or disk, it is composed of two distinct, blueshifted clumps south of the nucleus and a series of low-significance redshifted clumps extending toward a nearby companion galaxy. The velocity of the redshifted clouds increases with radius to a value consistent with the companion galaxy, suggesting that an interaction between these galaxies <20 Myr ago disrupted a pre-existing molecular gas reservoir within the BCG. Most of the molecular gas, 7.8 ± 0.9 × 10{sup 8} M {sub ⊙}, is located in the filament. The CO emission is co-spatial with a 10{sup 4} K emission-line nebula and soft X-rays from 0.5 keV gas, indicating that the molecular gas has cooled out of the intracluster medium over a period of 25–100 Myr. The filament trails an X-ray cavity, suggesting that the gas has cooled from low-entropy gas that has been lifted out of the cluster core and become thermally unstable. We are unable to distinguish between inflow and outflow along the filament with the present data. Cloud velocities along the filament are consistent with gravitational free-fall near the plane of the sky, although their increasing blueshifts with radius are consistent with outflow.

  7. The ALMA-PILS Survey: Formaldehyde deuteration in warm gas on small scales toward IRAS 16293-2422 B

    Science.gov (United States)

    Persson, M. V.; Jørgensen, J. K.; Müller, H. S. P.; Coutens, A.; van Dishoeck, E. F.; Taquet, V.; Calcutt, H.; van der Wiel, M. H. D.; Bourke, T. L.; Wampfler, S. F.

    2018-02-01

    Context. The enhanced degrees of deuterium fractionation observed in envelopes around protostars demonstrate the importance of chemistry at low temperatures, relevant in pre- and protostellar cores. Formaldehyde is an important species in the formation of methanol and more complex molecules. Aims: Here, we aim to present the first study of formaldehyde deuteration on small scales around the prototypical low-mass protostar IRAS 16293-2422 using high spatial and spectral resolution Atacama Large Millimeter/submillimeter Array (ALMA) observations. We determine the excitation temperature, abundances and fractionation level of several formaldehyde isotopologues, including its deuterated forms. Methods: Excitation temperature and column densities of formaldehyde in the gas close to one of the components of the binary were constrained through modeling of optically thin lines assuming local thermodynamical equilibrium. The abundance ratios were compared to results from previous single dish observations, astrochemical models and local ISM values. Results: Numerous isotopologues of formaldehyde are detected, among them H2C17O, and D213CO for the first time in the ISM. The large range of upper energy levels covered by the HDCO lines help constrain the excitation temperature to 106 ± 13 K. Using the derived column densities, formaldehyde shows a deuterium fractionation of HDCO/H2CO = 6.5 ± 1%, D2CO/HDCO = 12.8-4.1+3.3%, and D2CO/H2CO = 0.6(4) ± 0.1%. The isotopic ratios derived are 16O/18O = 805-79+43, 18O/17O = 3.2-0.3+0.2, and 12C/13C = 56-11+8. Conclusions: The HDCO/H2CO ratio is lower than that found in previous studies, highlighting the uncertainties involved in interpreting single dish observations of the inner warm regions. The D2CO/HDCO ratio is only slightly larger than the HDCO/H2CO ratio. This is consistent with formaldehyde forming in the ice as soon as CO has frozen onto the grains, with most of the deuteration happening toward the end of the prestellar core

  8. ALMA continuum observations of the protoplanetary disk AS 209. Evidence of multiple gaps opened by a single planet

    Science.gov (United States)

    Fedele, D.; Tazzari, M.; Booth, R.; Testi, L.; Clarke, C. J.; Pascucci, I.; Kospal, A.; Semenov, D.; Bruderer, S.; Henning, Th.; Teague, R.

    2018-02-01

    This paper presents new high angular resolution ALMA 1.3 mm dust continuum observations of the protoplanetary system AS 209 in the Ophiuchus star forming region. The dust continuum emission is characterized by a main central core and two prominent rings at r = 75 au and r = 130 au intervaled by two gaps at r = 62 au and r = 103 au. The two gaps have different widths and depths, with the inner one being narrower and shallower. We determined the surface density of the millimeter dust grains using the 3D radiative transfer disk code DALI. According to our fiducial model the inner gap is partially filled with millimeter grains while the outer gap is largely devoid of dust. The inferred surface density is compared to 3D hydrodynamical simulations (FARGO-3D) of planet-disk interaction. The outer dust gap is consistent with the presence of a giant planet (Mplanet 0.7 MSaturn); the planet is responsible for the gap opening and for the pile-up of dust at the outer edge of the planet orbit. The simulations also show that the same planet could be the origin of the inner gap at r = 62 au. The relative position of the two dust gaps is close to the 2:1 resonance and we have investigated the possibility of a second planet inside the inner gap. The resulting surface density (including location, width and depth of the two dust gaps) are in agreement with the observations. The properties of the inner gap pose a strong constraint to the mass of the inner planet (Mplanet age of the system (0.5-1 Myr), this result implies that the formation of giant planets occurs on a timescale of ≲1 Myr. The reduced image (FITS file) is only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/610/A24

  9. ALMA: the completion of the 25 Europeans antennas: focus on main performances, problems found during erection and lessons learned

    Science.gov (United States)

    Marchiori, Gianpietro; Rampini, Francesco; Giacomel, Luigino; Giacomel, Stefano; Marcuzzi, Enrico; Formentin, Federico

    2014-07-01

    The 2013 saw the completion of the Atacama Large Millimeter Array (ALMA). The array consists of 66 antennas and operates in Chile at the Chajnantor plateau at 5000 m altitude. 25 of the 12 meter diameter antennas have been delivered by the AEM consortium constituted by Thales Alenia Space France, Thales Alenia Space Italy, European Industrial Engineering (EIE GROUP), and MT Mechatronics. The purpose of this paper is to present a summary of the results obtained by the antennas during the different test campaign and a summary of the problems aroused during the erection and the assembly phases and the relative lesson learned. The results of the engineering performances and antenna systems, performed during the acceptance phases of the first antennas, have shown the full correspondence between what was expected during the design phase and what has been achieved in the final product, with a difference of less than 10% and the trend tends to be conservative. As for "on sky antennas performances", all the tests done in the 25 antennas showed excellent results. The antenna All Sky Pointing Error and Offset Pointing Error with and without metrology correction turned to be always excellent. The Fast Motion Capability with the tracking requirements after a step motion was better than an order of magnitude compared to the requests. Four years of on-site activities and the various phases of construction and assembly of 25 antennas have been a major challenge for the European Consortium. The problems encountered in this phase were many and varied: interfaces issues, design and foundation problems, manufacturing and assembly errors, electrical installation, shipment delays, human errors, adverse weather conditions, financial aspects, schedule, etc. The important is being prepared with an "a priori", that is a risk assessment which helps ensuring the best solution for the complete customer satisfaction of the scientific and technical requests. Despite the already excellent

  10. ALMA OBSERVATIONS OF THE GALACTIC CENTER: SiO OUTFLOWS AND HIGH-MASS STAR FORMATION NEAR Sgr A*

    Energy Technology Data Exchange (ETDEWEB)

    Yusef-Zadeh, F.; Royster, M.; Roberts, D. A. [Department of Physics and Astronomy and Center for Interdisciplinary Research in Astronomy, Northwestern University, Evanston, IL 60208 (United States); Wardle, M. [Department of Physics and Astronomy, and Centre for Astronomy, Astrophysics, and Astrophotonics, Macquarie University, Sydney, NSW 2109 (Australia); Arendt, R. [CREST/UMBC/NASA GSFC, Code 665, Greenbelt, MD 20771 (United States); Bushouse, H. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Lis, D. C. [California Institute of Technology, MC 320-47, Pasadena, CA 91125 (United States); Pound, M. W. [Department of Astronomy, University of Maryland, MD 20742 (United States); Whitney, B. [Space Science Institute, 4750 Walnut Street, Suite 205, Boulder, CO 80301 (United States); Wootten, A. [National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States)

    2013-04-20

    ALMA observations of the Galactic center with a spatial resolution of 2.''61 Multiplication-Sign 0.''97 resulted in the detection of 11 SiO (5-4) clumps of molecular gas within 0.6 pc (15'') of Sgr A*, interior to the 2 pc circumnuclear molecular ring. The three SiO (5-4) clumps closest to Sgr A* show the largest central velocities, {approx}150 km s{sup -1}, and the broadest asymmetric line widths with full width zero intensity (FWZI) {approx}110-147 km s{sup -1}. The remaining clumps, distributed mainly to the NE of the ionized mini-spiral, have narrow FWZI ({approx}18-56 km s{sup -1}). Using CARMA SiO (2-1) data, Large Velocity Gradient modeling of the SiO line ratios for the broad velocity clumps constrains the column density N(SiO) {approx}10{sup 14} cm{sup -2}, and the H{sub 2} gas density n{sub H{sub 2}} = (3-9) x 10{sup 5} cm{sup -3} for an assumed kinetic temperature 100-200 K. The SiO clumps are interpreted as highly embedded protostellar outflows, signifying an early stage of massive star formation near Sgr A* in the last 10{sup 4}-10{sup 5} yr. Support for this interpretation is provided by the SiO (5-4) line luminosities and velocity widths which lie in the range measured for protostellar outflows in star-forming regions in the Galaxy. Furthermore, spectral energy distribution modeling of stellar sources shows two young stellar object candidates near SiO clumps, supporting in situ star formation near Sgr A*. We discuss the nature of star formation where the gravitational potential of the black hole dominates. In particular, we suggest that external radiative pressure exerted on self-shielded molecular clouds enhances the gas density, before the gas cloud becomes gravitationally unstable near Sgr A*. Alternatively, collisions between clumps in the ring may trigger gravitational collapse.

  11. Avaliação de clones de bananeira do subgrupo Cavendish (Musa acuminata, AAA em Cruz das Almas-BA Evaluation of banana Cavendish clones in Cruz das Almas City, Bahia State, Brazil

    Directory of Open Access Journals (Sweden)

    Sebastião de Oliveira e Silva

    2004-12-01

    Full Text Available Foram avaliados em Cruz das Almas-BA, em dois ciclos, 69 clones Cavendish coletados em São Paulo, Minas Gerais, Bahia e Santa Catarina, sendo 49 do tipo Nanicão e 20 do tipo Grande Naine. Os clones foram estabelecidos em área experimental da Embrapa Mandioca e Fruticultura utilizando-se um delineamento em blocos ao acaso com cinco repetições e cinco plantas por parcela. Foram utilizados a irrigação por microaspersão, o espaçamento de 3,0 m x 2,0 m e um sistema de condução com três plantas/touceira. Os requerimentos agronômicos foram aplicados conforme preconizados para o cultivo. Na avaliação dos clones, foram consideradas as seguintes variáveis: altura da planta em centímetros (AP; número de dias do plantio à colheita (ND; peso do cacho em quilogramas (PC; número de frutos por cacho (NF; e comprimento do fruto em centímetros (CF. Pelos resultados obtidos, verificou-se uma variabilidade média em todas as variáveis avaliadas. Por apresentarem caracteres superiores, foram selecionados cinco clones de Grande Naine (G.N. Taperão, G.N.Rossete, G.N. Willians, G.N. Magário, G.N. SC-074 e quatro de Nanicão (N. IAC Abóbada Verde, N. Rossete, N. SC-0008 e N. SC-063.Sixty-nine clones of Cavendish type bananas (49 Nanicão and 20 Grande Naine collected in the States of São Paulo, Minas Gerais, Bahia and Santa Catarina were evaluated. The clones were established in an experimental area at the Cassava and Fruit Crops Research Center - EMBRAPA, using micro-aspersion irrigation, in plants spaced at 3.0 m x 2.0 m, and conducted with three plants/bushes. Random blocks were used with five replications and five plants per plot. All cultural requirements for the crop were carried out. For the clone evaluations, the following variables were considered: plant height in centimeters (PH; number of days from planting to yield (ND; weight of bunch in kilograms (WB; number of fruits per bunch (FB and length of fruit in centimeters (LF. The

  12. Study of the aluminium content in AGB winds using ALMA. Indications for the presence of gas-phase (Al2O3)n clusters

    Science.gov (United States)

    Decin, L.; Richards, A. M. S.; Waters, L. B. F. M.; Danilovich, T.; Gobrecht, D.; Khouri, T.; Homan, W.; Bakker, J. M.; Van de Sande, M.; Nuth, J. A.; De Beck, E.

    2017-12-01

    Context. The condensation of inorganic dust grains in the winds of evolved stars is poorly understood. As of today, it is not yet known which molecular clusters form the first dust grains in oxygen-rich (C/O histories in the winds of oxygen-rich AGB stars. Methods: We obtained Atacama Large Millimeter/sub-millimeter array (ALMA) observations with a spatial resolution of 120 × 150 mas tracing the dust formation region of the low mass-loss rate AGB star, R Dor, and the high mass-loss rate AGB star, IK Tau. We detected emission line profiles of AlO, AlOH, and AlCl in the ALMA data and used these line profiles to derive a lower limit of atomic aluminium incorporated in molecules. This constrains the aluminium budget that can condense into grains. Results: Radiative transfer models constrain the fractional abundances of AlO, AlOH, and AlCl in IK Tau and R Dor. We show that the gas-phase aluminium chemistry is completely different in both stars with a remarkable difference in the AlO and AlOH abundance stratification. The amount of aluminium locked up in these three molecules is small, ≤1.1 × 10-7 w.r.t. H2, for both stars, i.e. only ≤2% of the total aluminium budget. An important result is that AlO and AlOH, which are the direct precursors of alumina (Al2O3) grains, are detected well beyond the onset of the dust condensation, which proves that the aluminium oxide condensation cycle is not fully efficient. The ALMA observations allow us to quantitatively assess the current generation of theoretical dynamical-chemical models for AGB winds. We discuss how the current proposed scenario of aluminium dust condensation for low mass-loss rate AGB stars within a few stellar radii from the star, in particular for R Dor and W Hya, poses a challenge if one wishes to explain both the dust spectral features in the spectral energy distribution (SED) in interferometric data and in the polarized light signal. In particular, the estimated grain temperature of Al2O3 is too high for

  13. Solar Research with ALMA

    Czech Academy of Sciences Publication Activity Database

    Karlický, Marian; Bárta, Miroslav; Dabrowski, Bartosz Premyslaw; Heinzel, Petr

    2011-01-01

    Roč. 268, č. 1 (2011), s. 165-173 ISSN 0038-0938 R&D Projects: GA AV ČR IAA300030701; GA ČR GAP209/10/1680 Institutional research plan: CEZ:AV0Z10030501 Keywords : Sun * atmosphere * radio radiation * radioheliograph Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 2.776, year: 2011

  14. Adding Support to the ALMA Common Software for Real-Time Operations through the Usage of a POSIX-Compliant RTOS

    Science.gov (United States)

    Tobar, R. J.; von Brand, H.; Araya, M. A.; Juerges, T.

    2010-12-01

    The ALMA Common Software (ACS) framework lacks of the real-time capabilities to control the antennas’ instrumentation — as has been probed by previous works — which has lead to non-portable workarounds to the problem. Indeed, the time service used in ACS, based in the Container/Component model, presents plenty of results that confirm this statement. This work addresses the problem of design and integrate a real-time service for ACS, providing to the framework an implementation such that the control operations over the different instruments could be done within real-time constraints. This implementation is compared with the current time service, showing the difference between the two systems when subjecting them to common scenarios. Also, the new implementation is done following the POSIX specification, ensuring interoperability and portability through different operating systems.

  15. Composição florística da floresta estacional decídua montana de Serra das Almas, CE, Brasil

    OpenAIRE

    Lima,Jacira Rabelo; Sampaio,Everardo Valadares de Sá Barretto; Rodal,Maria Jesus Nogueira; Araújo,Francisca Soares

    2009-01-01

    No domínio semi-árido brasileiro, a flora das bacias sedimentares ainda é pouco conhecida, mas os levantamentos já existentes indicam que há grande heterogeneidade florística e fisionômica. Mesmo áreas geográficas próximas podem apresentar dissimilaridade florística. Visando testar esta hipótese, a composição florística e o espectro biológico da floresta estacional decídua de Serra das Almas, estado do Ceará, foram analisados e comparados com os de 14 áreas sedimentares no Nordeste. Foram enc...

  16. [Almas delirantes (1925) by Luís Cebola: the poetics of the human psyche and the physician as mediator between the universe of mental illness and society].

    Science.gov (United States)

    Pereira, Denise

    2018-03-01

    Lúis Cebola's 1925 work Almas delirantes [Delusional Souls] presented various psychopathologies through metaphorical and lyrical portraits rather than from a medical/ scientific point of view, showing that he perceived his patients as more than objects of scientific study in a process of identification, empathy, and compassion. Cebola defined psychopathological states according to contrast with normality, but stressed that these diseases could arise in any individual, and the book simultaneously acted as a warning to readers. The text also publicized the Museum of Madness [Museu da Loucura], which he created at the Casa de Saúde do Telhal, and the art produced by his patients, positioning himself as a messenger between the closed universe of the psychiatric hospital and Portuguese society.

  17. Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herscheltype="fn" rid="fn1" />

    Science.gov (United States)

    Dye, S.; Furlanetto, C.; Dunne, L.; Eales, S. A.; Negrello, M.; Nayyeri, H.; van der Werf, P. P.; Serjeant, S.; Farrah, D.; Michałowski, M. J.; Baes, M.; Marchetti, L.; Cooray, A.; Riechers, D. A.; Amvrosiadis, A.

    2018-02-01

    We have modelled ˜0.1 arcsec resolution ALMA imaging of six strong gravitationally lensed galaxies detected by the Herschel Space Observatory. Our modelling recovers mass properties of the lensing galaxies and, by determining magnification factors, intrinsic properties of the lensed sub-millimetre sources. We find that the lensed galaxies all have high ratios of star formation rate to dust mass, consistent with or higher than the mean ratio for high redshift sub-millimetre galaxies and low redshift ultra-luminous infra-red galaxies. Source reconstruction reveals that most galaxies exhibit disturbed morphologies. Both the cleaned image plane data and the directly observed interferometric visibilities have been modelled, enabling comparison of both approaches. In the majority of cases, the recovered lens models are consistent between methods, all six having mass density profiles that are close to isothermal. However, one system with poor signal to noise shows mildly significant differences.

  18. A desmaterialização do corpo: da alma (analógica à informação (digital

    Directory of Open Access Journals (Sweden)

    Paula Sibilia

    2008-09-01

    Full Text Available Apresenta-se aqui uma reflexão acerca da persistência da visão dualista do ser humano: a possibilidade de uma subjetividade descarnada, uma idéia perfeitamente datada, parece continuar vigente na sociedade contemporânea. Se até pouco tempo atrás os corpos eram aprisionados pela alma (uma entidade opaca e analógica, hoje é a informação digital que os amordaça e os torna manipuláveis. Essa informação imaterial que comanda os corpos assume diversas formas: do código genético aos circuitos cerebrais e à imagem do “corpo perfeito”.

  19. KINEMATIC STRUCTURE OF MOLECULAR GAS AROUND HIGH-MASS YSO, PAPILLON NEBULA, IN N159 EAST IN THE LARGE MAGELLANIC CLOUD: A NEW PERSPECTIVE WITH ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Saigo, Kazuya; Harada, Ryohei; Kawamura, Akiko [Chile Observatory, National Astronomical Observatory of Japan, National Institutes of Natural Science, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Onishi, Toshikazu; Tokuda, Kazuki; Morioka, Yuuki [Department of Physical Science, Graduate School of Science, Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531 (Japan); Nayak, Omnarayani; Meixner, Margaret [The Johns Hopkins University, Department of Physics and Astronomy, 366 Bloomberg Center, 3400 N. Charles Street, Baltimore, MD 21218 (United States); Sewiło, Marta [NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States); Indebetouw, Remy [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Torii, Kazufumi; Ohama, Akio; Hattori, Yusuke; Yamamoto, Hiroaki; Tachihara, Kengo [Department of Physics, Nagoya University, Chikusa-ku, Nagoya 464-8602 (Japan); Minamidani, Tetsuhiro [Nobeyama Radio Observatory, 462-2 Nobeyama Minamimaki-mura, Minamisaku-gun, Nagano 384-1305 (Japan); Inoue, Tsuyoshi [Division of Theoretical Astronomy, National Astronomical Observatory (Japan); Madden, Suzanne; Lebouteiller, Vianney [Laboratoire AIM, CEA, Universite Paris VII, IRFU/Service d’Astrophysique, Bat. 709, F-91191 Gif-sur-Yvette (France); Galametz, Maud [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); and others

    2017-01-20

    We present the ALMA Band 3 and Band 6 results of {sup 12}CO(2-1), {sup 13}CO(2-1), H30 α recombination line, free–free emission around 98 GHz, and the dust thermal emission around 230 GHz toward the N159 East Giant Molecular Cloud (N159E) in the Large Magellanic Cloud (LMC). LMC is the nearest active high-mass star-forming face-on galaxy at a distance of 50 kpc and is the best target for studing high-mass star formation. ALMA observations show that N159E is the complex of filamentary clouds with the width and length of ∼1 pc and several parsecs. The total molecular mass is 0.92 × 10{sup 5} M {sub ⊙} from the {sup 13}CO(2-1) intensity. N159E harbors the well-known Papillon Nebula, a compact high-excitation H ii region. We found that a YSO associated with the Papillon Nebula has the mass of 35 M {sub ⊙} and is located at the intersection of three filamentary clouds. It indicates that the formation of the high-mass YSO was induced by the collision of filamentary clouds. Fukui et al. reported a similar kinematic structure toward two YSOs in the N159 West region, which are the other YSOs that have the mass of ≳35 M {sub ⊙}. This suggests that the collision of filamentary clouds is a primary mechanism of high-mass star formation. We found a small molecular hole around the YSO in Papillon Nebula with a sub-parsec scale. It is filled by free–free and H30 α emission. The temperature of the molecular gas around the hole reaches ∼80 K. It indicates that this YSO has just started the distruction of parental molecular cloud.

  20. ALMA Observation of 158 μm [C II] Line and Dust Continuum of a z = 7 Normally Star-forming Galaxy in the Epoch of Reionization

    Science.gov (United States)

    Ota, Kazuaki; Walter, Fabian; Ohta, Kouji; Hatsukade, Bunyo; Carilli, Chris L.; da Cunha, Elisabete; González-López, Jorge; Decarli, Roberto; Hodge, Jacqueline A.; Nagai, Hiroshi; Egami, Eiichi; Jiang, Linhua; Iye, Masanori; Kashikawa, Nobunari; Riechers, Dominik A.; Bertoldi, Frank; Cox, Pierre; Neri, Roberto; Weiss, Axel

    2014-09-01

    We present ALMA observations of the [C II] line and far-infrared (FIR) continuum of a normally star-forming galaxy in the reionization epoch, the z = 6.96 Lyα emitter (LAE) IOK-1. Probing to sensitivities of σline = 240 μJy beam-1 (40 km s-1 channel) and σcont = 21 μJy beam-1, we found the galaxy undetected in both [C II] and continuum. Comparison of ultraviolet (UV)-FIR spectral energy distribution (SED) of IOK-1, including our ALMA limit, with those of several types of local galaxies (including the effects of the cosmic microwave background, CMB, on the FIR continuum) suggests that IOK-1 is similar to local dwarf/irregular galaxies in SED shape rather than highly dusty/obscured galaxies. Moreover, our 3σ FIR continuum limit, corrected for CMB effects, implies intrinsic dust mass M dust LAEs on the L [C II] versus SFR and L [C II]/L FIR versus L FIR diagrams imply that LAEs in the reionization epoch have significantly lower gas and dust enrichment than AGN-powered systems and starbursts at similar/lower redshifts, as well as local star-forming galaxies. Based in part on data collected with the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555; and observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

  1. THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: IMPLICATIONS FOR SPECTRAL LINE INTENSITY MAPPING AT MILLIMETER WAVELENGTHS AND CMB SPECTRAL DISTORTIONS

    Energy Technology Data Exchange (ETDEWEB)

    Carilli, C. L.; Walter, F. [National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801 (United States); Chluba, J. [Jodrell Bank Centre for Astrophysics, University of Manchester, Oxford Road, M13 9PL (United Kingdom); Decarli, R. [Max-Planck Institute for Astronomy, D-69117 Heidelberg (Germany); Aravena, M. [Nucleo de Astronomia, Facultad de Ingenieria, Universidad Diego Portales, Av. Ejercito 441, Santiago (Chile); Wagg, J. [Square Kilometre Array Organisation, Lower Withington, Cheshire (United Kingdom); Popping, G. [European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748, Garching (Germany); Cortes, P. [Joint ALMA Observatory—ESO, Av. Alonso de Cordova, 3104, Santiago (Chile); Hodge, J. [Leiden Observatory, Leiden University, Niels Bohrweg 2, NL2333 RA Leiden (Netherlands); Weiss, A. [Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany); Bertoldi, F. [Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, D-53121 Bonn (Germany); Riechers, D., E-mail: ccarilli@aoc.nrao.edu [Cornell University, 220 Space Sciences Building, Ithaca, NY 14853 (United States)

    2016-12-10

    We present direct estimates of the mean sky brightness temperature in observing bands around 99 and 242 GHz due to line emission from distant galaxies. These values are calculated from the summed line emission observed in a blind, deep survey for spectral line emission from high redshift galaxies using ALMA (the ALMA spectral deep field observations “ASPECS” survey). In the 99 GHz band, the mean brightness will be dominated by rotational transitions of CO from intermediate and high redshift galaxies. In the 242 GHz band, the emission could be a combination of higher order CO lines, and possibly [C ii] 158 μ m line emission from very high redshift galaxies ( z  ∼ 6–7). The mean line surface brightness is a quantity that is relevant to measurements of spectral distortions of the cosmic microwave background, and as a potential tool for studying large-scale structures in the early universe using intensity mapping. While the cosmic volume and the number of detections are admittedly small, this pilot survey provides a direct measure of the mean line surface brightness, independent of conversion factors, excitation, or other galaxy formation model assumptions. The mean surface brightness in the 99 GHZ band is: T{sub B}  = 0.94 ± 0.09 μ K. In the 242 GHz band, the mean brightness is: T{sub B}  = 0.55 ± 0.033 μ K. These should be interpreted as lower limits on the average sky signal, since we only include lines detected individually in the blind survey, while in a low resolution intensity mapping experiment, there will also be the summed contribution from lower luminosity galaxies that cannot be detected individually in the current blind survey.

  2. ALMA observations of the host galaxy of GRB 090423 at z = 8.23: deep limits on obscured star formation 630 million years after the big bang

    Energy Technology Data Exchange (ETDEWEB)

    Berger, E.; Zauderer, B. A.; Chary, R.-R.; Laskar, T.; Chornock, R.; Davies, J. E. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Tanvir, N. R. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH (United Kingdom); Stanway, E. R.; Levan, A. J. [Department of Physics, University of Warwick, Gibbet Hill Road, Coventry CV4 7AL (United Kingdom); Levesque, E. M. [CASA, University of Colorado UCB 389, Boulder, CO 80309 (United States)

    2014-12-01

    We present rest-frame far-infrared (FIR) and optical observations of the host galaxy of GRB 090423 at z = 8.23 from the Atacama Large Millimeter Array (ALMA) and the Spitzer Space Telescope, respectively. The host remains undetected to 3σ limits of F {sub ν}(222 GHz) ≲ 33 μJy and F {sub ν}(3.6 μm) ≲ 81 nJy. The FIR limit is about 20 times fainter than the luminosity of the local ULIRG Arp 220 and comparable to the local starburst M 82. Comparing this with model spectral energy distributions, we place a limit on the infrared (IR) luminosity of L {sub IR}(8-1000 μm) ≲ 3 × 10{sup 10} L {sub ☉}, corresponding to a limit on the obscured star formation rate of SFR{sub IR}≲5 M {sub ☉} yr{sup –1}. For comparison, the limit on the unobscured star formation rate from Hubble Space Telescope rest-frame ultraviolet (UV) observations is SFR{sub UV} ≲ 1 M {sub ☉} yr{sup –1}. We also place a limit on the host galaxy stellar mass of M {sub *} ≲ 5 × 10{sup 7} M {sub ☉} (for a stellar population age of 100 Myr and constant star formation rate). Finally, we compare our millimeter observations to those of field galaxies at z ≳ 4 (Lyman break galaxies, Lyα emitters, and submillimeter galaxies) and find that our limit on the FIR luminosity is the most constraining to date, although the field galaxies have much larger rest-frame UV/optical luminosities than the host of GRB 090423 by virtue of their selection techniques. We conclude that GRB host galaxies at z ≳ 4, especially those with measured interstellar medium metallicities from afterglow spectroscopy, are an attractive sample for future ALMA studies of high redshift obscured star formation.

  3. An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling

    Science.gov (United States)

    Miettinen, O.; Delvecchio, I.; Smolčić, V.; Aravena, M.; Brisbin, D.; Karim, A.; Magnelli, B.; Novak, M.; Schinnerer, E.; Albrecht, M.; Aussel, H.; Bertoldi, F.; Capak, P. L.; Casey, C. M.; Hayward, C. C.; Ilbert, O.; Intema, H. T.; Jiang, C.; Le Fèvre, O.; McCracken, H. J.; Muñoz Arancibia, A. M.; Navarrete, F.; Padilla, N. D.; Riechers, D. A.; Salvato, M.; Scott, K. S.; Sheth, K.; Tasca, L. A. M.

    2017-09-01

    Context. Submillimetre galaxies (SMGs) represent an important source population in the origin and cosmic evolution of the most massive galaxies. Hence, it is imperative to place firm constraints on the fundamental physical properties of large samples of SMGs. Aims: We determine the physical properties of a sample of SMGs in the COSMOS field that were pre-selected at the observed-frame wavelength of λobs = 1.1 mm, and followed up at λobs = 1.3 mm with the Atacama Large Millimetre/submillimetre Array (ALMA). Methods: We used the MAGPHYS model package to fit the panchromatic (ultraviolet to radio) spectral energy distributions (SEDs) of 124 of the target SMGs, which lie at a median redshift of z = 2.30 (19.4% are spectroscopically confirmed). The SED analysis was complemented by estimating the gas masses of the SMGs by using the λobs = 1.3 mm dust emission as a tracer of the molecular gas component. Results: The sample median and 16th-84th percentile ranges of the stellar masses, obscured star formation rates, dust temperatures, and dust and gas masses were derived to be log(M⋆/M⊙) = 11.09+0.41-0.53, SFR = 402+661-233 M⊙ yr-1, Tdust = 39.7+9.7-7.4 K, log(Mdust/M⊙) = 9.01+0.20-0.31, and log(Mgas/M⊙ = 11.34+0.20-0.23, respectively. The Mdust/M⋆ ratio was found to decrease as a function of redshift, while the Mgas/Mdust ratio shows the opposite, positive correlation with redshift. The derived median gas-to-dust ratio of 120+73-30 agrees well with the canonical expectation. The gas fraction (Mgas/ (Mgas + M⋆)) was found to range from 0.10 to 0.98 with a median of 0.62+0.27-0.23. We found that 57.3% of our SMGs populate the main sequence (MS) of star-forming galaxies, while 41.9% of the sources lie above the MS by a factor of greater than three (one source lies below the MS). These super-MS objects, or starbursts, are preferentially found at z ≳ 3, which likely reflects the sensitivity limit of our source selection. We estimated that the median gas

  4. O nível de complexidade da alma humana: tradução e comentários de um texto de Tomás de Aquino

    OpenAIRE

    Amatuzzi, Mauro Martins

    2017-01-01

    Este trabalho apresenta uma tradução do primeiro artigo da Questão Disputada de Tomás de Aquino Sobre a Alma (QD de Anima, art.1), seguida de comentários. O problema discutido diz respeito a como conciliar a concepção da alma humana como algo subsistente com a concepção segundo a qual ela é apenas a estrutura do organismo físico. Este problema põe em confronto um monismo materialista com um dualismo espiritualista. Tomás de Aquino retém a intuição subjacente de cada uma dessas posições mas nã...

  5. ALMA observation of 158 μm [C II] line and dust continuum of a z = 7 normally star-forming galaxy in the epoch of reionization

    International Nuclear Information System (INIS)

    Ota, Kazuaki; Walter, Fabian; Da Cunha, Elisabete; González-López, Jorge; Decarli, Roberto; Hodge, Jacqueline A.; Ohta, Kouji; Hatsukade, Bunyo; Nagai, Hiroshi; Iye, Masanori; Kashikawa, Nobunari; Carilli, Chris L.; Egami, Eiichi; Jiang, Linhua; Riechers, Dominik A.; Bertoldi, Frank; Cox, Pierre; Neri, Roberto; Weiss, Axel

    2014-01-01

    We present ALMA observations of the [C II] line and far-infrared (FIR) continuum of a normally star-forming galaxy in the reionization epoch, the z = 6.96 Lyα emitter (LAE) IOK-1. Probing to sensitivities of σ line = 240 μJy beam –1 (40 km s –1 channel) and σ cont = 21 μJy beam –1 , we found the galaxy undetected in both [C II] and continuum. Comparison of ultraviolet (UV)-FIR spectral energy distribution (SED) of IOK-1, including our ALMA limit, with those of several types of local galaxies (including the effects of the cosmic microwave background, CMB, on the FIR continuum) suggests that IOK-1 is similar to local dwarf/irregular galaxies in SED shape rather than highly dusty/obscured galaxies. Moreover, our 3σ FIR continuum limit, corrected for CMB effects, implies intrinsic dust mass M dust < 6.4 × 10 7 M ☉ , FIR luminosity L FIR < 3.7 × 10 10 L ☉ (42.5-122.5 μm), total IR luminosity L IR < 5.7 × 10 10 L ☉ (8-1000 μm), and dust-obscured star formation rate (SFR) < 10 M ☉ yr –1 , if we assume that IOK-1 has a dust temperature and emissivity index typical of local dwarf galaxies. This SFR is 2.4 times lower than one estimated from the UV continuum, suggesting that <29% of the star formation is obscured by dust. Meanwhile, our 3σ [C II] flux limit translates into [C II] luminosity, L [C II] < 3.4 × 10 7 L ☉ . Locations of IOK-1 and previously observed LAEs on the L [C II] versus SFR and L [C II] /L FIR versus L FIR diagrams imply that LAEs in the reionization epoch have significantly lower gas and dust enrichment than AGN-powered systems and starbursts at similar/lower redshifts, as well as local star-forming galaxies.

  6. ALMA 26 arcmin2 Survey of GOODS-S at One-millimeter (ASAGAO): X-Ray AGN Properties of Millimeter-selected Galaxies

    Science.gov (United States)

    Ueda, Y.; Hatsukade, B.; Kohno, K.; Yamaguchi, Y.; Tamura, Y.; Umehata, H.; Akiyama, M.; Ao, Y.; Aretxaga, I.; Caputi, K.; Dunlop, J. S.; Espada, D.; Fujimoto, S.; Hayatsu, N. H.; Imanishi, M.; Inoue, A. K.; Ivison, R. J.; Kodama, T.; Lee, M. M.; Matsuoka, K.; Miyaji, T.; Morokuma-Matsui, K.; Nagao, T.; Nakanishi, K.; Nyland, K.; Ohta, K.; Ouchi, M.; Rujopakarn, W.; Saito, T.; Tadaki, K.; Tanaka, I.; Taniguchi, Y.; Wang, T.; Wang, W.-H.; Yoshimura, Y.; Yun, M. S.

    2018-01-01

    We investigate the X-ray active galactic nucleus (AGN) properties of millimeter galaxies in the Great Observatories Origins Deep Survey South (GOODS-S) field detected with the Atacama Large Millimeter/submillimeter Array (ALMA), by utilizing the Chandra 7-Ms data, the deepest X-ray survey to date. Our millimeter galaxy sample comes from the ASAGAO survey covering 26 arcmin2 (12 sources at a 1.2 mm flux-density limit of ≈ 0.6 mJy), supplemented by the deeper but narrower 1.3 mm survey of a part of the ASAGAO field by Dunlop et al. Ofthe 25 total millimeter galaxies, 14 have Chandra counterparts. The observed AGN fractions at z=1.5{--}3 are found to be {90}-19+8% and {57}-25+23% for the ultra-luminous and luminous infrared galaxies with log {L}{IR}/{L}ȯ = 12–12.8 and log {L}{IR}/{L}ȯ = 11.5–12, respectively. The majority (∼2/3) of the ALMA and/or Herschel detected X-ray AGNs at z = 1.5‑3 appear to be star-formation-dominant populations, having {L}{{X}}/ {L}{IR} ratios smaller than the “simultaneous evolution” value expected from the local black-hole-mass-to-stellar-mass ({M}{BH}–M *) relation. On the basis of the {L}{{X}} and stellar mass relation, we infer that a large fraction of star-forming galaxies at z=1.5{--}3 have black hole masses that are smaller than those expected from the local {M}{BH}–M * relation. This contrasts previous reports on luminous AGNs at the same redshifts detected in wider and shallower surveys, which are subject to selection biases against lower luminosity AGNs. Our results are consistent with an evolutionary scenario in which star formation occurs first, and an AGN-dominant phase follows later, in objects that finally evolve into galaxies with classical bulges.

  7. Patología, escritura y género en el fin de siglo: Alma contemporánea y Manual del perfecto enfermo

    Directory of Open Access Journals (Sweden)

    Alba del Pozo García

    2015-11-01

    Full Text Available Este artículo aborda dos ensayos españoles sobre la enfermedad publicados en el cambio de siglo XIX-XX, de José María Llanas Aguilaniedo (Alma contemporánea, 1899 y de Rafael Urbano (Manual del perfecto enfermo, 1911. Se examina el modo en el que asumen la neurosis masculina como una manifestación positiva e inevitable de la vida moderna, en línea con el ambiente cultural de un fin de siglo marcado por los discursos médicos y la correlación que establecen entre el genio, la producción artística y las patologías psiquiátricas. Ambos textos se identifican con la retórica clínica y plantean un propósito curativo explícito. Sin embargo, en lugar de limitarse a reproducir el binomio enfermo/sano, lo van a problematizar, puesto que la categoría de enfermedad que desarrollan se va a desligar del modelo médico para desplazarse al terreno de la subjetividad, la escritura y la identidad. This paper analyses two Spanish essays on illness published during the fin de siècle: José María Llanas Aguilaniedo’s 1899 Alma contemporánea and Rafael Urbano’s 1911 Manual del perfecto enfermo. The focus lies on how masculine neurosis is read as a sign of modern struggles in a fin de siècle culture characterized by the hegemony of medical discourses and the relationship between genius, artistic production, and psychiatric pathologies. Both texts are associated to medical discourses and suggest healing strategies. In this scope, the typical ill/health opposition undergoes a critical turn. In fact, these texts depict a notion of illness that undermines medical rhetoric, placing illness in the field of subjectivity, writing and identity.

  8. AVALIAÇÃO DAS CONDIÇÕES HIGIÊNICO-SANITÁRIAS DO PESCADO COMERCIALIZADO NO MUNICÍPIO DE CRUZ DAS ALMAS, BAHIA

    Directory of Open Access Journals (Sweden)

    NORMA SUELY EVANGELISTA BARRETO

    2012-01-01

    Full Text Available The goal of paper was to evaluate the quality of fish commercialized in supermarkets and marketplace stalls in Cruz das Almas, Bahia. Sensorial, physicochemical and microbiological analysis were performed in 11 fish samples (three fresh fish samples, four frozen fish samples, and four dry salted fish samples. Supermarkets presented better hygiene conditions and facilities, and offered staff training. In the market stalls the facilities were in disagreement with food legislation. The sensorial analysis indicated tha 60% of the samples were in accordance with the concept of freshness. Hundred percent of the fresh and frozen fish samples were negative for sulphydric gas reaction, and humidity varied from 65.79 to 81.59%. Humidity in all the dry salted fish samples was higher than the maximum values allowed, and the chloride test was 1.1 × 103 MPN g-1. Escherichia coli (08 was isolated only from fish samples collected in the marketplace stalls and was resistant to eritromicine 08 (100%, amicacyn 02 (25%, ampicillin, cephalotin and tetracycline 01 (12.5%. Multiresistance profile was observed in 62.5% of the isolates.

  9. Kodaly Yönteminin İlköğretim Öğrencilerinin Keman Çalma Becerisi Üzerindeki Etkisi

    OpenAIRE

    Yıldırım, Kemal; YILDIRIM, Kemal

    2014-01-01

    Bu araştırmanın amacı, Kodaly yönteminin ilköğretim öğrencilerinin keman çalma becerisi üzerindeki etkisini araştırmaktır. Ön test-son test kontrol gruplu yarı deneysel desenin kullanıldığı bu araştırmada, 2007-2008 öğretim yılı bahar döneminde İzmir ilinde özel bir ilköğretim okulu’nda daha önceden herhangi bir çalgı eğitimi almamış 3,4 ve 5. sınıflarda öğrenim gören öğrenciler içinden; tek ses tekrarlama becerisi, ezgi tekrarlama becerisi, ritim tekrarlama becerisi, şarkı söyleme becerisi, ...

  10. ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Luminosity Functions and the Evolution of the Cosmic Density of Molecular Gas

    Science.gov (United States)

    Decarli, Roberto; Walter, Fabian; Aravena, Manuel; Carilli, Chris; Bouwens, Rychard; da Cunha, Elisabete; Daddi, Emanuele; Ivison, R. J.; Popping, Gergö; Riechers, Dominik; Smail, Ian R.; Swinbank, Mark; Weiss, Axel; Anguita, Timo; Assef, Roberto J.; Bauer, Franz E.; Bell, Eric F.; Bertoldi, Frank; Chapman, Scott; Colina, Luis; Cortes, Paulo C.; Cox, Pierre; Dickinson, Mark; Elbaz, David; Gónzalez-López, Jorge; Ibar, Edo; Infante, Leopoldo; Hodge, Jacqueline; Karim, Alex; Le Fevre, Olivier; Magnelli, Benjamin; Neri, Roberto; Oesch, Pascal; Ota, Kazuaki; Rix, Hans-Walter; Sargent, Mark; Sheth, Kartik; van der Wel, Arjen; van der Werf, Paul; Wagg, Jeff

    2016-12-01

    In this paper we use ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field in band 3 and band 6, to place blind constraints on the CO luminosity function and the evolution of the cosmic molecular gas density as a function of redshift up to z ˜ 4.5. This study is based on galaxies that have been selected solely through their CO emission and not through any other property. In all of the redshift bins the ASPECS measurements reach the predicted “knee” of the CO luminosity function (around 5 × 109 K km s-1 pc2). We find clear evidence of an evolution in the CO luminosity function with respect to z ˜ 0, with more CO-luminous galaxies present at z ˜ 2. The observed galaxies at z ˜ 2 also appear more gas-rich than predicted by recent semi-analytical models. The comoving cosmic molecular gas density within galaxies as a function of redshift shows a drop by a factor of 3-10 from z ˜ 2 to z ˜ 0 (with significant error bars), and possibly a decline at z > 3. This trend is similar to the observed evolution of the cosmic star formation rate density. The latter therefore appears to be at least partly driven by the increased availability of molecular gas reservoirs at the peak of cosmic star formation (z ˜ 2).

  11. ALMA OBSERVATIONS OF A HIGH-DENSITY CORE IN TAURUS: DYNAMICAL GAS INTERACTION AT THE POSSIBLE SITE OF A MULTIPLE STAR FORMATION

    Energy Technology Data Exchange (ETDEWEB)

    Tokuda, Kazuki; Onishi, Toshikazu [Department of Physical Science, Graduate School of Science, Osaka Prefecture University, 1-1 Gakuen-cho, Naka-ku, Sakai, Osaka 599-8531 (Japan); Saigo, Kazuya; Kawamura, Akiko [National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan); Fukui, Yasuo; Inutsuka, Shu-ichiro; Tachihara, Kengo [Department of Physics, Nagoya University, Chikusa-ku, Nagoya 464-8602 (Japan); Matsumoto, Tomoaki [Faculty of Humanity and Environment, Hosei University, Fujimi, Chiyoda-ku, Tokyo 102-8160 (Japan); Machida, Masahiro N. [Department of Earth and Planetary Sciences, Kyushu University, Fukuoka 812-8581 (Japan); Tomida, Kengo, E-mail: s_k.tokuda@p.s.osakafu-u.ac.jp [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)

    2014-07-01

    Starless dense cores eventually collapse dynamically, forming protostars inside them, and the physical properties of the cores determine the nature of the forming protostars. We report ALMA observations of dust continuum emission and molecular rotational lines toward MC27 or L1521F, which is considered to be very close to the first protostellar core phase. We found a few starless high-density cores, one of which has a very high density of ∼10{sup 7} cm{sup –3}, within a region of several hundred AU around a very low-luminosity protostar detected by Spitzer. A very compact bipolar outflow with a dynamical timescale of a few hundred years was found toward the protostar. The molecular line observation shows several cores with an arc-like structure, possibly due to the dynamical gas interaction. These complex structures revealed in the present observations suggest that the initial condition of star formation is highly dynamical in nature, which is considered to be a key factor in understanding fundamental issues of star formation such as the formation of multiple stars and the origin of the initial mass function of stars.

  12. Cuerpo y alma en el Carmelo descalzo femenino. Una aproximación a la alimentación conventual en la Cataluña moderna

    Directory of Open Access Journals (Sweden)

    M. Mercé GRAS I CASANOVAS

    2009-11-01

    Full Text Available RESUMEN: Cuerpo y alma en el Carmelo descalzo femenino. Unaaproximación a la alimentación conventual en la Cataluña moderna. A través del análisis de un conjunto de fuentes diversas: regla y cosntituciones, ceremoniales, cartas pastorales, hagiografías, epistolarios, polémicas internas, cuentas conventuales y libros de cocina, hemos pretendido reconstruir el marco teórico, la realidad material, el ritual y la contradictoria vivencia de la experencia alimentaria en un colectivo social específico.ABSTRACT: Body and soul in the feminine Discalced Carmel. An approach to the conventual alimentation in modern Catalonia. Through the analysis of an ensemble of sources of different kinds: Rule ans constitutions, ceremonials, pastoral letters, hagiographies, internal polemics, conventual account-books and kitchen's books, we have tried to recreate the theoretical archetype, the material reality, the ritual, and the contradictory experience of the alimentary life in a specific social collectivity.

  13. ALMA view of a massive spheroid progenitor: a compact rotating core of molecular gas in an AGN host at z = 2.226

    Science.gov (United States)

    Talia, M.; Pozzi, F.; Vallini, L.; Cimatti, A.; Cassata, P.; Fraternali, F.; Brusa, M.; Daddi, E.; Delvecchio, I.; Ibar, E.; Liuzzo, E.; Vignali, C.; Massardi, M.; Zamorani, G.; Gruppioni, C.; Renzini, A.; Mignoli, M.; Pozzetti, L.; Rodighiero, G.

    2018-05-01

    We present ALMA observations at 107.291 GHz (band 3) and 214.532 GHz (band 6) of GMASS 0953, a star-forming galaxy at z = 2.226 hosting an obscured active galactic nucleus (AGN) that has been proposed as a progenitor of compact quiescent galaxies (QGs). We measure for the first time the size of the dust and molecular gas emission of GMASS 0953 that we find to be extremely compact (˜1 kpc). This result, coupled with a very high interstellar medium (ISM) density (n ˜ 105.5 cm-3), a low gas mass fraction (˜0.2), and a short gas depletion time-scale (˜150 Myr), implies that GMASS 0953 is experiencing an episode of intense star formation in its central region that will rapidly exhaust its gas reservoirs, likely aided by AGN-induced feedback, confirming its fate as a compact QG. Kinematic analysis of the CO(6-5) line shows evidence of rapidly rotating gas (Vrot = 320^{+92}_{-53} km s-1), as observed also in a handful of similar sources at the same redshift. On-going quenching mechanisms could either destroy the rotation or leave it intact leading the galaxy to evolve into a rotating QG.

  14. VALES - IV. Exploring the transition of star formation efficiencies between normal and starburst galaxies using APEX/SEPIA Band-5 and ALMA at low redshift

    Science.gov (United States)

    Cheng, C.; Ibar, E.; Hughes, T. M.; Villanueva, V.; Leiton, R.; Orellana, G.; Muñoz Arancibia, A.; Lu, N.; Xu, C. K.; Willmer, C. N. A.; Huang, J.; Cao, T.; Yang, C.; Xue, Y. Q.; Torstensson, K.

    2018-03-01

    In this work, we present new the Swedish-ESO PI receiver for the Atacama Pathfinder Experiment APEX/SEPIA Band-5 observations targeting the CO (J = 2-1) emission line of 24 Herschel-detected galaxies at z = 0.1-0.2. Combining this sample with our recent new Valparaíso ALMA Line Emission Survey (VALES), we investigate the star formation efficiencies [SFEs = star formation rate (SFR)/M_H2] of galaxies at low redshift. We find the SFE of our sample bridges the gap between normal star-forming galaxies and Ultra-Luminous Infrared Galaxies (ULIRGs), which are thought to be triggered by different star formation modes. Considering the SFE΄ as the SFR and the L^' }_CO ratio, our data show a continuous and smooth increment as a function of infrared luminosity (or star formation rate) with a scatter about 0.5 dex, instead of a steep jump with a bimodal behaviour. This result is due to the use of a sample with a much larger range of sSFR/sSFRms using LIRGs, with luminosities covering the range between normal and ULIRGs. We conclude that the main parameters controlling the scatter of the SFE in star-forming galaxies are the systematic uncertainty of the αCO conversion factor, the gas fraction, and physical size.

  15. Resignificación de la muerte en los Andes: La festividad de Wiñay Pacha o todas las almas en Santiago de Chile

    Directory of Open Access Journals (Sweden)

    Francisca Fernández Droguett

    2014-12-01

    Full Text Available Desde el 2009 diversas organizaciones y agrupaciones de danza y música andina, han comenzado a conmemorar el día de difuntos en la ciudad de Santiago, denominándola Wiñay Pacha o Todas Almas. El siguiente artículo tiene por objetivo caracterizar esta práctica festiva desde los elementos culturales que configuran la visión de la muerte de los pueblos indígenas de Los Andes, a través de la vivencia del duelo y la forma de conmemorar a los difuntos, para luego reflexionar el modo en que se ha ido resignificando en el contexto urbano, mediante la revisión de su origen como festividad y su expresión como reivindicación de otros modos de vivenciar la muerte. La investigación se aborda desde una aproximación etnográfica, utilizando para la recopilación de datos la revisión bibliográfica, observación participante y entrevistas en profundidad.

  16. ALMA observations of the nearby AGB star L2 Puppis. II. Gas disk properties derived from 12CO and 13CO J = 3-2 emission

    Science.gov (United States)

    Homan, Ward; Richards, Anita; Decin, Leen; Kervella, Pierre; de Koter, Alex; McDonald, Iain; Ohnaka, Keiichi

    2017-05-01

    The circumstellar environment of the AGB star L2 Puppis was observed with ALMA in cycle 3, with a resolution of 15 × 18 mas. The molecular emission shows a differentially rotating disk, inclined to a nearly edge-on position. In the first paper in this series (Paper I) the molecular emission was analysed to accurately deduce the motion of the gas in the equatorial regions of the disk. In this work we model the optically thick 12CO J = 3-2 and the optically thin 13CO J = 3-2 rotational transition to constrain the physical conditions in the disk. To realise this effort we make use of the 3D NLTE radiative transfer code LIME. The temperature structure and velocity structure show a high degree of complexity, both radially and vertically. The radial H2 density profile in the disk plane is characterised by a power law with a slope of -3.1. We find a 12CO over 13CO abundance ratio of 10 inside the disk. Finally, estimations of the angular momentum in the disk surpass the expected available angular momentum of the star, strongly supporting the indirect detection of a compact binary companion reported in Paper I. We estimate the mass of the companion to be around 1 Jupiter mass.

  17. Interpreting major industrial landscapes: Social follow-up on meanings, the case of two aluminium smelters, Alcan (Alma, Canada) and Pechiney (Dunkirk, France)

    International Nuclear Information System (INIS)

    Fortin, Marie-Jose; Gagnon, Christiane

    2006-01-01

    Landscape is becoming an object of growing social concern and, as such, an object of mediation between major industrial producers and local communities. The question of the capacity of environmental assessment to address this issue is thus raised. Until now, landscape studies have focused on visual aspects, although subjective dimensions such as perceptions and meanings have been recognised. The research in this article concerns the subjective dimensions, and is presented with a view to further the understanding of the process of the social interpretation of landscape as it relates to heavy industrial sites. Within a socioconstructivist perspective, two case studies (a longitudinal follow-up and an ex-post) of two aluminum smelters, one in Alma (Quebec, Canada) and the other in Dunkirk (France) were conducted. The results show that nearby residents' interpretations of landscape varied according to three sets of factors related to 1) the dynamics of regional development and the historical place of industry in the community, 2) the relationship between residents and the industry and local governance capacities, and 3) the social impacts experienced. To conclude, three ways of using qualitative methodologies for social and environmental follow-up in a socioconstructivist approach to landscape are proposed

  18. The Effect of Oxygen Enrichment on Cardiorespiratory and Neuropsychological Responses in Workers With Chronic Intermittent Exposure to High Altitude (ALMA, 5,050 m

    Directory of Open Access Journals (Sweden)

    Fernando A. Moraga

    2018-03-01

    Full Text Available It is estimated that labor activity at high altitudes in Chile will increase from 60,000 to 120,000 workers by the year 2020. Oxygenation of spaces improves the quality of life for workers at high geographic altitudes (<5,000 m. The aim of this study was to determine the effect of a mobile oxygen module system on cardiorespiratory and neuropsychological performance in a population of workers from Atacama Large Millimeter/submillimeter Array (ALMA, 5,050 m radiotelescope in the Chajnantor Valley, Chile. We evaluated pulse oximetry, systolic and diastolic arterial pressure (SAP/DAP, and performed neuropsychological tests (Mini-Mental State examination, Rey-Osterrieth Complex Figure test at environmental oxygen conditions (5,050 m, and subsequently in a mobile oxygenation module that increases the fraction of oxygen in order to mimic the higher oxygen partial pressure of lower altitudes (2,900 m. The use of module oxygenation at an altitude of 5,050 m, simulating an altitude of 2,900 m, increased oxygen saturation from 84 ± 0.8 to 91 ± 0.8% (p < 0.00001, decreased heart rate from 90 ± 8 to 77 ± 12 bpm (p < 0.01 and DAP from 96 ± 3 to 87 ± 5 mmHg (p < 0.01. In addition, mental cognitive state of workers (Mini-Mental State Examination shown an increased from 19 to 31 points (p < 0.02. Furthermore, the Rey-Osterrieth Complex Figure test (memory shown a significant increase from 35 to 70 (p < 0.0001. The results demonstrate that the use of an oxygen module system at 5,050 m, simulating an altitude equivalent to 2,900 m, by increasing FiO2 at 28%, significantly improves cardiorespiratory response and enhances neuropsychological performance in workers exposed to an altitude of 5,050 m.

  19. Starburst to Quiescent from HST/ALMA: Stars and Dust Unveil Minor Mergers in Submillimeter Galaxies at z ∼ 4.5

    Science.gov (United States)

    Gómez-Guijarro, C.; Toft, S.; Karim, A.; Magnelli, B.; Magdis, G. E.; Jiménez-Andrade, E. F.; Capak, P. L.; Fraternali, F.; Fujimoto, S.; Riechers, D. A.; Schinnerer, E.; Smolčić, V.; Aravena, M.; Bertoldi, F.; Cortzen, I.; Hasinger, G.; Hu, E. M.; Jones, G. C.; Koekemoer, A. M.; Lee, N.; McCracken, H. J.; Michałowski, M. J.; Navarrete, F.; Pović, M.; Puglisi, A.; Romano-Díaz, E.; Sheth, K.; Silverman, J. D.; Staguhn, J.; Steinhardt, C. L.; Stockmann, M.; Tanaka, M.; Valentino, F.; van Kampen, E.; Zirm, A.

    2018-04-01

    Dust-enshrouded, starbursting, submillimeter galaxies (SMGs) at z ≥ 3 have been proposed as progenitors of z ≥ 2 compact quiescent galaxies (cQGs). To test this connection, we present a detailed spatially resolved study of the stars, dust, and stellar mass in a sample of six submillimeter-bright starburst galaxies at z ∼ 4.5. The stellar UV emission probed by HST is extended and irregular and shows evidence of multiple components. Informed by HST, we deblend Spitzer/IRAC data at rest-frame optical, finding that the systems are undergoing minor mergers with a typical stellar mass ratio of 1:6.5. The FIR dust continuum emission traced by ALMA locates the bulk of star formation in extremely compact regions (median r e = 0.70 ± 0.29 kpc), and it is in all cases associated with the most massive component of the mergers (median {log}({M}* /{M}ȯ )=10.49+/- 0.32). We compare spatially resolved UV slope (β) maps with the FIR dust continuum to study the infrared excess (IRX = L IR/L UV)–β relation. The SMGs display systematically higher IRX values than expected from the nominal trend, demonstrating that the FIR and UV emissions are spatially disconnected. Finally, we show that the SMGs fall on the mass–size plane at smaller stellar masses and sizes than the cQGs at z = 2. Taking into account the expected evolution in stellar mass and size between z = 4.5 and z = 2 due to the ongoing starburst and mergers with minor companions, this is in agreement with a direct evolutionary connection between the two populations.

  20. “CRIANÇA, A ALMA DO NEGÓCIO”: REFLEXÕES SOBRE PUBLICIDADE INFANTIL E ÉTICA EMPRESARIAL

    Directory of Open Access Journals (Sweden)

    Ivania Skura

    2015-08-01

    Full Text Available Em abril de 2014, a resolução nº 163 que define princípios aplicados à publicidade direcionada à criança, aprovada pelo CONANDA - Conselho Nacional dos Direitos da Criança e do Adolescente coloca em pauta o tema da publicidade infantil que vem ao encontro das discussões pautadas em princípios éticos e legais do CONAR - Conselho Nacional de Autorregulamentação Publicitária, CDC - Código de Defesa do Consumidor e ECA - Estatuto da Criança e do Adolescente. Esta discussão é ampliada para os modos práticos de regulamentar a ética empresarial nas comunicações direcionadas ao público-alvo infantil, como os movimentos consumeristas e as respostas sociais e reflexões em torno das consequências sociais desta prática. Utiliza-se como breve exemplo empírico a realidade retratada no documentário “Criança, a alma do negócio” e problematiza-se de que maneira o mercado publicitário se apresenta como ferramenta social que cria e dissemina modos de ser e viver e, no contexto do consumo infantil, deve atentar-se para a prática de anunciar com um controle eficaz que não prejudique o desenvolvimento e bem-estar das crianças.

  1. ALMA Observations of Gas-rich Galaxies in z ∼ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments

    Energy Technology Data Exchange (ETDEWEB)

    Noble, A. G.; McDonald, M. [Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States); Muzzin, A. [Department of Physics and Astronomy, York University, 4700 Keele Street, Toronto, ON MJ3 1P3 (Canada); Nantais, J. [Departamento de Ciencias Físicas, Universidad Andres Bello, Fernandez Concha 700, Las Condes 7591538, Santiago, Región Metropolitana (Chile); Rudnick, G. [The University of Kansas, Department of Physics and Astronomy, 1251 Wescoe Hall Drive, Lawrence, KS 66045 (United States); Van Kampen, E.; Manilla-Robles, A. [European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München (Germany); Webb, T. M. A.; Delahaye, A. [Department of Physics, McGill University, 3600 rue University, Montréal, QC H3A 2T8 (Canada); Wilson, G.; DeGroot, A.; Foltz, R. [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Yee, H. K. C. [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4 (Canada); Boone, K.; Hayden, B.; Perlmutter, S. [Department of Physics, University of California Berkeley, 366 LeConte Hall, MC 7300, Berkeley, CA 94720-7300 (United States); Cooper, M. C. [Department of Physics and Astronomy, University of California, Irvine, 4129 Frederick Reines Hall, Irvine, CA 92697 (United States); Demarco, R. [Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción, Región del Biobío (Chile); Lidman, C., E-mail: noble@mit.edu [Australian Astronomical Observatory, 105 Delhi Road, North Ryde, NSW 2113 (Australia)

    2017-06-20

    We present ALMA CO (2–1) detections in 11 gas-rich cluster galaxies at z ∼ 1.6, constituting the largest sample of molecular gas measurements in z > 1.5 clusters to date. The observations span three galaxy clusters, derived from the Spitzer Adaptation of the Red-sequence Cluster Survey. We augment the >5 σ detections of the CO (2–1) fluxes with multi-band photometry, yielding stellar masses and infrared-derived star formation rates, to place some of the first constraints on molecular gas properties in z ∼ 1.6 cluster environments. We measure sizable gas reservoirs of 0.5–2 × 10{sup 11} M {sub ☉} in these objects, with high gas fractions ( f {sub gas}) and long depletion timescales ( τ ), averaging 62% and 1.4 Gyr, respectively. We compare our cluster galaxies to the scaling relations of the coeval field, in the context of how gas fractions and depletion timescales vary with respect to the star-forming main sequence. We find that our cluster galaxies lie systematically off the field scaling relations at z = 1.6 toward enhanced gas fractions, at a level of ∼4 σ , but have consistent depletion timescales. Exploiting CO detections in lower-redshift clusters from the literature, we investigate the evolution of the gas fraction in cluster galaxies, finding it to mimic the strong rise with redshift in the field. We emphasize the utility of detecting abundant gas-rich galaxies in high-redshift clusters, deeming them as crucial laboratories for future statistical studies.

  2. ALMA and GMRT Constraints on the Off-axis Gamma-Ray Burst 170817A from the Binary Neutron Star Merger GW170817

    Science.gov (United States)

    Kim, S.; Schulze, S.; Resmi, L.; González-López, J.; Higgins, A. B.; Ishwara-Chandra, C. H.; Bauer, F. E.; de Gregorio-Monsalvo, I.; De Pasquale, M.; de Ugarte Postigo, A.; Kann, D. A.; Martín, S.; Oates, S. R.; Starling, R. L. C.; Tanvir, N. R.; Buchner, J.; Campana, S.; Cano, Z.; Covino, S.; Fruchter, A. S.; Fynbo, J. P. U.; Hartmann, D. H.; Hjorth, J.; Jakobsson, P.; Levan, A. J.; Malesani, D.; Michałowski, M. J.; Milvang-Jensen, B.; Misra, K.; O’Brien, P. T.; Sánchez-Ramírez, R.; Thöne, C. C.; Watson, D. J.; Wiersema, K.

    2017-12-01

    Binary neutron-star mergers (BNSMs) are among the most readily detectable gravitational-wave (GW) sources with the Laser Interferometer Gravitational-wave Observatory (LIGO). They are also thought to produce short γ-ray bursts (SGRBs) and kilonovae that are powered by r-process nuclei. Detecting these phenomena simultaneously would provide an unprecedented view of the physics during and after the merger of two compact objects. Such a Rosetta Stone event was detected by LIGO/Virgo on 2017 August 17 at a distance of ∼44 Mpc. We monitored the position of the BNSM with Atacama Large Millimeter/submillimeter Array (ALMA) at 338.5 GHz and the Giant Metrewave Radio Telescope (GMRT) at 1.4 GHz, from 1.4 to 44 days after the merger. Our observations rule out any afterglow more luminous than 3× {10}26 {erg} {{{s}}}-1 {{Hz}}-1 in these bands, probing >2–4 dex fainter than previous SGRB limits. We match these limits, in conjunction with public data announcing the appearance of X-ray and radio emission in the weeks after the GW event, to templates of off-axis afterglows. Our broadband modeling suggests that GW170817 was accompanied by an SGRB and that the γ-ray burst (GRB) jet, powered by {E}{AG,{iso}}∼ {10}50 erg, had a half-opening angle of ∼ 20^\\circ , and was misaligned by ∼ 41^\\circ from our line of sight. The data are also consistent with a more collimated jet: {E}{AG,{iso}}∼ {10}51 erg, {θ }1/2,{jet}∼ 5^\\circ ,{θ }{obs}∼ 17^\\circ . This is the most conclusive detection of an off-axis GRB afterglow and the first associated with a BNSM-GW event to date. We use the viewing angle estimates to infer the initial bulk Lorentz factor and true energy release of the burst.

  3. Tests of star formation metrics in the low-metallicity galaxy NGC 5253 using ALMA observations of H30α line emission

    Science.gov (United States)

    Bendo, G. J.; Miura, R. E.; Espada, D.; Nakanishi, K.; Beswick, R. J.; D'Cruze, M. J.; Dickinson, C.; Fuller, G. A.

    2017-11-01

    We use Atacama Large Millimeter/submillimeter Array (ALMA) observations of H30α (231.90 GHz) emission from the low-metallicity dwarf galaxy NGC 5253 to measure the star formation rate (SFR) within the galaxy and to test the reliability of SFRs derived from other commonly used metrics. The H30α emission, which originates mainly from the central starburst, yields a photoionizing photon production rate of (1.9 ± 0.3) × 1052 s-1 and an SFR of 0.087 ± 0.013 M⊙ yr-1 based on conversions that account for the low metallicity of the galaxy and for stellar rotation. Among the other star formation metrics we examined, the SFR calculated from the total infrared flux was statistically equivalent to the values from the H30α data. The SFR based on a previously published version of the H α flux that was extinction corrected using Paα and Paβ lines was lower than but also statistically similar to the H30α value. The mid-infrared (22 μm) flux density and the composite star formation tracer based on H α and mid-infrared emission give SFRs that were significantly higher because the dust emission appears unusually hot compared to typical spiral galaxies. Conversely, the 70 and 160 μm flux densities yielded SFRs lower than the H30α value, although the SFRs from the 70 μm and H30α data were within 1σ-2σ of each other. While further analysis on a broader range of galaxies is needed, these results are instructive of the best and worst methods to use when measuring SFR in low-metallicity dwarf galaxies like NGC 5253.

  4. An ALMA survey of submillimeter galaxies in the extended Chandra deep field south: The redshift distribution and evolution of submillimeter galaxies

    International Nuclear Information System (INIS)

    Simpson, J. M.; Swinbank, A. M.; Smail, Ian; Alexander, D. M.; Danielson, A. L. R.; Thomson, A. P.; Brandt, W. N.; Bertoldi, F.; Karim, A.; De Breuck, C.; Chapman, S. C.; Coppin, K. E. K.; Da Cunha, E.; Hodge, J. A.; Schinnerer, E.; Dannerbauer, H.; Greve, T. R.; Ivison, R. J.; Knudsen, K. K.; Poggianti, B. M.

    2014-01-01

    We present the first photometric redshift distribution for a large sample of 870 μm submillimeter galaxies (SMGs) with robust identifications based on observations with ALMA. In our analysis we consider 96 SMGs in the Extended Chandra Deep Field South, 77 of which have 4-19 band photometry. We model the SEDs for these 77 SMGs, deriving a median photometric redshift of z phot = 2.3 ± 0.1. The remaining 19 SMGs have insufficient photometry to derive photometric redshifts, but a stacking analysis of Herschel observations confirms they are not spurious. Assuming that these SMGs have an absolute H-band magnitude distribution comparable to that of a complete sample of z ∼ 1-2 SMGs, we demonstrate that they lie at slightly higher redshifts, raising the median redshift for SMGs to z phot = 2.5 ± 0.2. Critically we show that the proportion of galaxies undergoing an SMG-like phase at z ≥ 3 is at most 35% ± 5% of the total population. We derive a median stellar mass of M * = (8 ± 1) × 10 10 M ☉ , although there are systematic uncertainties of up to 5 × for individual sources. Assuming that the star formation activity in SMGs has a timescale of ∼100 Myr, we show that their descendants at z ∼ 0 would have a space density and M H distribution that are in good agreement with those of local ellipticals. In addition, the inferred mass-weighted ages of the local ellipticals broadly agree with the look-back times of the SMG events. Taken together, these results are consistent with a simple model that identifies SMGs as events that form most of the stars seen in the majority of luminous elliptical galaxies at the present day.

  5. ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CO LUMINOSITY FUNCTIONS AND THE EVOLUTION OF THE COSMIC DENSITY OF MOLECULAR GAS

    Energy Technology Data Exchange (ETDEWEB)

    Decarli, Roberto; Walter, Fabian [Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg (Germany); Aravena, Manuel; Assef, Roberto J. [Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército 441, Santiago (Chile); Carilli, Chris [National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, P.O. Box O, Socorro, NM 87801 (United States); Bouwens, Rychard [Leiden Observatory, Leiden University, P.O. Box 9513, NL2300 RA Leiden (Netherlands); Da Cunha, Elisabete [Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122 (Australia); Daddi, Emanuele [Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, Irfu/Service d’Astrophysique, CEA Saclay, Orme des Merisiers, F-91191 Gif-sur-Yvette cedex (France); Ivison, R. J.; Popping, Gergö [European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748, Garching (Germany); Riechers, Dominik [Cornell University, 220 Space Sciences Building, Ithaca, NY 14853 (United States); Smail, Ian R. [6 Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham DH1 3LE (United Kingdom); Swinbank, Mark [Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-053121 Bonn (Germany); Weiss, Axel; Anguita, Timo, E-mail: decarli@mpia.de [Departamento de Ciencias Físicas, Universidad Andres Bello, Fernandez Concha 700, Las Condes, Santiago (Chile); and others

    2016-12-10

    In this paper we use ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field in band 3 and band 6, to place blind constraints on the CO luminosity function and the evolution of the cosmic molecular gas density as a function of redshift up to z  ∼ 4.5. This study is based on galaxies that have been selected solely through their CO emission and not through any other property. In all of the redshift bins the ASPECS measurements reach the predicted “knee” of the CO luminosity function (around 5 × 10{sup 9} K km s{sup −1} pc{sup 2}). We find clear evidence of an evolution in the CO luminosity function with respect to z  ∼ 0, with more CO-luminous galaxies present at z  ∼ 2. The observed galaxies at z  ∼ 2 also appear more gas-rich than predicted by recent semi-analytical models. The comoving cosmic molecular gas density within galaxies as a function of redshift shows a drop by a factor of 3–10 from z  ∼ 2 to z  ∼ 0 (with significant error bars), and possibly a decline at z  > 3. This trend is similar to the observed evolution of the cosmic star formation rate density. The latter therefore appears to be at least partly driven by the increased availability of molecular gas reservoirs at the peak of cosmic star formation ( z  ∼ 2).

  6. First Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C II]-bright Gas and CO-bright Gas at Low Metallicity

    Science.gov (United States)

    Jameson, Katherine E.; Bolatto, Alberto D.; Wolfire, Mark; Warren, Steven R.; Herrera-Camus, Rodrigo; Croxall, Kevin; Pellegrini, Eric; Smith, John-David; Rubio, Monica; Indebetouw, Remy; Israel, Frank P.; Meixner, Margaret; Roman-Duval, Julia; van Loon, Jacco Th.; Muller, Erik; Verdugo, Celia; Zinnecker, Hans; Okada, Yoko

    2018-02-01

    The Small Magellanic Cloud (SMC) provides the only laboratory to study the structure of molecular gas at high resolution and low metallicity. We present results from the Herschel Spectroscopic Survey of the SMC (HS3), which mapped the key far-IR cooling lines [C II], [O I], [N II], and [O III] in five star-forming regions, and new ALMA 7 m array maps of {}12{CO} and {}13{CO} (2-1) with coverage overlapping four of the five HS3 regions. We detect [C II] and [O I] throughout all of the regions mapped. The data allow us to compare the structure of the molecular clouds and surrounding photodissociation regions using {}13{CO}, {}12{CO}, [C II], and [O I] emission at ≲ 10\\prime\\prime (value at high {A}V in the centers of the clouds and fall to ∼ 1/5{--}1/10× the Milky Way value in the outskirts, indicating the presence of translucent molecular gas not traced by bright {}12{CO} emission. We estimate the amount of molecular gas traced by bright [C II] emission at low {A}V and bright {}12{CO} emission at high {A}V. We find that most of the molecular gas is at low {A}V and traced by bright [C II] emission, but that faint {}12{CO} emission appears to extend to where we estimate that the {{{H}}}2-to-H I transition occurs. By converting our {{{H}}}2 gas estimates to a CO-to-{{{H}}}2 conversion factor (X CO), we show that X CO is primarily a function of {A}V, consistent with simulations and models of low-metallicity molecular clouds. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

  7. Preliminary report on arsenic and heavy metals contents in soils and stream bed sediments of Cornia, Bruna and Alma coastal plains (Southern Tuscany

    Directory of Open Access Journals (Sweden)

    Dughetti F.

    2013-04-01

    Full Text Available The Department of Earth Sciences of University of Florence has conducted over the past ten years, numerous studies about the distribution of arsenic and heavy metals in mineralized areas of Tuscany, particularly in the Pecora basin. The area hosts several polymetallic ore bodies and a pyrite ore deposit. The studies have identified several geochemical anomalies (As, Cu, Pb, Zn… both in the areas which host the ore bodies and in the coastal plain (Scarlino Plain. To increase the knowledge concerning the distribution of As and heavy metals in other Tuscan coastal plains, research is under way in the alluvial plains of the Bruna, Cornia and Alma rivers. The preliminary analysis have focused on soils and stream sediments, to better understand the correlations between the downstream transport of rivers and the soils. We have made physic-chemical analysis, particle size analysis, mineralogical analysis for X-ray powder diffraction, chemical analysis for the determination of major element (X-ray Fluorescence and for the determination of 35 minor elements and traces (AAS and ICP.Preliminary data show high concentrations of several elements (As, Zn, Co…. The concentrations of these elements in soils and stream bed sediments are not always consistent; in particular we have found higher concentrations in soils than in stream bed sediments in Cornia Plain, while the opposite happens in the Bruna basin. Therefore the natural processes of rocks weathering does not seem to have affected uniformly. The distribution of As and heavy metals in soils and stream bed sediments of the all three basins of interest are still under investigation.

  8. The ALMA-PILS survey: The sulphur connection between protostars and comets: IRAS 16293-2422 B and 67P/Churyumov-Gerasimenko

    Science.gov (United States)

    Drozdovskaya, Maria N.; van Dishoeck, Ewine F.; Jørgensen, Jes K.; Calmonte, Ursina; van der Wiel, Matthijs H. D.; Coutens, Audrey; Calcutt, Hannah; Müller, Holger S. P.; Bjerkeli, Per; Persson, Magnus V.; Wampfler, Susanne F.; Altwegg, Kathrin

    2018-02-01

    The evolutionary past of our Solar System can be pieced together by comparing analogous low-mass protostars with remnants of our Protosolar Nebula - comets. Sulphur-bearing molecules may be unique tracers of the joint evolution of the volatile and refractory components. ALMA Band 7 data from the large unbiased Protostellar Interferometric Line Survey (PILS) are used to search for S-bearing molecules in the outer disc-like structure, ˜60 au from IRAS 16293-2422 B, and are compared with data on 67P/C-G stemming from the ROSINA instrument aboard Rosetta. Species such as SO2, SO, OCS, CS, H2CS, H2S and CH3SH are detected via at least one of their isotopologues towards IRAS 16293-2422 B. The search reveals a first-time detection of OC33S towards this source and a tentative first-time detection of C36S towards a low-mass protostar. The data show that IRAS 16293-2422 B contains much more OCS than H2S in comparison to 67P/C-G; meanwhile, the SO/SO2 ratio is in close agreement between the two targets. IRAS 16293-2422 B has a CH3SH/H2CS ratio in range of that of our Solar System (differences by a factor of 0.7 - 5.3). It is suggested that the levels of UV radiation during the initial collapse of the systems may have varied and have potentially been higher for IRAS 16293-2422 B due to its binary nature; thereby, converting more H2S into OCS. It remains to be conclusively tested if this also promotes the formation of S-bearing complex organics. Elevated UV levels of IRAS 16293-2422 B and a warmer birth cloud of our Solar System may jointly explain the variations between the two low-mass systems.

  9. SDSS-IV MaNGA-resolved Star Formation and Molecular Gas Properties of Green Valley Galaxies: A First Look with ALMA and MaNGA

    Science.gov (United States)

    Lin, Lihwai; Belfiore, Francesco; Pan, Hsi-An; Bothwell, M. S.; Hsieh, Pei-Ying; Huang, Shan; Xiao, Ting; Sánchez, Sebastián F.; Hsieh, Bau-Ching; Masters, Karen; Ramya, S.; Lin, Jing-Hua; Hsu, Chin-Hao; Li, Cheng; Maiolino, Roberto; Bundy, Kevin; Bizyaev, Dmitry; Drory, Niv; Ibarra-Medel, Héctor; Lacerna, Ivan; Haines, Tim; Smethurst, Rebecca; Stark, David V.; Thomas, Daniel

    2017-12-01

    We study the role of cold gas in quenching star formation in the green valley by analyzing ALMA 12CO (1-0) observations of three galaxies with resolved optical spectroscopy from the MaNGA survey. We present resolution-matched maps of the star formation rate and molecular gas mass. These data are used to calculate the star formation efficiency (SFE) and gas fraction ({f}{gas}) for these galaxies separately in the central “bulge” regions and outer disks. We find that, for the two galaxies whose global specific star formation rate (sSFR) deviates most from the star formation main sequence, the gas fraction in the bulges is significantly lower than that in their disks, supporting an “inside-out” model of galaxy quenching. For the two galaxies where SFE can be reliably determined in the central regions, the bulges and disks share similar SFEs. This suggests that a decline in {f}{gas} is the main driver of lowered sSFR in bulges compared to disks in green valley galaxies. Within the disks, there exist common correlations between the sSFR and SFE and between sSFR and {f}{gas} on kiloparsec scales—the local SFE or {f}{gas} in the disks declines with local sSFR. Our results support a picture in which the sSFR in bulges is primarily controlled by {f}{gas}, whereas both SFE and {f}{gas} play a role in lowering the sSFR in disks. A larger sample is required to confirm if the trend established in this work is representative of the green valley as a whole.

  10. Pedreira das Almas de Jorge Andrade e Alberto D'Averso. Cinquenta anos de criação dramatúrgica e transposição cênica

    Directory of Open Access Journals (Sweden)

    Luiz Humberto Martins Arantes

    2009-01-01

    Full Text Available This article is a study on the transposition of the dramatic text to the staging. For that, it proposes to follow the ways that led both playwright Jorge Andrade to write Pedreira das Almas, a play from 1958, and director Alberto D’Aversa to make a homonymous spectacle, also in 1958. The research on the creation and transposition process of both of them will permit to understand how a play inspired by the city of São Tomé das Letras, Minas Gerais, has been taken and re-signified by the modern drama of São Paulo, which emerged as a novelty then.

  11. ALMA observations of the nearby AGB star L$_{\\rm 2}$ Puppis. II. Gas disk properties derived from $^{\\rm 12}$CO and $^{\\rm13}$CO $J=$3$-$2 emission

    OpenAIRE

    Homan, Ward; Richards, Anita; Decin, Leen; Kervella, Pierre; de Koter, Alex; McDonald, Iain; Ohnaka, Keiichi

    2018-01-01

    The circumstellar environment of the AGB star L$_{\\rm 2}$ Puppis was observed with ALMA in cycle 3, with a resolution of $15 \\times 18 \\rm\\ mas$. The molecular emission shows a differentially rotating disk, inclined to a nearly edge-on position. In the first paper in this series (paper I) the molecular emission was analysed to accurately deduce the motion of the gas in the equatorial regions of the disk. In this work we model the optically thick $^{\\rm 12}$CO $J=$3$-$2 and the optically thin ...

  12. A peregrinação da alma no Scivias de Hildegard de Bingen: criação, queda, redenção e salvação

    Directory of Open Access Journals (Sweden)

    Maria Carmen Gomes Martiniano de Oliveira

    2013-12-01

    Full Text Available Hildegard de Bingen, religiosa beneditina que viveu no século XII, alegava ter escrito sua primeira obra, o Scivias, obedecendo a um "comando divino" que ela teria recebido em uma de suas visões espirituais. Segundo Hildegard, essas visões a acompanhavam desde sua infância, e nelas ela recebia mensagens "divinas". O Scivias, escrito entre 1141 e 1151, consistia, de acordo com Hildegard, na transcrição dessas mensagens e era uma obra com ensinamentos em ortodoxia doutrinária. A obra, contendo as visões de Hildegard, é dividida em três partes de tamanho desigual que tratam respectivamente da criação e queda (primeira parte, da redenção e da salvação. Este artigo visa a analisar a quarta visão da primeira parte do Scivias em que Hildegard narra a peregrinação de uma alma pecadora. A caminhada dessa alma é interessante à medida que sintetiza, em sua jornada, as etapas doutrinárias cristãs trabalhadas em todo o Scivias, a saber, criação, queda, redenção e salvação.

  13. Marka Genişleme Stratejilerinin Üniversite Öğrencilerinin Satın Alma Niyetleri Üzerine Etkileri

    Directory of Open Access Journals (Sweden)

    Şükran KARACA

    2015-04-01

    Full Text Available Belirli bir marka imajı yaratmış olan firmaların yeni ürünlerini mevcut marka ismi ile pazarlaması ve bu şekilde mevcut markanın tüketici gözündeki değerini ve itibarını yeni ürünlere transfer etmek istemesi olan marka genişleme stratejisi, bugün birçok firmanın tercih ettiği bir uygulamadır. Bu çalışmada işletmelerin uyguladıkları marka genişleme stratejilerine yönelik tüketici tutumları ve bu tutumları etkileyen değişkenleri tespit etmek suretiyle marka genişleme stratejisinin tüketicilerin satın alma niyetleri üzerindeki etkilerini belirlemek amaçlanmıştır. Araştırma kapsamında Cumhuriyet Üniversitesi’nde öğrenim gören 445 öğrenciye yüz yüze anket uygulanmıştır. Sonuçlar SPSS 20.0 programında değerlendirilerek öğrencilerin verdiği cevapların frekans ve yüzdeleri alınmış, cevaplar t testi ve ANOVA analizi ile değerlendirilmiştir. Çalışmada öğrencilerin Adidas firmasının marka genişlemesine yönelik uygulamalarının hayali ürün kategorisi olan kot pantolon ürününe karşı olumlu tutum sergilediklerini, diğer hayali ürün kategorileri olan cep telefonu ve dizüstü bilgisayar açısından bazı faktörler dışında olumlu bir tutum sergilemedikleri ortaya çıkmıştır.

  14. Las Opiniones sacadas de los más auténticos y antigos philósofos que sobre la alma escrivieron i sus definiciones, de Daniel Arón Afia.

    Directory of Open Access Journals (Sweden)

    2008-06-01

    Full Text Available Included in a volume published in 1568 in Venice alongside the first Spanish translation of Leon Hebreo’s Diálogos de amor, the Opiniones sacadas de los más auténticos y antigos philósofos que sobre la alma escrivieron y sus difiniciones, were written by Aron Daniel Afia, an important Latin and Philosophy scholar in the Salonika of the second half of the 16th c. Descendant of a Converso family returned to Judaism after settlement in Ottoman lands, his short twelve folio work is a compendium of definitions of the soul proposed by thinkers from Antiquity to Renaissance, being a precious example of the intellectual activity (in Latin, Spanish and Hebrew of the Conversos who chose exile in the Levant. The volume, dedicated to Philip II, shows the attachment of former Conversos to Spanish culture.Las Opiniones sacadas de los más auténticos y antigos philósofos que sobre la alma escrivieron y sus definiciones fueron publicadas en 1568 en Venecia, junto con la primera traducción española de los Diálogos de amor de León Hebreo. Escritas por Daniel Arón Afia, profesor de latín y filosofía establecido en la Salónica de la segunda mitad del siglo XVI, este autor de familia conversa vuelta al judaísmo tras su establecimiento en tierras otomanas. El opúsculo de apenas doce folios es un compendio de definiciones del alma propuestas por pensadores, desde la Antigüedad hasta el Renacimiento, muestra de la actividad intelectual desarrollada en hebreo, latín y castellano de los conversos que escogieron la vía del exilio en el Levante mediterráneo. El volumen fue dedicado a Felipe II y muestra el apego de su promotor a la cultura hispánica.

  15. The ALMA Frontier Fields Survey. II. Multiwavelength Photometric analysis of 1.1 mm continuum sources in Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223

    Science.gov (United States)

    Laporte, N.; Bauer, F. E.; Troncoso-Iribarren, P.; Huang, X.; González-López, J.; Kim, S.; Anguita, T.; Aravena, M.; Barrientos, L. F.; Bouwens, R.; Bradley, L.; Brammer, G.; Carrasco, M.; Carvajal, R.; Coe, D.; Demarco, R.; Ellis, R. S.; Ford, H.; Francke, H.; Ibar, E.; Infante, L.; Kneissl, R.; Koekemoer, A. M.; Messias, H.; Muñoz Arancibia, A.; Nagar, N.; Padilla, N.; Pelló, R.; Postman, M.; Quénard, D.; Romero-Cañizales, C.; Treister, E.; Villard, E.; Zheng, W.; Zitrin, A.

    2017-08-01

    Context. The Hubble and Spitzer Space Telescope surveys of the Frontier Fields provide extremely deep images around six massive, strong-lensing clusters of galaxies. The ALMA Frontier Fields survey aims to cover the same fields at 1.1 mm, with maps reaching (unlensed) sensitivities of 5σ) sources in the first three Frontier Fields clusters observed by ALMA, based on data from Hubble and Spitzer, the Very Large Telescope and the Herschel Space Observatory. Methods: We measure the total photometry in all available bands and determine the photometric redshifts and the physical properties of the counterparts via SED-fitting. In particular, we carefully estimate the far-infrared (FIR) photometry using 1.1 mm priors to limit the misidentification of blended FIR counterparts, which strongly affect some flux estimates in previous FIR catalogs. Due to the extremely red nature of these objects, we used a large range of parameters (e.g. 0.0 ALMA surveys.

  16. Brown dwarf disks with ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Ricci, L.; Isella, A. [Department of Astronomy, California Institute of Technology, MC 249-17, Pasadena, CA 91125 (United States); Testi, L.; De Gregorio-Monsalvo, I. [European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching (Germany); Natta, A. [INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze (Italy); Scholz, A., E-mail: lricci@astro.caltech.edu [School of Cosmic Physics, Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2 (Ireland)

    2014-08-10

    We present Atacama Large Millimeter/submillimeter Array continuum and spectral line data at 0.89 mm and 3.2 mm for three disks surrounding young brown dwarfs and very low mass stars in the Taurus star forming region. Dust thermal emission is detected and spatially resolved for all the three disks, while CO(J = 3-2) emission is seen in two disks. We analyze the continuum visibilities and constrain the disks' physical structure in dust. The results of our analysis show that the disks are relatively large; the smallest one has an outer radius of about 70 AU. The inferred disk radii, radial profiles of the dust surface density, and disk to central object mass ratios lie within the ranges found for disks around more massive young stars. We derive from our observations the wavelength dependence of the millimeter dust opacity. In all the three disks, data are consistent with the presence of grains with at least millimeter sizes, as also found for disks around young stars, and confirm that the early stages of the solid growth toward planetesimals occur also around very low-mass objects. We discuss the implications of our findings on models of solids evolution in protoplanetary disks, the main mechanisms proposed for the formation of brown dwarfs and very low-mass stars, as well as the potential of finding rocky and giant planets around very low-mass objects.

  17. Morte e práticas fúnebres na secularizada República: a Irmandade e o Cemitério São Miguel e Almas de Porto Alegre na primeira metade do século XX

    OpenAIRE

    Dillmann, Mauro

    2013-01-01

    Nesta tese, abordamos as práticas fúnebres e cemiteriais que a Irmandade São Miguel e Almas, de Porto Alegre (RS), adotou em seu cemitério, inserindo-as no contexto de secularização dos campos santos e de projetos e ideias de modernização que a cidade vivenciou, sobretudo em termos urbanísticos, nas primeiras décadas do século XX. Identificamos e analisamos as mudanças introduzidas nas práticas fúnebres ao longo da primeira metade do século XX, bem como aspectos relativos ao gerenciamento do ...

  18. CARACTERIZAÇÃO E ANÁLISE DA FEIRA LIVRE DE CRUZ DAS ALMAS-BA SOB A ÓTICA DO PLANEJAMENTO E GESTÃO MUNICIPAL

    Directory of Open Access Journals (Sweden)

    Daciane Oliveira Silva

    2014-03-01

    Full Text Available As feiras livres são atividades econômicas que fazem parte da economia informal de uma parcela considerável das cidades, principalmente no nordeste brasileiro. São responsáveis por abrigar pessoas que não se enquadram nos padrões exigidos pela modernização tecnológica e são de abrangência local e regional. Este tipo de comércio se articula com outras modalidades de atividades econômicas rurais e urbanas e é gerido pelas prefeituras. No presente artigo, analisa-se a feira livre da cidade de Cruz das Almas, no Recôncavo baiano, sob a ótica da gestão e planejamento municipal; para tanto faz-se uma abordagem ancorada nas contribuições da teoria dos dois circuitos da economia urbana de Milton Santos. Em relação aos procedimentos metodológicos, optou-se por estudo exploratório de caráter qualitativo e quantitativo. A pesquisa revelou que a feira livre apresenta problemas, principalmente em relação à gestão dos espaços públicos. Como proposta, sugere-se a criação e reformulação de políticas públicas para o fortalecimento dessa atividade econômica. Para isso, devem-se empregar os resultados da pesquisa de campo, no que se refere às sugestões dos feirantes, e, em paralelo, promover a abertura de canais de participação com a Associação de Barraqueiros e Feirantes de Cruz das Almas (ABAFACA na elaboração dessas políticas.

  19. Entre Napoleón y Jesucristo: las peripecias del “alma rusa” en la obra de Dostoievski / Between Napoleon and Jesus Christ: The adventures of the "Russian soul" in Dostoevsky's work

    Directory of Open Access Journals (Sweden)

    Tatiana Bubnova

    2011-11-01

    Full Text Available RESUMEN: Dos componentes del “alma rusa” que se destacan en la obra de Dostoievski – el napoleonismo y la cristología — resultan de la interacción de la cultura rusa con la historia y la civilización occidental. Paradójicamente, la evolución de las dos líneas en las novelas del gran escritor ruso conduce a una determinada, en algunos aspectos, de los dos tipos, en particular, en El idiota. La revisión del manoseado tópico del “alma rusa” a la luz de las recientes investigaciones de los especialistas rusos pone de manifiesto nuevasintertextualidades y abre la obra a un diálogo renovado acerca de la identidad. El trabajo se inspira en la antropología filosófica y la filosofía del lenguaje de M. M. Bajtín. ABSTRACT: This is an analysis of the two components of the “Russian soul” highlighted in the Dostoevsky’s novels: Napoleonism and Christology. The origins of both of them can be found in the Western history and civilization. There is a certain paradox in the fact that the evolution of these two lines in the oeuvre of the great Russian writer arrives to an approachof the two types, the Napoleonic one and that of the follower of Christ, especially in The Idiot. A revision of the “Russian soul” under the light of the most recent interpretations of Russian critics discovers new intertexts and opens Dostoevsky’s text to a renewed identity dialogue. This paper is influenced by Bakhtin’s philosophical anthropology and philosophy of language.

  20. Health sector challenges and responses beyond the Alma-Ata Declaration: a Caribbean perspective Retos y respuestas del sector salud más allá de la declaración de Alma-Ata: una perspectiva Caribeña

    Directory of Open Access Journals (Sweden)

    Jasneth Mullings

    2007-03-01

    Full Text Available Al igual que el resto del mundo, el Caribe ha sido testigo del drástico paso de las enfermedades nutricionales y transmisibles a las enfermedades no transmisibles y crónicas. No obstante, en el Caribe este cambio ha coincidido con una nueva dinámica, creada por la emergencia de enfermedades transmisibles -como la infección por el VIH/sida- junto con los problemas relacionados con el envejecimiento, las enfermedades cardiovasculares, la violencia y las lesiones, entre otros. En este artículo se hace una revisión de la historia de la atención sanitaria en el Caribe, los retos y enfoques del sector salud y la nueva orientación en la atención primaria de salud (APS. Las observaciones se basan en trabajos publicados. En el Caribe, la Declaración de Alma-Ata sirvió como importante punto de giro y ofreció orientación, apoyo y dirección a medida que los países perfilaban sus servicios de salud para satisfacer sus necesidades. La creatividad y el ingenio surgieron como rasgos distintivos del enfoque caribeño en la reestructuración de la APS, ante los retos económicos, sociales, culturales, de recursos humanos y de políticas que enfrentaban. El fortalecimiento de de la capacidad institucional, la extensión de los programas sociales, los esquemas nacionales de seguros de salud, los programas específicos de promoción de salud y la ampliación de la investigación en apoyo al desarrollo de políticas continúan evidenciando el esfuerzo caribeño para responder a los cruciales retos epidemiológicos. A pesar de esos retos, se han establecido alianzas dentro y fuera del Caribe. Además, la Carta del Caribe para la Promoción de la Salud ha servido como elemento crítico para el desarrollo de la APS.

  1. ALMA imaging of gas and dust in a galaxy protocluster at redshift 5.3: [C II] emission in 'typical' galaxies and dusty starbursts ≈1 billion years after the big bang

    Energy Technology Data Exchange (ETDEWEB)

    Riechers, Dominik A. [Department of Astronomy, Cornell University, 220 Space Sciences Building, Ithaca, NY 14853 (United States); Carilli, Christopher L. [National Radio Astronomy Observatory, PO Box O, Socorro, NM 87801 (United States); Capak, Peter L.; Yan, Lin [Spitzer Science Center, California Institute of Technology, MC 220-6, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Scoville, Nicholas Z. [Astronomy Department, California Institute of Technology, MC 249-17, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Smolčić, Vernesa [University of Zagreb, Physics Department, Bijenička cesta 32, 10002 Zagreb (Croatia); Schinnerer, Eva [Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg (Germany); Yun, Min [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Cox, Pierre [ALMA Santiago Central Office, Alonso de Cordova 3107, Vitacura, Santiago (Chile); Bertoldi, Frank; Karim, Alexander, E-mail: dr@astro.cornell.edu [Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, Bonn, D-53121 (Germany)

    2014-12-01

    We report interferometric imaging of [C II]({sup 2} P {sub 3/2}→{sup 2} P {sub 1/2}) and OH({sup 2}Π{sub 1/2} J = 3/2→1/2) emission toward the center of the galaxy protocluster associated with the z = 5.3 submillimeter galaxy (SMG) AzTEC-3, using the Atacama Large (sub)Millimeter Array (ALMA). We detect strong [C II], OH, and rest-frame 157.7 μm continuum emission toward the SMG. The [C II]({sup 2} P {sub 3/2}→{sup 2} P {sub 1/2}) emission is distributed over a scale of 3.9 kpc, implying a dynamical mass of 9.7 × 10{sup 10} M {sub ☉}, and a star formation rate (SFR) surface density of Σ{sub SFR} = 530 M {sub ☉} yr{sup –1} kpc{sup –2}. This suggests that AzTEC-3 forms stars at Σ{sub SFR} approaching the Eddington limit for radiation pressure supported disks. We find that the OH emission is slightly blueshifted relative to the [C II] line, which may indicate a molecular outflow associated with the peak phase of the starburst. We also detect and dynamically resolve [C II]({sup 2} P {sub 3/2}→{sup 2} P {sub 1/2}) emission over a scale of 7.5 kpc toward a triplet of Lyman-break galaxies with moderate UV-based SFRs in the protocluster at ∼95 kpc projected distance from the SMG. These galaxies are not detected in the continuum, suggesting far-infrared SFRs of <18-54 M {sub ☉} yr{sup –1}, consistent with a UV-based estimate of 22 M {sub ☉} yr{sup –1}. The spectral energy distribution of these galaxies is inconsistent with nearby spiral and starburst galaxies, but resembles those of dwarf galaxies. This is consistent with expectations for young starbursts without significant older stellar populations. This suggests that these galaxies are significantly metal-enriched, but not heavily dust-obscured, 'normal' star-forming galaxies at z > 5, showing that ALMA can detect the interstellar medium in 'typical' galaxies in the very early universe.

  2. İNTERNET KULLANICILARININ İNTERNETTEN ALIŞ-VERİŞE YÖNELİK SATIN ALMA KARAR SÜREÇLERİNİN İNCELENMESİ ve KULLANIM YOĞUNLUKLARI AÇISINDAN SINIFILANDIRILMASI ÜZERİNE BİR ARAŞTIRMA-INVESTIGATING INTERNET USERS DECISION MAKING PROCESSES REGARDING THEIR INTERNET

    Directory of Open Access Journals (Sweden)

    Emrah CENGİZ

    2012-06-01

    Full Text Available Tüketici satın alma karar süreci uzun yıllardır işletmelerin ve akademisyenlerin ilgi odaklarından birisidir. Tüketicilerin hangi faktörlerin etkisi altında ve hangi aşamalardan geçerek satın alma kararını verdikleri çeşitli modellerle açıklanmaya çalışılmış, karar sürecine hangi aşamalarda ne şekilde etki edilebileceği araştırma konusu olmuştur. Son zamanların önemle üzerinde durulan pazarlama fenomenlerinden biri de internet ve internet üzerinden satın alma eğilimleridir. İnternet üzerinden satın alma davranışı da aynı şekilde gerek işletmelerin gerekse akademisyenlerin önemle üzerinde durup inceledikleri bir konudur. Bu çalışmada tüketicilerin internet kullanma yoğunluğu temelinde, “internetten alış-verişe yönelik satın alma karar süreçleri”, “internette gerçekleştirdikleri faaliyetler” ve “demografik özellikler” açısından fark olup olmadığını incelenmiştir. Ayrıca, interneti yoğun veya az kullanmakla birlikte, internetten alış-veriş yapan tüketicilerin ayırt edici özellikleri belirlenmiştir.-Consumer buying process is one of the center of attention both businesses and academics for many years. Which factors influence the consumer decision making and buying stages have trying to explain by various models and which factors affecting the decision process have been investigated by many researcher. Internet and purchasing via internet are one of the very important marketing phenomenons of last decades. Purchasing via internet is also a hot topic among the business and academics. In this study consumers use the Internet on the basis of intensity, “internet shopping for the purchase decision process”, “internet activities performed”, and “demographic characteristics” in term of whether the differences were examined. In addition consumer’s distinctive characteristics have been identified in order to internet usage frequencies.

  3. Türkçe Öğretmeni Adaylarının Dinlerken Not Alma Stilleri / Turkish Language Teacher Candidates’ Note-Taking Styles while Listening

    OpenAIRE

    Gürkan TABAK; Adnan KARADÜZ

    2016-01-01

    Bu araştırma, Türkçe öğretmeni adaylarının dinlerken not alma stillerinin tespit edilmesi amacıyla gerçekleştirilmiştir. Bu araştırmada temel nitel çalışma deseni uygulanarak gerçekleştirilmiştir. Araştırmanın katılımcılarını, 2013–2014 eğitim-öğretim yılı güz döneminde Erciyes Üniversitesi Eğitim Fakültesi Türkçe öğretmenliği bölümü üçüncü sınıfa devam eden 22 Türkçe öğretmeni adayı oluşturmuştur. Katılımcıların belirlenmesinde kolay ulaşılabilir durum ve maksimum çeşitlilik örneklemelerinde...

  4. A interação naturante entre o demiurgo e o mundo, a questão dos "dois tipos de matéria" e a natureza da "implantação" da alma no corpo

    Directory of Open Access Journals (Sweden)

    Edrisi Fernandes

    2010-12-01

    Full Text Available Em seu Comentário ao Timeu, Proclo diz que em algumas ocasiões Platão fala de um modelo (a partir do qual o mundo é criado que é idêntico ao Demiurgo, enquanto noutras ocasiões sugere que o modelo é distinto do Demiurgo. Aqui, identidade e diferença remetem à semelhança ou dessemelhança com o inteligível, identificado com a eternidade (estabilidade; fixidez. Ora, Platão também fala no Timeu que o Cosmos é bonito e seu Construtor (o Demiurgo é bom porquanto fixou a vista no modelo eterno. Se perguntarmos o que é engendrado quando o Demiurgo fixa a vista num modelo que não lhe é idêntico, encontramos a resposta no Timeu: inveja, defeitos, desordem, limitação quanto à inteligência e à alma, incompletude, feiúra e imperfeição. Plotino, por sua vez, menciona (Enéadas, II.4, a existência de dois tipos de matéria, inteligível e sensível. A matéria inteligível ou divina equivale à "Díade indefinida", identificada com a processão do Noûs. Para Plotino, apesar de a matéria inteligível ser eterna e imutável sua archê é constituída por diferença e movimento - condições que preparam a naturação da matéria sensível. Para Proclo, a Alma, desdobramento do Noûs, faz a mediação entre o Intelecto, a matéria inteligível e a matéria sensível. Diversos intérpretes parecem ter entendido a matéria inteligível como matéria da Alma, e para explicar a interação entre o inteligível e o sensível muitas teorias surgiram a respeito da constituição da matéria inteligível e sobre a natureza do "veículo" ou "veículos" que estariam associados à "descida" e encarnação da Alma.In his Commentary on the Timaeus Proclus says that in some occasions Plato speaks of a model (from which the world is created that is identical to the Demiurge while in other occasions he suggests that the model is distinct from the Demiurge. Here, identity and difference refer to the similarity with or dissimilarity from the

  5. Espelho da alma: teoria social e subjetivação em um conto de Machado de Assis Mirror of the soul: subjectivity and social theory in a short history by Machado de Assis

    Directory of Open Access Journals (Sweden)

    César Sabino

    2011-01-01

    Full Text Available O objetivo deste trabalho é delinear de forma breve as interseções teóricas existentes no conto "O espelho. Um esboço de uma nova teoria da alma humana", de Machado de Assis, e parte da tradição da teoria social que sugere uma síntese sociológica entre ação e estrutura relacionada ao aspecto da construção da identidade e subjetivação, reprodução e mudança social.This paper aims to present a brief outline of the theoretical intersections in the short history "The looking glass. Rough draft of a new theory of the human soul", by Machado de Assis. It departs from the tradiction of social theory that suggests a sociological syntheses between action and strutcture that is closely linked to the issue of one's construction of identity and subjectivaction, their reproduction and social transformation.

  6. Driving and control strategies in alternative current machines of permanent magnet with non-sinusoidal flux; Estrategias de acionamento e controle em maquinas CA de ima permanente com fluxo nao senoidal

    Energy Technology Data Exchange (ETDEWEB)

    Monteiro, Jose Roberto Boffino de Almeida

    1997-07-01

    The aim of this work is to study and analyze the torque performance of brush less machines with non-sinusoidal distributed magnetic fluxes. The machine type considered is a surface mount permanent magnet brush less machine. Three mathematical models for the machine are considered: the per stator phase, the vectorial and the linear second order speed-voltage models. Machines with different stator windings are compared including the permanent magnet synchronous machines with sinusoidal distributed stator windings. The torque outputs of these machines are obtained considering two kinds of open loop driving systems: one with a six-pulse waveform and other with a sinusoidal waveform. Finally, a vectorial control is proposed for the non-sinusoidal machines. The torque ripple as well the overall performance of non-sinusoidal machines with vectorial control is compared to that of sinusoidal machines. (author)

  7. Análise experimental do comportamento de vigas mistas de concreto e alvenaria estrutural sujeitas à flexão simples

    OpenAIRE

    Ramos, Angélica Paiva [UNESP

    2012-01-01

    O presente trabalho apresenta uma análise experimental de vigas de alvenaria submetidas à flexão simples. Como definição do projeto foram executadas 8 (oito) vigas denominadas mistas, sendo compostas por blocos estruturais de concreto e uma camada superior de graute. Baseado nos domínios de deformação do concreto armado dividiu-se, para uma melhor análise 4 (quatro) grupos compostos de 2 vigas cada, onde se diferenciaram pela taxa de armadura longitudinal, definidas como A1, A2, A3 e A4, empr...

  8. Modelo de estoque para peças de reposição sujeitas à demanda intermitente e lead time estocástico

    OpenAIRE

    Gerson Luis Caetano da Silva

    2009-01-01

    O controle de estoque de peças de reposição é muito crítico para a maioria das empresas devido ao alto custo de estoque associado a estes itens e à complexidade em desenvolver modelos de estoque para controlá-los. A grande maioria destes itens é slow-moving com demanda irregular e intermitente o que torna difícil a tarefa de prever a demanda futura. Foi desenvolvida uma metodologia para classificar e controlar peças de reposição considerando demanda e lead time estocásticos. Foi utilizada uma...

  9. DUYGUSALLIK VE BİLİŞSELLİĞİN PLANSIZ SATIN ALMA DAVRANIŞINA ETKİSİ-THE INFLUENCE OF AFFECT AND COGNITION ON IMPULSE BUYING BEHAVIOR

    Directory of Open Access Journals (Sweden)

    Caner DİNCER

    2012-06-01

    Full Text Available Bu çalışmanın amacı, yazını zenginleştirmek ve yönetimsel kullanım için yeni bakış açıları sağlamak üzere, tüketicilerin kendilerini algılayışlarını göz önüne alarak plansız satın alma davranışı eğilimlerini incelemektir. Çalışmanın araştırma tasarımı, diğer çalışmalarda kullanılan ölçekleri Türk tüketicisine uyarlayan, toplamda 284 üniversite öğrencisi üzerinde gerçekleştirilmiş bir anket çalışmasından meydana gelmektedir. Duygusal ve bilişsel eğilim ölçekleri yüksek iç tutarlılık, güvenilirlik göstermiş ve analizlerde kullanılmışlardır. Bulgular, plansız satın alma davranışının tamamen duygusal olduğunu ve demografik özelliklerle bir ilişkisi olmadığını göstermiştir. Bu sonuçlar, firmalar için duygusal alışveriş ortamı yaratmanın ve pazarlama kampanyalarında duygusal unsurların kullanımının önemini vurgularken, araştırmacılar için de bu duygusal unsurların saptanmasının önemini vurgular.-The purpose of the study is to investigate the impulse buying tendency of the consumers while taking into consideration their self-perception in order to enrich the literature and provide new points of view for managerial use. The design of the study consists of a questionnaire administered to a total of 284 university students, adapting existing scales to Turkish context. The scales of affective and cognitive tendency showed high internal reliability and are used in the analysis. The findings revealed that impulse buying is purely affective and does not have any significant correlation with the used demographic variables. These results emphasize the importance of emotional shopping environment and the use of affective components in marketing campaigns for firms as well as the determination of these affective components for the researchers.

  10. O INTIMISMO NO HISTÓRICO A PARTIR DE LEITURA DAS OBRAS: A PROLE DO CORVO, DE LUIZ ANTONIO DE ASSIS BRASIL E NETTO PERDE SUA ALMA, DE TABAJARA RUAS

    Directory of Open Access Journals (Sweden)

    Cibele Hechel Colares da Costa (FURG

    2015-03-01

    Full Text Available O presente trabalho busca demonstrar, através da leitura dos romances A prole do corvo, de Luiz Antonio de Assis Brasil e Netto perde sua alma, de Tabajara Ruas, de que forma essas duas obras, que são comumente citadas na historiografia literária como romances de caráter histórico apenas, também apresentam características que as aproximam do intimismo. Nesse sentido, para pensá-las enquanto romances históricos, utiliza-se os autores Maria Teresa de Freitas (1986, Seymour Menton (1993 e Rogério Puga (2006; enquanto que para refletir sobre os aspectos que as compõem, enquanto textos intimista, utiliza-se os teóricos: Hans Meyerhoff (1976, Robert Humphrey (1976 e Normam Friedman (2002. Além dos autores de cunho teórico, alguns nomes da historiografia da literatura foram observados no presente estudo, tais como: Regina Zilberman (1982, Luis Augusto Fischer (2004, Luis Marobim (1985; 1995, Massaud Moises (1993 e Alfredo Bosi (1994, os quais auxiliam na compreensão de como os romancistas em questão são vistos pela historiografia. Ao final do estudo, espera-se conseguir demonstrar, através das reflexões e comparações desenvolvidas, como Assis Brasil e Ruas destacam-se dentro da literatura por conta de seu hibridismo temático, visto que suas obras, em análise nesse momento, permitem uma leitura inovadora, pois suas escritas demonstram uma perspectiva intimista relacionada a elementos da historiografia do estado do Rio Grande do Sul.PALAVRAS-CHAVE: Luiz Antonio de Assis Brasil. Tabajara Ruas. Intimismo. Romance histórico. Literatura sul-rio-grandense. Abstract This paper stresses, by reading the novels A prole do corvo, by Luiz Antonio de Assis Brasil and Netto perde sua alma, by Tabajara Ruas, how these two works, which are commonly mentioned in literary history as historic character novels only, also have characteristics that approach the intimacy. In this sense to imagine them as historical novels we use the authors Maria

  11. Instagram’dan Alışveriş Yapan Tüketicilerin Satın Alma Davranışları: Keşifsel Bir Çalışma

    Directory of Open Access Journals (Sweden)

    Eda YAŞA ÖZELTÜRKAY

    2017-07-01

    Full Text Available Teknolojinin gelişmesi, tüketicilerin satın alma davranışlarında değişikliklerin yaşanmasına nedenolmuştur. Tüketiciler, diğer geleneksel mecraların yanı sıra, internet ve sosyal medya gibi mecralardanda alışveriş yapmaya başlamışlardır. Bu yeni mecralardan birisi de Instagram’dır. Instagram, birçok tüketiciiçin yeni bir mecra olmasına rağmen, Instagram’dan alışveriş yapan tüketicilerin sayısı gün geçtikçeartmaktadır. Bu nedenle, bu araştırmanın amacı, Instagram’dan alışveriş yapan tüketicilerin profillerinive satın alma davranışlarını ortaya çıkartmaktır. Araştırmada, nitel araştırma yöntemlerindenbiri olan derinlemesine görüşme yöntemi kullanılmıştır. Adana’da oturan 22 katılımcı ile derinlemesinegörüşmeler yapılmıştır. Bu katılımcılara, kartopu örneklem yöntemi vasıtasıyla ulaşılmıştır. Araştırmasonuçlarına göre, Instagram’dan alışveriş yapan tüketicilerin büyük çoğunluğu kadındır. Katılımcılarınyarısı 2 yıldır Instagram hesabına sahiptir ve gün içerisinde 10-15 defa Instagram hesabınabakmaktadırlar. Katılımcıların hepsi öncelikle, işletme ve işletmenin ürünleri hakkında bilgi sahibi olmakiçin hesapları takip etmekte ve genellikle Instagram’dan kıyafet, ayakkabı, takı ve saat almaktadırlar.Katılımcılar sırasıyla kapıda ödeme kolaylığı, ürün çeşitliliği, fiyatının uygun olması gibi özelliklerindendolayı Instagram’dan alışveriş yapmayı tercih etmektedirler. Katılımcıların yaklaşık yarısıürünün altında fiyatının yazmasını istemektedir.

  12. A statistical study of giant molecular clouds traced by 13CO, C18O, CS, and CH3OH in the disk of NGC 1068 based on ALMA observations

    Science.gov (United States)

    Tosaki, Tomoka; Kohno, Kotaro; Harada, Nanase; Tanaka, Kunihiko; Egusa, Fumi; Izumi, Takuma; Takano, Shuro; Nakajima, Taku; Taniguchi, Akio; Tamura, Yoichi

    2017-04-01

    We present 1{^''.}4 (98 pc) resolution ALMA observations of 13CO(J = 1-0), C18O(J = 1-0), CS(J = 2-1), and CH3OH(JK = 2K-1K) molecular rotational lines in the central 1΄ (4.2 kpc) diameter region of NGC 1068 to study the physical and chemical properties of giant molecular clouds (GMCs) and to test whether these GMC-scale properties are linked to the larger-scale galactic environment. Using the derived 13CO cube, we have identified 187 high-significance (>8 σ) GMCs by employing the CLUMPFIND algorithm. The molecular gas masses of GMCs (M_^{13CO}), derived from the 13CO data, range from 1.8 × 104 M⊙ to 4.2 × 107 M⊙. A mass function of GMCs in NGC 1068 has been obtained for the first time at ∼100 pc resolution. We find the slope of the mass function γ = -1.25 ± 0.07 for a mass range of M_^{13CO} ≥ 105 M⊙. This is shallower than the GMCs in the disk regions of the Milky Way, M 51, and NGC 300. Further, we find that the high mass cut-off of the GMC mass function occurs at M_^{13CO} ˜ 6 × 107 M⊙, which is an order of magnitude larger than that in the nuclear bar region of M 51, indicating that the more massive clouds dominate the mass budget in NGC 1068. The observed C18O(J = 1-0)/13CO(J = 1-0) intensity ratios are found to be fairly uniform (0.27 ± 0.05) among the identified GMCs. In contrast, the CH3OH(JK = 2K-1K)/13CO(J = 1-0) ratios exhibit striking spatial variation across the disk, with the smallest values around the bar-end (<0.03), and larger ratios along the spiral arms (∼0.1-0.2). We find that GMCs with detectable methanol emission tend to have systematically larger velocity widths than those without methanol emission, suggesting that (relatively weak) shocks are responsible for the enhancement of the CH3OH/13CO ratios of GMCs in the disk of NGC 1068.

  13. ALMA HCN AND HCO{sup +} J  = 3 − 2 OBSERVATIONS OF OPTICAL SEYFERT AND LUMINOUS INFRARED GALAXIES: CONFIRMATION OF ELEVATED HCN-TO-HCO{sup +} FLUX RATIOS IN AGNS

    Energy Technology Data Exchange (ETDEWEB)

    Imanishi, Masatoshi; Nakanishi, Kouichiro [National Astronomical Observatory of Japan, National Institutes of Natural Sciences (NINS), 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Izumi, Takuma, E-mail: masa.imanishi@nao.ac.jp [Institute of Astronomy, School of Science, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan)

    2016-12-01

    We present the results of our ALMA observations of three active galactic nucleus (AGN)-dominated nuclei in optical Seyfert 1 galaxies (NGC 7469, I Zw 1, and IC 4329 A) and eleven luminous infrared galaxies (LIRGs) with various levels of infrared estimated energetic contributions by AGNs at the HCN and HCO{sup +} J  = 3 − 2 emission lines. The HCN and HCO{sup +} J  = 3 − 2 emission lines are clearly detected at the main nuclei of all sources, except for IC 4329 A. The vibrationally excited ( v {sub 2} = 1f) HCN J  = 3 − 2 and HCO{sup +} J  = 3 − 2 emission lines are simultaneously covered, and HCN v {sub 2} = 1f J  = 3 − 2 emission line signatures are seen in the main nuclei of two LIRGs, IRAS 12112+0305 and IRAS 22491–1808, neither of which shows clear buried AGN signatures in the infrared. If the vibrational excitation is dominated by infrared radiative pumping, through the absorption of infrared 14 μ m photons, primarily originating from AGN-heated hot dust emission, then these two LIRGs may contain infrared-elusive, but (sub)millimeter-detectable, extremely deeply buried AGNs. These vibrationally excited emission lines are not detected in the three AGN-dominated optical Seyfert 1 nuclei. However, the observed HCN v {sub 2} = 1f to v  = 0 flux ratios in these optical Seyferts are still consistent with the intrinsic flux ratios in LIRGs with detectable HCN v {sub 2} = 1f emission lines. The observed HCN-to-HCO{sup +} J  = 3 − 2 flux ratios tend to be higher in galactic nuclei with luminous AGN signatures compared with starburst-dominated regions, as previously seen at J  = 1 − 0 and J  = 4 − 3.

  14. Thirty years after Alma-Ata: a systematic review of the impact of community health workers delivering curative interventions against malaria, pneumonia and diarrhoea on child mortality and morbidity in sub-Saharan Africa

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    Lewin Simon

    2011-10-01

    Full Text Available Abstract Background Over thirty years have passed since the Alma-Ata Declaration on primary health care in 1978. Many governments in the first decade following the declaration responded by developing national programmes of community health workers (CHWs, but evaluations of these often demonstrated poor outcomes. As many CHW programmes have responded to the HIV/AIDS pandemic, international interest in them has returned and their role in the response to other diseases should be examined carefully so that lessons can be applied to their new roles. Over half of the deaths in African children under five years of age are due to malaria, diarrhoea and pneumonia - a situation which could be addressed through the use of cheap and effective interventions delivered by CHWs. However, to date there is very little evidence from randomised controlled trials of the impacts of CHW programmes on child mortality in Africa. Evidence from non-randomised controlled studies has not previously been reviewed systematically. Methods We searched databases of published and unpublished studies for RCTs and non-randomised studies evaluating CHW programmes delivering curative treatments, with or without preventive components, for malaria, diarrhoea or pneumonia, in children in sub-Saharan Africa from 1987 to 2007. The impact of these programmes on morbidity or mortality in children under six years of age was reviewed. A descriptive analysis of interventional and contextual factors associated with these impacts was attempted. Results The review identified seven studies evaluating CHWs, delivering a range of interventions. Limited descriptive data on programmes, contexts or process outcomes for these CHW programmes were available. CHWs in national programmes achieved large mortality reductions of 63% and 36% respectively, when insecticide-treated nets and anti-malarial chemoprophylaxis were delivered, in addition to curative interventions. Conclusions CHW programmes could

  15. Faculdades da alma e suas implicações para a educação: saberes divulgados no século XIX Faculties of the soul and their implications for education: knowledges circulated in the 19th century

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    Raquel Martins de Assis

    2012-03-01

    Full Text Available Este artigo descreve resultados de uma pesquisa que buscou investigar como o tema das faculdades da alma e de suas implicações no desenvolvimento humano e na educação da pessoa foi divulgado, ao final do século XIX, pela imprensa periódica. Esperando contribuir para a história da psicologia e da educação, o artigo apresenta a análise de escritos sobre educação moral e educação estética de uma Secção Scientífica ou Pedagógica assinada por José Miguel de Siqueira e publicada no jornal O Baependyano (1877-1889. Inicialmente, são feitas breves descrições do periódico e de sua posição na conjuntura da época, bem como do lugar em que foi publicado. Em seguida, tratamos da definição de pedagogia apresentada pelo jornal, levando em consideração as apropriações de autores estrangeiros comumente presentes no campo da educação. A pedagogia considerada moderna é definida em tais escritos como a expansão e o desenvolvimento das forças animais, racionais e morais do ser humano; sua finalidade seria a formação do homem social pronto para o trabalho e para o serviço da sociedade e do Estado. Partindo dessa discussão, abordamos as concepções de educação espontânea, educação regular e instrução contidas no periódico. A educação é entendida como a unidade entre cultura e instrução, sendo a cultura a principal responsável pelo direcionamento das faculdades da alma e pela formação moral; a instrução, por sua vez, é tomada como aquisição de conhecimentos, mas também desempenha um papel importante na formação de hábitos e costumes.The article describes the results of a research that investigated how the theme of the faculties of the soul and of their implications for human development and for the education of a person was made available in the late 19th century by the circulating press. In an attempt to contribute to the history of psychology and education, the article presents the analysis of

  16. Lisanslı Spor Ürünlerinin Algılanan Değer Bileşenlerinin Satın Alma Niyeti ile İlişkisi: Türkiye’nin En Büyük Üç Futbol Kulübünün İncelenmesi

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    İpek KAZANÇOĞLU

    2016-03-01

    Full Text Available Lisanslı ürünler futbol kulüplerine hem düzenli bir gelir kaynağı, hem de taraftarlarıyla olan duygusal bağlarını geliştirme imkânı sunmaktadır. Araştırmanın amacı; taraftarların takımla özdeşleşme düzeyleri ve lisanslı ürünlerin algılanan değeri arasındaki ilişkileri incelemek, bu faktörlerin satın alma niyeti üzerindeki etkilerini araştırmaktır. Türkiye’nin üç büyük futbol kulübünün taraftarlarından toplam 953 kişiyle anket çalışması gerçekleştirilmiştir. Araştırma sonuçlarına göre, taraftarların takımla özdeşleşme düzeyi ile lisanslı ürünleri satın alma niyeti arasında doğrudan ilişkinin olmadığı, algılanan değerin etkisi aracılığıyla takımla özdeşleşmenin satın alma niyetine etkisi olduğu belirlenmiştir. Kulüpler temelindeki farklılıkların görülmesi için yapılan analizler, her kulüp için lisanslı ürünlerin öne çıkan algılanan değer boyutlarının farklılaştığını göstermektedir.

  17. MIKROPROPAGASI ANGGREK ALMA Grammatophyllum scriptum Blume

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    Elizabeth Handini

    2008-01-01

    Full Text Available Grammatophyllum scriptum is a beautiful wild orchid that has an interesting economic value. However, the existence of this ornamental plant species is at risk because of irresponsible exploitation of the natural population and insufficient cultivation efforts. Currently, the Bogor Botanic Garden is developing a program of orchid propagation for enhancing the conservation of all potential orchid collections. The propagation of G. scriptum was basically carried out by culturing the seeds in a modified Hyponex or Vacin & Went medium, transplanting the plantlets into a more suitable medium and finally acclimatizing the resulting seedlings. A study was done to observe the effect of fertilizer application on the growth of acclimatized G. scriptum seedlings, as a means to improve the propagation technique of the species. The result showed that the application of 1 and 2 m1/I organic fertilizer (Sugih as well as 1 and 2 g/I inorganic fertilizer (Hyponex increased the seedling mortality, in which the application of 2 g/ml Hyponex fertilizer was being the most damaging treatment, leaving 12,5 % seedlings to survive. However, in terms of seedling growth, the application of 1 m1/I Sugih fertilizer was slightly beneficial to the formation of root and the elongation of stem of the acclimatized seedlings. It may be suggested, therefore, that G. scriptum seedlings require no (or very little amount of supplementary fertilizer to boost their vegetative growth.

  18. Con el alma en el cuerpo

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    Claudio Bardelli

    2015-01-01

    Full Text Available La moda "modelo" arrasa y arrastra legiones de entusiastas jóvenes ¿Se trata de la versión de los años 90 de la mujer-objeto? ¿o de una nueva femineidad globalizada por los medios?

  19. Educando el alma psicológica

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    Matthew Curtis

    2007-01-01

    Full Text Available Este trabajo retoma aspectos de una exploración de los trabajos de cuatro importantes psicólogos educativos estadounidenses –Granville Stanley Hall, William James, John Dewey y Edward Thorndike– para concentrarse en los principios rectores del desarrollo de los niños. Los trabajos de estos autores están considerados como funciones que psicologizan al niño como un proceso de llegar a ser humano, que deba ser educado con fines éticos e inteligentes. Dos puntos de partida históricos se abordan en este artículo: (1 explorar la psicología como una formación de la moral del niño y (2 la clasificación y el orden del ser de forma razonada a partir de una psicología que abre el interior del niño a la supervisión y al calculo. Este enfoque explora la psicología educativa como una maquinaria de prácticas discusivas, intelectuales y materiales que invitan al estudiante a ver /ser visto y formar/ser formado de formas particulares. Educar al yo autónomo requería métodos modernos

  20. TERMAL TURİZMDE TÜKETİCİ SATIN ALMA DAVRANIŞINI ETKİLEYEN FAKTÖRLERİN BELİRLENMESİ: GÖNEN ÖRNEĞİ - DETERMINATION OF THE FACTORS AFFECTING CONSUMER PURCHASE BEHAVIOR IN THERMAL TOURISM

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    Mehmet İLBAN

    2012-11-01

    Full Text Available Özet:Günümüzde turistik bölgeler arasında yaşanan yoğunrekabet, tüketicilerin satın alma davranışlarını etkileyebilmeyi,buna bağlı olarak benzersiz bir ürün yaratmayı ve ürününfarklılığını ortaya koyabilmeyi son derece önemli halegetirmiştir. Bu durum turistik bölgenin turist sayısı ve eldeedeceği gelir düzeyini de yakından ilgilendirmektedir.Dolayısıyla, tüketiciler açısından turistik bölge tercihinde satınalma davranışını etkileyen faktörlerin öncelikle nelerolduğunun tespiti ve tüketicilerin belirli özelliklerine görehedef pazarların belirlenmesi bu çabaları yerine getirmedemuhakkak ki oldukça önemli katkılar sağlayacaktır. Bunoktadan hareketle, demografik özelliklerine göre termalturizme yönelik tüketicilerin satın alma davranışlarınıetkileyen faktörlerin belirlenmesi amacıyla bir anket çalışmasıuygulanmıştır. Anketlerden elde edilen verilerden hareketle,turistik tüketicilerin satın alma davranışlarını etkileyenfaktörlerin öncelik sırasına göre şu şekilde sıralanmıştır;pazarlama çabaları, ekonomik faktörler, sosyal faktörler,psikolojik faktörler ve kişisel ve kültürel faktörler. Ayrıcaaraştırmada, turistik tüketicilerin demografik özelliklerinegöre satın alma davranışlarını etkileyen faktörleri algılamalarıarasında anlamlı farklılıklar bulunmuştur.Abstract:Today, fierce competition among the tourist areasmade affecting buying behavior of the consumers andcorrespondingly creating a unique product and putting forththe difference of the product extremely important. This case isa particular concern to tourist number of the tourist area andthe income level. Hence, firstly, from the perspective of touriststo choose a tourist place, determination of the factors affectingthe buying behaviors of the consumers and specifying thetarget markets according to the certain features of theconsumers, will make a significant contribution

  1. Kredi Kartının Plansız Satın Alma Davranışına Etkisi: Karabük Üniversitesi Akademik Personeline Yönelik Bir Uygulama / The effect of Credit Card on Impulse Purchase: An application for the Academic staff of Karabuk University

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    Selçuk Yurtsever

    2012-12-01

    Full Text Available Kredi kartı kullanımının giderek yaygınlaşması, satın alma eylemlerinde ödeme kolaylığı sağlayarak hayatı kolaylaştırmasının yanı sıra tüketimi ve ihtiyaç fazlası satın almayı artırarak tüketicilerin gereksiz ürünlere sahip olmalarına ve kredi kartı borçlarını ödemede zorluk çekmelerine neden olmaktadır. Bu araştırma kredi kartının kontrolsüz bir tüketici davranışı olan plansız satın alma davranışlarına etkisini incelemektedir. Araştırma kapsamında Türkiye’de sosyo-ekonomik sınıf olarak en üst sınıfın bir altı olan B sosyo-ekonomik sınıf içerisinde yer alan akademisyenlerin kredi kartı kullanımları ele alınmaktadır. Bu bağlamda Karabük Üniversitesi akademik personeline anket uygulaması yapılmıştır. Anket sonucu ulaşılan verilere, Yüzde Analizi, Mertebeli Dereceleme ve Tek Faktörlü Çoklu Varyans Analizi (MANOVA uygulanmaktadır. Araştırma sonuçlarına göre araştırmaya katılan akademisyenlerin kredi kartını kontrollü ve bilinçli kullandıkları ve kredi kartı kullanımlarının plansız satın alma davranışına neden olmadığı ifade edilebilir. The effect of Credit Card on Impulse Purchase: An application for the Academic staff of Karabuk University Along with providing facility in payment, the widening use of credit cards also increases consumption and causes consumers to buy non-essential products and experience difficulties in paying their credit card debts by increasing surplus purchases. This research focuses on the effects of credit cards on impulse purchase, which is an uncontrolled consumer behavior. Within the scope of the research, the use of credit cards by academicians in the socio-economic class B which comes next after the top level socio-economic class in Turkey is assessed. In this context, a survey is carried out with the academic staff of Karabuk University. The data acquired as the result of the survey is evaluated with

  2. Investigation of Maths Oriented Academic Risk-Taking Behaviours of Secondary School Students by Some Variables [Ortaokul Öğrencilerinin Matematik Odaklı Akademik Risk Alma Davranışlarının Bazı Değişkenlere Göre İncelenmesi

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    Esat Avcı

    2016-08-01

    Full Text Available In this study, secondary school students' academic risk-taking behaviours have been investigated to understand whether they vary according to some variables or not. These variables are: Gender, grade level, town, type of school, parents education level, economic status of the family, the previous year's maths scores. Survey method was used in the study. The population is students who are studying in secondary schools located in Akdeniz, Mezitli, Toroslar and Yenişehir provinces of Mersin, in the 2014 - 2015 academic year. The research sample is 1054 students who are studying at 14 of these schools. “Mathematics-oriented academic risk taking behaviors scale” was used for data collection. Data for the analysis of independent samples t-test and ANOVA were used. There is no significant variance between maths-oriented academic risk-taking behaviours of students based on variables such as gender, town, school type and economic status of the family whereas there is meaningful variance based on variables such as grade level, level of parents education and last year's mathematics score. [Bu araştırmada ortaokul öğrencilerinin akademik risk alma davranışlarının bazı değişkenlere göre farklılık gösterip göstermediği araştırılmıştır. Bu değişkenler şunlardır: Cinsiyet, sınıf düzeyi, ilçe, okul türü, anne ve baba eğitim düzeyi, ailelerin ekonomik durumu, bir önceki seneki matematik puanları. Çalışmada tarama yöntemi kullanılmıştır. Araştırma evreni, 2014 – 2015 eğitim öğretim yılında Mersin ili Akdeniz, Mezitli, Toroslar ve Yenişehir ilçelerinde bulunan ortaokullarda okumakta olan öğrencilerdir. Araştırma örneklemi ise bu okullardan 14 tanesinde okumakta olan 1054 öğrencidir. Veri toplama aracı olarak “Matematik Odaklı Akademik Risk Alma Ölçeği” kullanılmıştır. Verilerin analizi için bağımsız örneklem t testi ve ANOVA uygulanmıştır. Öğrencilerin matematik odakl

  3. El cuidado del alma y otros cuidados en las cartas de aniversario del cabildo de los clérigos de Cuéllar en el siglo XIV = The Care of the Soul and Other Concerns in Obit Endowment Charters of the Chapter of Clerics of Cuéllar in the Fourteenth Century

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    Mauricio Herrero Jiménez

    2016-06-01

    Full Text Available El trabajo que presentamos tiene como objeto fundamental el estudio de las cartas de aniversario. Aplicando el método de la ciencia diplomática, nos proponemos mostrar cómo las cartas de aniversario del cabildo de los clérigos de Cuéllar muestran lo concerniente a la preocupación por el alma después de la muerte, al valor de la oración y lo que fue donado para pagarlas, con  cuyas donaciones el capítulo incremento su patrimonio, sobre todo en el siglo XIV.The present paper aims to offer an study of anniversary documents. Using the method of the diplomatic science, we propose showing how the anniversary documents of the chapter of clerics of Cuéllar teach us to concern about the soul after death, the value of prayer, and what was donated to pay them, with whose donations the chapter increased its heritage specially in the XIV century.

  4. Alma e destino do povo português: o fado como identidade nacional lusa no limiar do estado novo (1927–1933 = Portuguese people’s soul and destiny: the fado as lusitanian national identity on the threshold of the estado novo (1927–1933

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    Gasparotto, Lucas André

    2014-01-01

    Full Text Available O fado, gênero musical considerado canção nacional em Portugal, apresenta trajetória histórica cuja origem remonta ao início da segunda metade do século XIX. Desde pelo menos o último terço dos oitocentos, observa-se, nas primeiras obras dedicadas à história do fado, o aparecimento de um debate acerca do status de símbolo nacional atribuído ao gênero. É, contudo, no final dos anos 1920 e início dos 1930 que se observa uma série de elementos responsáveis por atribuir carga simbólica e identitária ao fado, capaz de consolidá-lo como identidade nacional portuguesa. Através de conjunto de fontes que contempla legislação, obras literárias e jornalísticas e jornais de temática específica, este trabalho analisa as características do cenário musical fadista em Portugal durante o período de 1927 a 1933, destacando um processo de ritualização das práticas artísticas que objetivava dignificar o gênero mediante às diversas camadas da sociedade. A pesquisa sustenta-se na discussão em torno dos conceitos de nação e identidade nacional, a fim de definir o fado como alma e destino do povo português, enquanto canção popular com status de canção nacional capaz de credenciá-lo como uma cultura comum

  5. A educação do corpo para o "soldado integral", "forte de físico, culto de cérebro e grande de alma" The education of the body for an "integral soldier", "physically strong, intelligent and soul superior"

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    Renata Duarte Simões

    2012-06-01

    Full Text Available Este estudo reflete sobre o treinamento paramilitar realizado pela Milícia Integralista, unidade armada da Ação Integralista Brasileira (AIB, principal partido de extrema direita no Brasil da década de 1930, no sentido de formar o "soldado integral", "forte de físico, culto de cérebro e grande de alma". Analisa os números do jornal Monitor Integralista, periódico doutrinário e prescritivo do movimento, encontrado no Arquivo Público e Histórico do Município de Rio Claro, SP, e o jornal A Offensiva, que se encontra microfilmado na Biblioteca Nacional no Rio de Janeiro. Concluiu que o objetivo de Plínio Salgado, Chefe Nacional da AIB, era treinar verbalmente, por meio de discursos, de propaganda boca a boca e pelo voto, ou corporalmente, pela luta armada e corporal, os integralistas para torná-los aptos a defender as causas do movimento.This study examines the paramilitary training carried out by the Integralist Militia (Milícia Integralista, unit of the Brazilian Integralist Action (Ação Integralista Brasileira, AIB of the extreme right wing political party in Brazil in the 1930s. The training was aimed to create the "integral soldier", a "physically strong, intelligent and soul superior" one. The study analyzes issues of the newspaper "Monitor Integralista", a prescriptive and dogmatic journal of the movement, found in the Public and History Archives of the city of Rio Claro, State of São Paulo, and in the "A Offensiva" newspaper, microfilmed an archived at the National Library of Rio de Janeiro. It concludes that Plínio Salgado's goal, the National Head of the AIB, was to train, by using verbal persuasion, speeches, word of mouth and by vote, by force and physical combat, the integralists to defend the causes of the movement.

  6. Methodology to relieve tensions in buried pipelines in areas of slow land moviment; Metodologia para alivio de tensoes em dutos enterrados em areas sujeitas a movimentacao lenta do solo

    Energy Technology Data Exchange (ETDEWEB)

    Paula, Angelo J.; Stanger, Daniel; Soares, Jose P.; Novaes, Jose L.; Bonini, Luis H.; Moya, Marcelo; Sacramento, Waldemar; Ribeiro, Walter M. [TRANSPETRO - PETROBRAS Transporte, Rio de Janeiro, RJ (Brazil)

    2005-07-01

    This paper shows the methodology developed by TRANSPETRO Team of Geotecnia and used to relieve the MERLUZA pipeline tensions. After the problem is detect by usual Systematic Geotechnical Inspections and confirmed by direct and indirect measures, which identify deformations (curve model) caused by strength of land movement, this methodology is apply in this section. In this intervention the standard procedures consist on the following steps: test 'in situ' on the surface of pipeline iron; installation of instruments to measure the relief of tensions; controlled excavation of the ditch; installation of permanent instruments to measure the future new deformations and tensions; and the recomposition of the place with compact land. (author)

  7. Tipos polínicos encontrados em colônias de abelhas africanizadas sujeitas à doença cria ensacada brasileira Pollen types found in africanized honeybees colonies submitted to brazilian sac brood disease

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    Marta Rodrigues Pacheco

    2009-10-01

    Full Text Available O pólen de algumas espécies de Stryphnodendron (Mimosoidea, conhecidas popularmente por barbatimão, tem sido apontado como agente causador da mortandade de larvas pré-pupas observada na cria ensacada brasileira (CEB. Neste estudo, objetivou-se identificar os tipos polínicos encontrados em amostras de pólen coletadas em colméias de Apis mellifera L., no Estado do Rio de Janeiro, a fim de elucidar as fontes florais utilizadas por essa espécie de abelhas em períodos sujeitos a CEB, com especial atenção para a presença do pólen de Stryphnodendron spp. Foram coletadas amostras de pólen apícola e pão de abelhas em sete apiários, em três municípios do Estado do Rio de Janeiro. A amostragem foi tomada um mês antes e durante a ocorrência da CEB. As famílias botânicas mais representativas foram: Leguminosae, Euphorbiaceae, Asteraceae, Poaceae e Myrtaceae. O pólen de Stryphnodendron não esteve presente nas amostras analisadas. A ausência de Stryphnodendron no menu floral das colônias africanizadas acometidas pela CEB em condições naturais sugere outro fator causal para a CEB no Estado do Rio de Janeiro.The pollen of some Stryphnodendron species (Mimosoidea, commonly known as barbatimão, has been identified as a causative agent of pre-pulps larvae mortality, observed in Brazilian sac brood disease (BSB. The goal of this study is to identify the pollen types found in samples of pollen collected by Apis mellifera L. to elucidate the floral diet used by this honeybee specie in Rio de Janeiro state during the periods where BSB usually occurs. Particular attention was given to the pollen of Stryphnodendron spp presence. Samples of pollen and bee bread were collected from seven apiaries located in Rio de Janeiro state, Brazil. Sampling procedures were done a month before BSB usual occurrence and also during its occurrence. Leguminosae, Euphorbiaceae, Asteraceae, Poaceae and Myrtaceae were most representative botanical families on pollen sampling. Pollen from Stryphnodendron was not presented at the analyzed samples. In order to Stryphnodendron absent at the floral diet of Africanized hives affected by BSB in natural conditions, it is proposed another causal factor for BSB in the state of Rio de Janeiro.

  8. Clásicos colombianos: Historia de una alma

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    Carlos Arturo Caparroso

    1960-12-01

    Full Text Available El doctor José María Samper (1828-1888 fue uno de nuestros más fecundos y múltiples escritores de la pasada centuria. Hombre de intensa y dramática acción política, y literato en el sentido más amplio de la palabra, representa algo así como un símbolo muy cabal de lo que fueron nuestros antepasados ilustres de la segunda generación de la República, la mayor parte de los cuales solían manejar, alternativamente, la espada del guerrero, la pluma del letrado y el verbo encendido ele la elocuencia tribunicia.

  9. Envidia, carcoma del alma: escorzo psico-literario

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    TERESA SÁNCHEZ SÁNCHEZ

    2004-01-01

    Full Text Available Desde Aristóteles hasta Castilla del Pino, desde Covarrubias hasta María Zambrano, desde el clasicismo grecolatino a la modernidad de los Simposiums de Psicología y Psicoanálisis, el tema de la envidia ha sido objeto de análisis. Tan sutiles matices provienen de la filosofía como de la psicología, de la literatura como de la clínica. La envidia es sometida a la mirada benevolente que exige su rango de emoción universal humana, derivada de la alteridad, la comparación y la autovaloración negativa, así como de la deficiente instalación narcisística y el anhelo de suplantación del otro idealizado. La envidia es antesala del odio y de un cortejo de expresiones interpersonales y sociales muy variadas y sibilinas. Anida, incluso, tras el choque de civilizaciones generador de los más atroces y destructivos episodios de fanatismo terrorista recientemente padecidos en nuestro mundo.

  10. Sigüenza y el alma del paisaje

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    Juan Navarro de San Pío

    2017-09-01

    Full Text Available Este artículo propone un análisis de la estética del paisaje en la obra del escritor Gabriel Miró. Para ello se investiga el significado y valor atribuido al paisaje en la trilogía novelesca  (Del vivir, Libro de Sigüenza, Años y Leguas de Sigüenza, héroe modernista de su paisaje literario, así como en el ensayo Sigüenza y el mirador azul. La visión del paisaje en Miró se reconstruye a través del diálogo con diferentes fuentes culturales y filosóficas (especialmente, Giner de los Ríos y Ortega y Gasset. El paisaje mironiano muestra así la evolución desde una inicial actitud panteísta hacia una posterior mirada fenomenológica y hermenéutica.

  11. El alma de un género

    Directory of Open Access Journals (Sweden)

    Juan Paulhiac

    2014-12-01

    Full Text Available Fiesta de picó. Champeta, espacio y cuerpo en Cartagena, Colombia. María A. Sanz Giraldo. Universidad del Rosario, Escuela de Ciencias Humanas, colección Ópera Prima, Bogotá, 2012, 286 págs.

  12. Tulemuslik juhtimine ebatavaliselt keerulistes haridusoludes / Andy Hargreaves, Alma Harris

    Index Scriptorium Estoniae

    Hargreaves, Andy

    2015-01-01

    Haridusjuhtimise tulemustest Eestis ja Inglismaal. Artiklis otsitakse vastust küsimusele, kuidas saada häid tulemusi koolides, mis tegutsevad keerulistes kogukondlikes või demograafilistes tingimustes

  13. Alma mater NYC : võimenda, kiirenda, kuhja / Mariliis Lilover

    Index Scriptorium Estoniae

    Lilover, Mariliis

    2014-01-01

    Mariliis Liloveri arhitektuurialastest õpingutest New Yorgis (Graduate School of Architecture, Planning and Preservation at Columbia University) ja tema arvamusest, et koolide ülesandeks on koolitada selline arhitekt, kelle eesmärk peaks olema ületada nii iseennast kui ka tellija unistusi, kavandades midagi, mida klient algul ei osanud soovida, kuid usub lõpuks, et just sellisest tulemusest ta unistaski

  14. Alma mater sõnas, pildis ja helis / Varje Sootak

    Index Scriptorium Estoniae

    Sootak, Varje, 1946-

    2007-01-01

    Tartu Ülikooli 375. aastapäeva puhul esitleti ülikooli kohvikus albumit "Universitas Tartuensis 375" ja samanimelise dokumentaalfilmi DVD-d. Viimase stsenaristideks on Jaak Lõhmus ja Lauri Vahtre, režissöörideks Rene Vilbre ja Märten Vaher

  15. La batalla global por el alma del capitalismo

    Directory of Open Access Journals (Sweden)

    Luis Esteban G. Manrique

    2012-07-01

    Full Text Available El gigante informático norteamericano Apple vale hoy en bolsa unos 350.000 millones de dólares, 20.000 millones más que la segunda compañía del país, ExxonMobil, y también más que los 32 mayores bancos de la zona euro juntos. Sin embargo, Apple apenas tiene 47.000 empleados en todo el mundo, 30.000 de los cuales trabajan en EE.UU., pero ninguno de ellos en plantas de ensamblaje. Todos sus famosos productos -los iMac, iPod, iPad, iPhone- son fabricados en China por la contratista taiwanesa Foxconn, para la que trabajan casi un millón de personas, 250.000 de ellas dedicadas en exclusiva a los artilugios electrónicos de la compañía de la manzana.

  16. The Marriage of Alma Mater to Adam Smith.

    Science.gov (United States)

    Buescher, John B.

    1987-01-01

    Businesses and universities must be encouraged to act from their traditional positions of strength, based on the longest view and the broadest interests. They must examine carefully their potential sources of conflict as well as opportunities for benefit before engaging in alliances that may become complex and difficult to manage. (MSE)

  17. Molecular data and radiative transfer tools for ALMA

    NARCIS (Netherlands)

    Tak, F F S van der; ; Hogerheijde, M

    2007-01-01

    Abstract: This paper presents an overview of several modeling tools for analyzing molecular line observations at submillimeter wavelengths. These tools are already proving to be very valuable for the interpretation of data from current telescopes, and will be indispensable for data obtained with

  18. Controller area network for monitor and control in ALMA

    Science.gov (United States)

    Brooks, Michael J.

    2000-06-01

    The Controller Area Network (CAN), initially developed for the automotive industry, is becoming increasingly popular in industrial process control applications. The need for distributed low data rate monitor and control networking in industry is similar to the needs of the various instrumentation and support equipment in a modern radio telescope. In particular, immunity to noise and low radio frequency emission characteristics are common to both domains. The Atacama Large Millimeter Array project has adopted CAN technology for use in local monitor and control applications at each of its 64 antennas. A standard interface slave node providing flexible I/O options is under development and a simple application-level protocol making use of CAN to access these nodes in a master/slave fashion has been implemented. This paper will present the work which has been completed to date including experiences in the use of CAN in an astronomical environment. In addition, analysis and simulation of CAN networks is compared with the performance of our implementation in the lab.

  19. TRANSITION DISK CHEMISTRY AND FUTURE PROSPECTS WITH ALMA

    International Nuclear Information System (INIS)

    Cleeves, L. Ilsedore; Bergin, Edwin A.; Bethell, Thomas J.; Calvet, Nuria; Fogel, Jeffrey K. J.; Sauter, Jürgen; Wolf, Sebastian

    2011-01-01

    We explore the chemical structure of a disk that contains a large central gap of R ∼ 45 AU, as is commonly seen in transitional disk systems. In our chemical model of a disk with a cleared inner void, the midplane becomes revealed to the central star so that it is directly irradiated. The midplane material at the truncation radius is permissive to reprocessed optical heating radiation, but opaque to the photodissociating ultraviolet, creating an environment abundant in gas-phase molecules. Thus the disk midplane, which would otherwise for a full disk be dominated by near complete heavy element freeze-out, should become observable in molecular emission. If this prediction is correct this has exciting prospects for observations with the Atacama Large Millimeter/Submillimeter Array, as the inner transition region should thus be readily detected and resolved, especially using high-J rotational transitions excited in the high density midplane gas. Therefore, such observations will potentially provide us with a direct probe of the physics and chemistry at this actively evolving interface.

  20. Envidia, carcoma del alma: escorzo psico-literario

    OpenAIRE

    TERESA SÁNCHEZ SÁNCHEZ

    2004-01-01

    Desde Aristóteles hasta Castilla del Pino, desde Covarrubias hasta María Zambrano, desde el clasicismo grecolatino a la modernidad de los Simposiums de Psicología y Psicoanálisis, el tema de la envidia ha sido objeto de análisis. Tan sutiles matices provienen de la filosofía como de la psicología, de la literatura como de la clínica. La envidia es sometida a la mirada benevolente que exige su rango de emoción universal humana, derivada de la alteridad, la comparación y la autovaloración negat...

  1. The 2014 ALMA Long Baseline Campaign: An Overview

    Czech Academy of Sciences Publication Activity Database

    Fomalont, E.B.; Vlahakis, C.; Corder, S.; Remijan, A.; Barkats, D.; Lucas, R.; Hunter, T.R.; Brogan, C.L.; Asaki, Y.; Matsushita, S.; Dent, W.R.F.; Hills, R.E.; Phillips, N.; Richards, A.M.S.; Cox, P.; Amestica, R.; Broguiere, D.; Cotton, W.; Hales, A.S.; Hiriart, R.; Hirota, A.; Hodge, J.A.; Impellizzeri, C.M.V.; Kern, J.; Kneissl, R.; Liuzzo, E.; Marcelino, N.; Marson, R.; Mignano, A.; Nakanishi, K.; Nikolic, B.; Perez, J.E.; Perez, L.M.; Toledo, I.; Bárta, Miroslav; Jáchym, Pavel; Karlický, Marian; Kraus, Michaela; Kunneriath, Devaky

    2015-01-01

    Roč. 808, č. 1 (2015), L1/1-L1/11 ISSN 2041-8205 Institutional support: RVO:67985815 Keywords : interferometers * submillimeter * high angular resolution Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 5.487, year: 2015

  2. Structure and Dynamics of an AGN torus: 3D hydrodynamical simulations for ALMA : 3D hydrodynamical simulations for ALMA

    NARCIS (Netherlands)

    Perez-Beaupuits, J. P.; Wada, K.; Spaans, Maarten; Gusten, R.

    A 3D hydrodynamical model of an AGN torus (Wada, Papadopoulos & Spaans, 2009), which follows the formation of H2 out of the neutral hydrogen phase according to the evolving ambient ISM conditions (at a resolution of 0.25 pc), is used to estimate the abundance of different atomic and molecular

  3. Evaluation of local tensions through finite elements applied to a large diameter pipe subjected to vacuum condition of a petroleum refinery; Avaliacao das tensoes locais atraves de elementos finitos aplicada a uma tubulacao de grande diametro sujeita a condicao de vacuo de uma dada refinaria de petroleo

    Energy Technology Data Exchange (ETDEWEB)

    Neves, Julio C. Goes; Balbi, Diego J. G. [Promom Engenharia, Rio de Janeiro, RJ (Brazil)

    2012-07-01

    The objective of this paper is to present an evaluation of the results obtained in the study of local stress in wall of large diameter pipe. The case study consists of to analyze a pipeline system with 66 inch, which is responsible for transporting oil, oven to the Tower of vacuum distillation unit in a petroleum refining. The absence of internal pressure leads to a critical with respect to the collapse of the walls of the tube in long sections, without the presence of additional elements increase the rigidity of the geometry. The ASME Section VIII Division 1 advocates the use of additional plates, called stiffeners, which aim to curb the efforts from this condition. Thus, it is necessary structural assessment of critical portions of the system in implementing this solution. Therefore, complementary approaches have been proposed, passing by ASME B31.3, Section VIII Division 1, moreover, a computer simulation of stresses through the finite element method, which the results were analyzed according to criteria of tensions presents in ASME Code Section VIII Division 2. (author)

  4. CARACTERÍSTICAS DE UM LATOSSOLO VERMELHO SOB PASTAGEM NATURAL SUJEITA À AÇÃO PROLONGADA DO FOGO E DE PRÁTICAS ALTERNATIVAS DE MANEJO CHARACTERISTICS OF AN O,XISOL UNDER NATIVE PASTURE SUBMITTED TO FIRE FOR LONG TIME AND ALTERNATIVE MANAGEMENTS

    Directory of Open Access Journals (Sweden)

    Ingrid Heringer

    2002-04-01

    Full Text Available Foram coletadas, em 1998, amostras de solo nas camadas de 0-2,5; 2,5-5,0; 5-10 e 10-30cm, em pastagem natural manejada sob queima sistemática e com distintas alternativas de manejo em relação às queimadas (sem queima, com ou sem roçada, e melhorado com calagem, adubação e introdução de espécies, há 7 e 24 anos, na região dos Campos de Cima da Serra, RS. O delineamento experimental foi o inteiramente casualizado com três repetições. O melhoramento da pastagem natural elevou os teores de Ca, Mg e P no solo, a saturação de bases e o pH e reduziu a acidez potencial. A queima da pastagem natural, em relação às demais áreas sem queima e sem melhoramento, promoveu aumento na acidez potencial e redução nos teores de magnésio na camada mais superficial do solo. A prática de roçada, por um lado aumenta o teor de Mg e a saturação de bases; e por outro, reduz a acidez potencial na superfície do solo, em relação ao solo de pastagem queimada ou só pastejada e sem roçada. Sistemas sem queima apresentam maior quantidade de água e cobertura do solo.Soil samples were taken, in 1998, from distinct layers (0-2.5; 2.5-5.0; 5-10 and 10-30cm in fields with native pasture under grazing, submitted to burning and alternative management practices (without burning with or without mowing, and improved for 7 and 24 years, in the Campos de Cima da Serra region, RS, Brazil. The experimental design was a completely randomized, with three replications. The improvement of native pasture increased the value of pH and the levels Ca, Mg, P and base saturation, and reduced the potential acidity. Biennial burning increased the potential acidity and reduced Mg. The mowing treatment increased the level of Mg and base saturation, and decreased the potencial acidity in the soil surface in comparison to the system without burning and without mowing. Systems without burning were more efficient in water conservation and soil cover.

  5. Mapping Vinyl Cyanide and Other Nitriles in Titan’s Atmosphere Using ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Lai, J. C.-Y.; Cordiner, M. A.; Nixon, C. A.; Achterberg, R. K.; Molter, E. M.; Palmer, M. Y.; Charnley, S. B.; Lindberg, J. E.; Mumma, M. J. [NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States); Teanby, N. A. [School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol, BS8 1RJ (United Kingdom); Kisiel, Z. [Institute of Physics, Polish Academy of Sciences, Al. Lotnikøw 32/46, 02-668 Warszawa (Poland); Irwin, P. G. J., E-mail: martin.cordiner@nasa.gov [Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, University of Oxford, Parks Road, Oxford, OX1 3PU (United Kingdom)

    2017-11-01

    Vinyl cyanide (C{sub 2}H{sub 3}CN) is theorized to form in Titan’s atmosphere via high-altitude photochemistry and is of interest regarding the astrobiology of cold planetary surfaces due to its predicted ability to form cell membrane-like structures (azotosomes) in liquid methane. In this work, we follow up on the initial spectroscopic detection of C{sub 2}H{sub 3}CN on Titan by Palmer et al. with the detection of three new C{sub 2}H{sub 3}CN rotational emission lines at submillimeter frequencies. These new, high-resolution detections have allowed for the first spatial distribution mapping of C{sub 2}H{sub 3}CN on Titan. We present simultaneous observations of C{sub 2}H{sub 5}CN, HC{sub 3}N, and CH{sub 3}CN emission, and obtain the first (tentative) detection of C{sub 3}H{sub 8} (propane) at radio wavelengths. We present disk-averaged vertical abundance profiles, two-dimensional spatial maps, and latitudinal flux profiles for the observed nitriles. Similarly to HC{sub 3}N and C{sub 2}H{sub 5}CN, which are theorized to be short-lived in Titan’s atmosphere, C{sub 2}H{sub 3}CN is most abundant over the southern (winter) pole, whereas the longer-lived CH{sub 3}CN is more concentrated in the north. This abundance pattern is consistent with the combined effects of high-altitude photochemical production, poleward advection, and the subsequent reversal of Titan’s atmospheric circulation system following the recent transition from northern to southern winter. We confirm that C{sub 2}H{sub 3}CN and C{sub 2}H{sub 5}CN are most abundant at altitudes above 200 km. Using a 300 km step model, the average abundance of C{sub 2}H{sub 3}CN is found to be 3.03 ± 0.29 ppb, with a C{sub 2}H{sub 5}CN/C{sub 2}H{sub 3}CN abundance ratio of 2.43 ± 0.26. Our HC{sub 3}N and CH{sub 3}CN spectra can be accurately modeled using abundance gradients above the tropopause, with fractional scale-heights of 2.05 ± 0.16 and 1.63 ± 0.02, respectively.

  6. O INDIVÍDUO: A ALMA DAS ORGANIZAÇÕES

    Directory of Open Access Journals (Sweden)

    Valéria Deluca Soares

    2016-11-01

    Full Text Available O presente artigo tem como proposta fazer uma análise, com base em alguns pressupostos, sobre organizações, cultura e comunicação, com ênfase no indivíduo organizacional. Para tal, com o uso de pesquisa bibliográfica, utilizou-se, como referência, os modelos e/ou teorias dos autores Clegg e Hardy (1999, Hall (1994, Enriquez (2000, Freitas, (1991, 1999, Losicer (1995, Volnovich (1995, Srour (1998, Schein (2001, Trompenaars (1994, Fleury (1989, Motta (1996, Aktouf (1993, Kreps (1995, Goldhaber (1991, Costa (1995, Kunsch (1999, Lindeborg (s.d. e Lite (1997 e Chanlat (1996. Tal discussão busca evidenciar a pertinente necessidade de ampliação das discussões em torno do sujeito organizacional. Palavras-chave: Organização, Indivíduos, Comunicação, Cultura.

  7. A natureza como negação da imortalidade da alma no jovem Feuerbach

    Directory of Open Access Journals (Sweden)

    Eduardo Ferreira Chagas

    2009-12-01

    Full Text Available This article aims at clarifying the two-pointed concept of nature as proposed by young Feuerbach in his work Thoughts on Death and Immortality (Gedanken über Tod und Unsterblichkeit: 1. nature as possibility and condition for all existence within space and time, and 2. nature as negation instance of all being. Nature offers young Feuerbach the model for solution of several oppositions, for one finds within it a dialectical process of assertion and negation, singularity and plurality, individual and gender. Thus, man experiments within nature not only positive assertion but also negation of his existence in the form of his ephemerality and death.

  8. CUERPOS TATUADOS, "ALMAS" TATUADAS: nuevas formas de subjetividad en la contemporaneidad

    Directory of Open Access Journals (Sweden)

    ANDREA LISSETT PÉREZ FONSECA

    2009-01-01

    Full Text Available ESTE ARTÍCULO HACE UNA DESCRIPCIÓN ETNOGRÁFICA CONTEMPORÁNEA DEL TATUAJE, DESDE UNA perspectiva conceptual que prioriza el sentido de práctica, de las interacciones y de las experiencias vividas durante el proceso de tatuarse. Esta reflexión intenta reconstruir una visión holística del tatuaje que abarca el mundo subjetivo de los actores, así como la dinámica social que hace parte de ese acto. Las principales conclusiones son: El surgimiento de una nueva "normalidad" estética y vivencial en el seno de la sociedad Occidental y la configuración de la nueva subjetividad de los "tatuados", entendida como un proceso interactivo, innovador, emotivo y reflexivo, en el que el cuerpo se convierte en forma de expresión y construcción del sujeto.

  9. [Dyslipidemia management in patients with high cardiovascular risk in Spain. ALMA study].

    Science.gov (United States)

    Pintó, Xavier; Trias Vilagut, Ferran; Rius Taruella, Joan; Mairal Sallán, Esther

    2018-01-01

    To assess the attitude of primary care (PCPs) and specialized care (SCPs) physicians towards the general set of patients with dyslipidemia, particularly those with cardiovascular risk factors. Observational, descriptive, multi-center study based on a survey. Different healthcare regions in Spain. 1,402 PCPs, and 596 SCPs. Physician's profile, routine practices in the management of patients with dyslipidemia. 84.3% took the global cardiovascular risk into account when prescribing the treatment. Target LDL-C concentration in patients without cardiovascular risk factors was <130mg/dL and <160mg/dL for 51.9% and 29.0% of physicians, respectively. In smokers and patients with hypertension or diabetes, the LDL target was <100mg/dL for 49-55% of physicians, whereas in patients with cardiovascular complication, ischemic cardiopathy or stroke, target LDL-C was <70mg/dL in 71-88% of them. First-line treatment for patients without cardiovascular risk factors was atorvastatin (66%), whereas in patients with diabetes, kidney disease or metabolic syndrome, most physicians (80-89%) used pitavastatin. SCPs showed a greater trend than PCPs to establish a LDL-C target of <70mg/dL in patients with previous stroke (77.5% vs 66.8%) or coronary disease (92.1% vs 80.6%) (P<.0001), as well as to prescribe a combined treatment in patients not achieving the target LDL-C concentrations (58.1% vs 50.2%, P=.0013). Although CVR assessment is generally accepted, there is broad disagreement in defining the objectives of LDL-C. Most often than PCPs, the SCPs consider more ambitious targets for LDL-C and the association of lipid-lowering drugs. Copyright © 2017 Elsevier España, S.L.U. All rights reserved.

  10. ALMA Astrochemical Observations of the Infrared-luminous Merger NGC 3256

    Science.gov (United States)

    Harada, Nanase; Sakamoto, Kazushi; Martín, Sergio; Aalto, Susanne; Aladro, Rebeca; Sliwa, Kazimierz

    2018-03-01

    In external galaxies, molecular composition may be influenced by extreme environments such as starbursts and galaxy mergers. To study such molecular chemistry, we observed the luminous infrared galaxy and merger NGC 3256 using the Atacama Large Millimeter/submillimeter Array. We covered most of the 3 and 1.3 mm bands for a multispecies, multitransition analysis. We first analyzed intensity ratio maps of selected lines such as HCN/HCO+, which shows no enhancement at an active galactic nucleus. We then compared the chemical compositions within NGC 3256 at the two nuclei, tidal arms, and positions with influence from galactic outflows. We found the largest variation in SiO and CH3OH, species that are likely to be enhanced by shocks. Next, we compared the chemical compositions in the nuclei of NGC 3256, NGC 253, and Arp 220; these galactic nuclei have varying star formation efficiencies. Arp 220 shows higher abundances of SiO and HC3N than NGC 3256 and NGC 253. Abundances of most species do not show a strong correlation with star formation efficiencies, although the CH3CCH abundance seems to have a weak positive correlation with the star formation efficiency. Lastly, the chemistry of spiral arm positions in NGC 3256 is compared with that of W51, a Galactic molecular cloud complex in a spiral arm. We found higher fractional abundances of shock tracers, and possibly also a higher dense gas fraction in NGC 3256 compared with W51.

  11. El sujeto Alma en el discurso filosófico de María Zambrano

    Directory of Open Access Journals (Sweden)

    Sally Abdalla Wahdan

    2016-11-01

    Full Text Available The purpose of this paper is to demonstrate how the Spanish thinker, María Zambrano, transfigures the concept of the "soul" to define and understand the idea of the subject in her contemporary philosophical discourse, developed through the essays she began to write since the 30th of last century. Through her critical thinking of the European rationalism and her adopting of a vision based upon a mediating solution to the old quarrel between Philosophy and Poetry, she reveals the adscriptions of the meaning of the soul and portrays the way or the experience that lead to soul consciousness. The study will shed light on these adscriptions and the confluence of that meaning with the poetic conception within the contemporary context of the Spanish philosopher and of other thinkers, as well.

  12. Des mots maudits, allá en el sur del alma

    Directory of Open Access Journals (Sweden)

    Francisco Albizú Labbé

    2012-08-01

    Full Text Available Ce numéro de la revue Babel est consacré à des mots maudits. Des mots dont le contenu nous est insoutenable. D’autant plus insoutenable qu’ils appartiennent au « dictionnaire de la douleur de chaque peuple », et qu’ils évoquent un autre dictionnaire, celui de l’ignominie universelle. Le substantif « disparition » et son corollaire « disparus » en font partie. L’Amérique latine a le triste privilège d’avoir réactualisé ces mots ; mais l’Espagne de la Guerre civile aussi. Nous pensons, bien ent...

  13. EL POSTULADO DE LA INMORTALIDAD DEL ALMA EN LA FILOSOFÍA MORAL KANTIANA. PARTE I.

    OpenAIRE

    Dulce Ma. Granja

    2013-01-01

    The aim of this article is to clarify the grounds of Kant’s practical postulate of the immortality of the soul. In order to do that, I discuss some passages of the Critique of Pure Reason, in which Kant explains the nature of antinomies and the reasons why these cannot be theoretically solved. After that, my next step will be to elucidate the connection in Kant’s philosophy between the moral law and the intelligible world. By doing so, I explore the arguments in the Groundwork of the Metaphys...

  14. ALMAS EXTERIORES. UMA REFLEXÃO SOBRE MODA E ESCRITURA EM MACHADO DE ASSIS

    Directory of Open Access Journals (Sweden)

    ÉLIDE VALARINI OLIVER

    Full Text Available Resumo Os elementos da indumentária em Machado ultrapassam o mero acessório para assumirem um manancial de significações que os atraem para o centro mesmo da construção da narrativa. Qual a função dos qualia ? São tais elementos contingentes, acessórios ou necessários?

  15. Si-BEARING MOLECULES TOWARD IRC+10216: ALMA UNVEILS THE MOLECULAR ENVELOPE OF CWLeo

    Energy Technology Data Exchange (ETDEWEB)

    Prieto, L. Velilla; Cernicharo, J.; Quintana-Lacaci, G.; Agúndez, M. [Group of Molecular Astrophysics, ICMM, CSIC, C/ Sor Juana Inés de la Cruz 3, E-28049 Cantoblanco, Madrid (Spain); Castro-Carrizo, A.; Guélin, M. [Institut de Radioastronomie Millimétrique, 300 rue de la la Piscine, F-38406 Saint Martin d’Hères (France); Fonfría, J. P. [Departamento de Estrellas y Medio Interestelar, Instituto de Astronomía, Universidad Nacional Autónoma de México (UNAM), Ciudad Universitaria, 04510, Mexico City, México (Mexico); Marcelino, N. [Istituto di Radiastronomia, INAF–CNR, via Gobetti 101, I-40129 Bologna (Italy); Zúñiga, J.; Requena, A.; Bastida, A. [Departamento de Química Física, Facultad de Química, Universidad de Murcia, Campus Espinardo, E-30100 Murcia (Spain); Lique, F. [LOMC–UMR 6294, CNRS–Université du Havre, 25 rue Philippe Lebon, BP 1123, F-76063 Le Havre cedex (France)

    2015-06-01

    We report the detection of SiS rotational lines in high-vibrational states as well as SiO and SiC{sub 2} lines in their ground vibrational state toward IRC+10216 during the Atacama Large Millimeter Array Cycle 0. The spatial distribution of these molecules shows compact emission for SiS and a more extended emission for SiO and SiC{sub 2} and also proves the existence of an increase in the SiC{sub 2} emission at the outer shells of the circumstellar envelope (CSE). We analyze the excitation conditions of the vibrationally excited SiS using the population diagram technique, and we use a large velocity gradient model to compare with the observations. We found moderate discrepancies between the observations and the models that could be explained if SiS lines detected are optically thick. Additionally, the line profiles of the detected rotational lines in the high-energy vibrational states show a decreasing linewidth with increasing energy levels. This may be evidence that these lines could be excited only in the inner shells, i.e., the densest and hottest, of the CSE of IRC+10216.

  16. Analytical Models of Spirals in Stellar Winds to Interpret ALMA Data

    NARCIS (Netherlands)

    Homan, W.; Decin, L.; de Koter, A.; van Marle, A.J.; Lombaert, R.; Vlemmings, W.H.T.

    2015-01-01

    Observations of stellar winds have shown that these outflows are non-homogeneous and might harbor structural complexities on macro- and microscales. Here, we focus on spiral structures with the aim to expand our understanding of the manifestation of such structures in the (one- and

  17. Exploring the CO/CN line ratio in nearby galaxies with the ALMA archive

    Science.gov (United States)

    Wilson, Christine D.

    2018-03-01

    We describe an archival project using Cycle 0 data from the Atacama Large Millimeter/submilleter Array to survey the CO/CN line ratio in 17 nearby galaxies. CN is an interesting molecule that traces dense gas exposed to ultraviolet radiation and its N = 1 - 0 lines can be observed simultaneously with the CO J = 1 - 0 line. We identify 8 galaxies with distances starburst-dominated regions, which may be in conflict with models of molecular abundances in X-ray dominated regions.

  18. Why complexity matters: using ALMaSS for risk assessment of wildlife

    DEFF Research Database (Denmark)

    Topping, Christopher John

    The primary focus of environmental risk assessment (ERA) for non-target organisms is on the direct effect of the toxicant. In some cases what are often termed large-scale sources of variation are also considered (e.g. expected crop distribution). However, these describe only part of the variation...

  19. EL POSTULADO DE LA INMORTALIDAD DEL ALMA EN LA FILOSOFÍA MORAL KANTIANA. PARTE I.

    Directory of Open Access Journals (Sweden)

    Dulce Ma. Granja

    2013-11-01

    Full Text Available The aim of this article is to clarify the grounds of Kant’s practical postulate of the immortality of the soul. In order to do that, I discuss some passages of the Critique of Pure Reason, in which Kant explains the nature of antinomies and the reasons why these cannot be theoretically solved. After that, my next step will be to elucidate the connection in Kant’s philosophy between the moral law and the intelligible world. By doing so, I explore the arguments in the Groundwork of the Metaphysics of Morals and the Critique of Practical Reason that prove that there is a practical access to the intelligible world, which is banned to those who consider the problems of antinomies –specially, the problem of human freedom– solely from a theoretical standpoint. I then reconstruct Kant’s view about the nature of practical postulates. In this regard, my analysis will focus on the notion of moral progress, which is, according to Kant, the actual motive that prompts us human beings to suppose legitimately our enduring existence after death. Lastly, I discuss the problematic nature of the notion of moral progress –which implies temporality–, and try to provide some reasonable grounds as to why it is nevertheless sound and cogent within Kant’s system.

  20. Dust attenuation in 2 galaxies from deep ALMA observations of the Hubble Ultra Deep Field

    Science.gov (United States)

    McLure, R. J.; Dunlop, J. S.; Cullen, F.; Bourne, N.; Best, P. N.; Khochfar, S.; Bowler, R. A. A.; Biggs, A. D.; Geach, J. E.; Scott, D.; Michałowski, M. J.; Rujopakarn, W.; van Kampen, E.; Kirkpatrick, A.; Pope, A.

    2018-05-01

    We present the results of a new study of the relationship between infrared excess (IRX ≡ LIR/LUV), ultraviolet (UV) spectral slope (β) and stellar mass at redshifts 2 galaxies in the mass range 9.25≤ log (M_{\\ast }/M_{⊙}) ≤ 10.75 are fully consistent with the IRX-β relation expected for a relatively grey attenuation curve, similar to the commonly adopted Calzetti law. Based on a large, mass-complete sample of 2 ≤ z ≤ 3 star-forming galaxies drawn from multiple surveys, we proceed to derive a new empirical relationship between β and stellar mass, making it possible to predict UV attenuation (A1600) and IRX as a function of stellar mass, for any assumed attenuation law. Once again, we find that z ≃ 2.5 star-forming galaxies follow A1600-M* and IRX-M* relations consistent with a relatively grey attenuation law, and find no compelling evidence that star-forming galaxies at this epoch follow a reddening law as steep as the Small Magellanic Cloud (SMC) extinction curve. In fact, we use a simple simulation to demonstrate that previous determinations of the IRX-β relation may have been biased towards low values of IRX at red values of β, mimicking the signature expected for an SMC-like dust law. We show that this provides a plausible mechanism for reconciling apparently contradictory results in the literature and that, based on typical measurement uncertainties, stellar mass provides a cleaner prediction of UV attenuation than β. Although the situation at lower stellar masses remains uncertain, we conclude that for 2 galaxies with log (M_{\\ast }/M_{⊙}) ≥ 9.75, both the IRX-β and IRX-M* relations are well described by a Calzetti-like attenuation law.

  1. De las pasiones del alma a la arquitectura: un paralelismo entre lenguajes

    OpenAIRE

    Pozo Alemán, Patricia

    2018-01-01

    Este artículo estudia el paralelismo que se crea entre el lenguaje de la literatura y el lenguaje de la arquitectura, tomando como base el Tratado de las pasiones de Descartes, y cómo las emociones y la expresión se trasladan de las palabras al dibujo, de ahí a la escultura, después a la arquitectura antropomórfica, y por último a la arquitectura contemporánea, para cerrar el círculo volviendo a la literatura propia de la estética y el arte.

  2. El objeto de la psicología: el alma como cultura encarnada

    OpenAIRE

    Ortíz Vanegas, Jennifer

    2013-01-01

    A lo largo de la historia de la psicología se ha evidenciado la dificultad para establecer un objeto de estudio común a todas las escuelas y corrientes psicológicas que, a pesar de ser tan diferentes y en ocasiones opuestas o contradictorias, reclaman ser psicología. Esta situación nos ha hecho preguntarnos si, dadas esas condiciones, es posible delimitar un objeto de estudio en el que confluyan las diferentes escuelas y corrientes psicológicas, pero sin que ello implique la exclusión de algu...

  3. “O Homem que Fora Consumido” – Um Conto da “Alma Exterior”

    Directory of Open Access Journals (Sweden)

    Maria Alice Ribeiro Gabriel

    2015-01-01

    Full Text Available http://dx.doi.org/10.5007/2175-8026.2015v68n2p43 Como ver o corpo além de sua materialidade é, obviamente, uma das maiores preocupações da ficção gótica de Edgar Allan Poe: “Metzengerstein”, “Morella”, “Ligeia”, “Uma estória das montanhas Ragged”, “Revelação mesmérica” e “Os fatos no caso de monsieur Valdemar” são alguns exemplos. Mas em seu grotesque cômico “O homem que fora consumido – Uma história das velhas campanhas dos Bugaboos e Kickapoos”, o humor negro e a sátira social prevalecem quando a trama centra-se no famoso brigadeiro por distinção John A. B. C. Smith e na obsessão do protagonista “Sobre este assunto – o do aspecto pessoal de Smith”. Este artigo pretende estabelecer algumas observações sobre as personagens do general Smith e do narrador não nomeado, utilizando como parâmetro teórico para esta análise os conceitos de patologia da adaptação, de Mahmoud Sami-Ali, e os de personalidade narcísica e estado-limite, desenvolvidos por Didier Anzieu.

  4. Heavy Rain y Beyond: Dos almas. Dramas interactivos en la narración transmedia

    Directory of Open Access Journals (Sweden)

    Jafet Israel Lara

    2014-06-01

    Full Text Available Since the nineties, transmedia storytelling has begun to spread through the new virtual avenues of information society of the 21st century. As part of these narratives is the “interactive drama”, which involves an exchange of technologies of film and videogame industry and restarts on different media and platforms. The purpose of this study is to analyze two “interactive dramas”: Heavy Rain and Beyond. Two Souls by director and developer David Cage. This research will see that these two games are part of the transmedia narrative, that offer new hybrid narrative forms, changing the reader in an interactive user. Also, there will be study the speech of the “interactive drama ” and its evolution in both dramatic-interactive texts.

  5. PEDAGOGIA JESUÍTICA E ALTERIDADE: A DEMONIZAÇÃO DA ALMA INDÍGENA

    Directory of Open Access Journals (Sweden)

    Fábio Eduardo Cressoni

    2012-10-01

    Full Text Available RESUMO:Este trabalho pretende discutir as dificuldades presentes no processo inicial de colonização da América portuguesa quando do processo de catequese / cristianização dos índios Tupinambá. Nesse sentido, demonstramos a relação entre estas dificuldades e a ação dos caraíbas nas aldeias, bem como a conseqüente demonização dos ritos e práticas indígenas. Logo, procuramos indicar os motivos pelos quais os padres da Companhia de Jesus passaram a condenar e demonizar os caraíbas e suas práticas e representações perante a sociedade Tupinambá quinhentista.PALAVRAS-CHAVE: América portuguesa; Companhia de Jesus; AlteridadeABSTRACT: This paper discusses the difficulties present in the initial process of colonization of Portuguese America when the process of catechesis / Christianization of the Tupinambá Indians. In this sense, we show the relationship between these problems and the action of the Caribbean in the villages, as well as the subsequent demonization of indigenous rites and practices. Therefore, the authors highlight the reasons why the Company's priests of Jesus began to condemn and demonize the Caribbean and its practices and representations before the sixteenth century Tupinambá society. KEYWORDS: Portuguese America; Society of Jesus; othernessRecebido: 30/06/2012       Aceito:19/10/2012

  6. Bullying e semiótica: um estudo dos estados de alma dos sujeitos

    Directory of Open Access Journals (Sweden)

    Marisa Ferreira Aderaldo

    2012-04-01

    Full Text Available Neste artigo, a análise se fundamenta no nível narrativo do percurso da produção de sentido e explora o conceito de paixão (LARA e MATTE, 2009 para formular a hipótese de que o agente do bullying pode ser identificado por um perfil patêmico, cuja satisfação ou realização tem como meta estimular a abulia ou ausência de um querer no outro; neste caso, o bulizado. O trabalho analisa uma ocorrência verídica de bullying contra uma pessoa com deficiência visual e aponta para paixões como malevolência, em relação ao bulizador (ou bulidor, e decepção, frustração e resignação, em relação ao bulizado (ou bulido, paixões que são identificadas, intradiscursivamente, nesta reflexão que problematiza o tema do (desempoderamento da pessoa com deficiência e o bullying.

  7. Maria Metade e as Incompletudes da Alma: o Ser Plural Moçambicano

    Directory of Open Access Journals (Sweden)

    Cristian Paula Santana

    2016-12-01

    Full Text Available We intend in this article to analyze the tale "Meia culpa, meia própria culpa," by Mia Couto, showing one of many possible perspectives of analysis of the author's work. Our analysis has by objective to explicit the between-place in Couto´s discourse, highlighting the social practices present in literary discourse, showing how the author relates his personages with the story of Mozambique and verifying the representation of the female figure from the perspective of identity in construction. We think the work of Mia Couto through antagonistic relations: colonizer / colonized, man / woman, white / black, dominating / dominated, etc. We chose this perspective because Mia Couto be a plural writer and Mozambique is a diverse country.We have as theoretical support Pierre Bourdieu with the work A dominação masculina (2012 to highlight the function of women and the social practices; also we rely on theorists such as Stuart Hall, A identidade cultural na pós-modernidade (2011 and Frantz Fanon Pele negra, máscaras brancas (2008, among others, to discuss the issues of identity.

  8. ALMA reveals sunburn: CO dissociation around AGB stars in the globular cluster 47 Tucanae

    OpenAIRE

    McDonald, Iain; Zijlstra, Albert A.; Lagadec, Eric; Sloan, Gregory C.; Boyer, Martha L.; Matsuura, Mikako; Smith, Rowan J.; Smith, Christina L.; Yates, Jeremy A.; van Loon, Jacco Th.; Jones, Olivia C.; Ramstedt, Sofia; Avison, Adam; Justtanont, Kay; Olofsson, Hans

    2015-01-01

    Atacama Large Millimetre Array observations show a non-detection of carbon monoxide around the four most luminous asymptotic giant branch (AGB) stars in the globular cluster 47 Tucanae. Stellar evolution models and star counts show that the mass-loss rates from these stars should be similar to 1.2-3.5x10(-7) M-circle dot yr(-1). We would naively expect such stars to be detectable at this distance (4.5 kpc). By modelling the ultraviolet radiation field from post-AGB stars and white dwarfs in 4...

  9. Ni "almas bellas" ni "guerreros justos": mujeres implicadas en violencia política

    Directory of Open Access Journals (Sweden)

    Concepción Fernández Villanueva

    2011-12-01

    Full Text Available La implicación de las mujeres en violencia política ha sido invisibilizada, marginalizada y desvalorizada. Estudios recientes sobre su participación en conflictos bélicos, movimientos de resistencia, movimientos revolucionarios y grupos terroristas a lo largo del siglo XX y XXI permiten rescatar la visibilidad de este fenómeno así como interpretarlo a la luz de los procesos psicosociales del contexto, que son similares a los que explican la implicación de los varones: en particular, los procesos grupales y comunitarios de carácter psicosocial, la ideología política, y la transformación de la identidad de género en un momento histórico de conquista de la igualdad. Los estereotipos sexistas e incluso algunas interpretaciones de la psicología diferencial de los géneros contribuyen a distorsionar la explicación de la implicación de las mujeres en esta y otras formas de violencia. The involvement of women in political violence has been hidden, marginalized and devalued. Recent studies about involvement of women in armed conflicts, resistance movements, revolutionary movements and terrorist groups throughout the twentieth and twentieth-first centuries can rescue the visibility of this phenomenon and interpret it in the light of the psychosocial processes of the context, similar to those that explain the involvement of men: particularly, group and community psychosocial processes, political ideology, and gender identity transformation towards women equality. Sexist stereotypes and even some interpretations of the psychology of gender differences help to distort the explanation of the involvement of women in this and other forms of violence.

  10. Pragmática, sociedade (e a alma, uma entrevista com Jacob Mey

    Directory of Open Access Journals (Sweden)

    Daniel do Nascimento e Silva

    2014-01-01

    Full Text Available Jacob Mey, o linguista que fundou (em 1977, com Hartmut Haberland o Journal of Pragmatics e autor de inúmeros livros e artigos no campo da pragmática, visitou o Brasil em novembro/dezembro de 2012, por ocasião da homenagem ao trabalho do pragmaticista Kanavillil Rajagopalan, realizada na Unicamp, onde Rajagopalan desenvolveu trabalho exemplar. A visita de Mey ao Brasil foi uma convite à reflexão sobre o objeto da pragmática, suas vizinhanças, seus principais problemas e sua agenda. Esta entrevista, realizada no Rio de Janeiro, conta a trajetória de Jacob Mey e sua visada crítica sobre os principais temas e problemas da pragmática.

  11. VLA AND ALMA IMAGING OF INTENSE GALAXY-WIDE STAR FORMATION IN z ∼ 2 GALAXIES

    Energy Technology Data Exchange (ETDEWEB)

    Rujopakarn, W.; Silverman, J. D. [Kavli Institute for the Physics and Mathematics of the universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583 (Japan); Dunlop, J. S.; Ivison, R. J.; McLure, R. J.; Michałowski, M. J. [Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Rieke, G. H. [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Cibinel, A. [Astronomy Centre, Department of Physics and Astronomy, University of Sussex, Brighton, BN1 9QH (United Kingdom); Nyland, K. [National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States); Jagannathan, P.; Bhatnagar, S. [National Radio Astronomy Observatory, Socorro, NM 87801 (United States); Alexander, D. M. [Department of Physics, Durham University, Durham DH1 3LE (United Kingdom); Biggs, A. D. [European Southern Observatory, Karl-Schwarzschild-Straße 2, Garching (Germany); Ballantyne, D. R. [Center for Relativistic Astrophysics, School of Physics, Georgia Institute of Technology, Atlanta, GA 30332 (United States); Dickinson, M. [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Elbaz, D. [CEA Saclay, DSM/Irfu/Service d’Astrophysique, Orme des Merisiers, F-91191 Gif-sur-Yvette Cedex (France); Geach, J. E. [Center for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield AL10 9AB (United Kingdom); Hayward, C. C. [Center for Computational Astrophysics, 160 Fifth Avenue, New York, NY 10010 (United States); Kirkpatrick, A., E-mail: wiphu.rujopakarn@ipmu.jp [Yale Center for Astronomy and Astrophysics, Physics Department, P.O. Box 208120, New Haven, CT 06520 (United States); and others

    2016-12-10

    We present ≃0.″4 resolution extinction-independent distributions of star formation and dust in 11 star-forming galaxies (SFGs) at z  = 1.3–3.0. These galaxies are selected from sensitive blank-field surveys of the 2′ × 2′ Hubble Ultra-Deep Field at λ  = 5 cm and 1.3 mm using the Karl G. Jansky Very Large Array and Atacama Large Millimeter/submillimeter Array. They have star formation rates (SFRs), stellar masses, and dust properties representative of massive main-sequence SFGs at z  ∼ 2. Morphological classification performed on spatially resolved stellar mass maps indicates a mixture of disk and morphologically disturbed systems; half of the sample harbor X-ray active galactic nuclei (AGNs), thereby representing a diversity of z  ∼ 2 SFGs undergoing vigorous mass assembly. We find that their intense star formation most frequently occurs at the location of stellar-mass concentration and extends over an area comparable to their stellar-mass distribution, with a median diameter of 4.2 ± 1.8 kpc. This provides direct evidence of galaxy-wide star formation in distant blank-field-selected main-sequence SFGs. The typical galactic-average SFR surface density is 2.5 M {sub ⊙} yr{sup −1} kpc{sup −2}, sufficiently high to drive outflows. In X-ray-selected AGN where radio emission is enhanced over the level associated with star formation, the radio excess pinpoints the AGNs, which are found to be cospatial with star formation. The median extinction-independent size of main-sequence SFGs is two times larger than those of bright submillimeter galaxies, whose SFRs are 3–8 times larger, providing a constraint on the characteristic SFR (∼300 M {sub ⊙} yr{sup −1}) above which a significant population of more compact SFGs appears to emerge.

  12. Central repository for low- and intermediate-level waste (ALMA) conceptual design, siting and safety study

    International Nuclear Information System (INIS)

    Kjellbert, N.; Haeggblom, H.; Cederstroem, M.; Lundgren, T.

    1980-07-01

    A generic design, siting and safety study of a proposed repository for low- and intermediate-level waste has been made. Special emphasis has been placed on safety characterostics. The conceptual design and the generic site, on which the study is based, are realistically chosen in accordance with present construction techniques and the existing geohydrological conditions in Sweden. (Auth.)

  13. Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA

    Science.gov (United States)

    Indebetouw, R.; Matsuura, M.; Dwek, E.; Zanardo, G.; Barlow, M. J.; Baes, M.; Bouchet, P.; Burrows, D. N.; Chevalier, R.; Clayton, G. C.; hide

    2014-01-01

    Supernova (SN) explosions are crucial engines driving the evolution of galaxies by shock heating gas, increasing the metallicity, creating dust, and accelerating energetic particles. In 2012 we used the Atacama Large Millimeter/ Submillimeter Array to observe SN1987A, one of the best-observed supernovae since the invention of the telescope. We present spatially resolved images at 450 µm, 870 µm, 1.4 mm, and 2.8 mm, an important transition wavelength range. Longer wavelength emission is dominated by synchrotron radiation from shock-accelerated particles, shorter wavelengths by emission from the largest mass of dust measured in a supernova remnant (>0.2 Solar Mass). For the first time we show unambiguously that this dust has formed in the inner ejecta (the cold remnants of the exploded star's core). The dust emission is concentrated at the center of the remnant, so the dust has not yet been affected by the shocks. If a significant fraction survives, and if SN 1987A is typical, supernovae are important cosmological dust producers.

  14. Programas trainees corporativos e o governo das almas Trainees corporate programs and the government of souls

    Directory of Open Access Journals (Sweden)

    Jairo Antônio da Cruz

    2012-04-01

    Full Text Available O artigo busca problematizar as transformações do trabalho na passagem da Modernidade para a Contemporaneidade, e alguns de seus efeitos nos domínios educacionais. Para tanto, mostramos o deslocamento de ênfase de um trabalho fabril para um trabalho que vem sendo chamado imaterial, que já não prioriza um sistema baseado na obediência a regulamentos e na vigilância do corpo. Sua organização lança mão de formas muito mais sutis de poder, apoiando-se em formas mais sofisticadas e complexas de atuar sobre os sujeitos. Esse quadro teórico serve de suporte para a análise de três programas trainees corporativos, que buscam capturar "grandes talentos" egressos de cursos superiores e torná-los fiéis colaboradores das organizações empresariais, fazendo com que desejem e passem a agir como autoem-presários prestadores de serviços.The article attempts to discuss changes in work in the passage from Modernity to Contemporary and some of its effects in education. For this, we show the displacement in emphasis from a factory work, guided by a disciplinary organization, to a work that is being called immaterial. This is no longer a priority a system based on obedience to rules and surveillance of the body. Its organization makes use of more subtle forms of power, relying on more sophisticated and complex ways of acting on the subject. This theoretical framework supports the analysis of three trainees corporate programs, whose purpose is capturing "great talents" graduates from colleges and making them loyal employees of business organizations, making they wish and start to act as self-entrepreneurs service providers.

  15. ALMA Thermal Observations of a Proposed Plume Source Region on Europa

    Energy Technology Data Exchange (ETDEWEB)

    Trumbo, Samantha K.; Brown, Michael E. [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States); Butler, Bryan J. [National Radio Astronomy Observatory, Socorro, NM 87801 (United States)

    2017-10-01

    We present a daytime thermal image of Europa taken with the Atacama Large Millimeter Array. The imaged region includes the area northwest of Pwyll Crater, which is associated with a nighttime thermal excess seen by the Galileo Photopolarimeter Radiometer and with two potential plume detections. We develop a global thermal model of Europa and simulate both the daytime and nighttime thermal emission to determine if the nighttime thermal anomaly is caused by excess endogenic heat flow, as might be expected from a plume source region. We find that the nighttime and daytime brightness temperatures near Pwyll Crater cannot be matched by including excess heat flow at that location. Rather, we can successfully model both measurements by increasing the local thermal inertia of the surface.

  16. ALMA REVEALS POTENTIAL LOCALIZED DUST ENRICHMENT FROM MASSIVE STAR CLUSTERS IN II Zw 40

    Energy Technology Data Exchange (ETDEWEB)

    Consiglio, S. Michelle; Turner, Jean L. [Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095 (United States); Beck, Sara [Department of Physics and Astronomy, University of Tel Aviv, Ramat Aviv (Israel); Meier, David S., E-mail: smconsiglio@ucla.edu [Department of Physics, New Mexico Institute of Mining and Technology, Socorro, NM 87801 (United States)

    2016-12-10

    We present subarcsecond images of submillimeter CO and continuum emission from a local galaxy forming massive star clusters: the blue compact dwarf galaxy II Zw 40. At ∼0.″4 resolution (20 pc), the CO(3-2), CO(1-0), 3 mm, and 870 μ m continuum maps illustrate star formation on the scales of individual molecular clouds. Dust contributes about one-third of the 870 μ m continuum emission, with free–free accounting for the rest. On these scales, there is not a good correspondence between gas, dust, and free–free emission. Dust continuum is enhanced toward the star-forming region as compared to the CO emission. We suggest that an unexpectedly low and spatially variable gas-to-dust ratio is the result of rapid and localized dust enrichment of clouds by the massive clusters of the starburst.

  17. ALMA observations of the supergiant B[e] star Wd1-9

    Science.gov (United States)

    Fenech, D. M.; Clark, J. S.; Prinja, R. K.; Morford, J. C.; Dougherty, S.; Blomme, R.

    2017-01-01

    Mass-loss in massive stars plays a critical role in their evolution, although the precise mechanism(s) responsible - radiatively driven winds, impulsive ejection and/or binary interaction - remain uncertain. In this Letter, we present Atacama Large Millimetre/Submillimeter Array line and continuum observations of the supergiant B[e] star Wd1-9, a massive post-main-sequence object located within the starburst cluster Westerlund 1 (Wd1). We find it to be one of the brightest stellar point sources in the sky at millimetre wavelengths, with (serendipitously identified) emission in the H41α radio recombination line. We attribute these properties to a low velocity (˜100 km s-1 ) ionized wind, with an extreme mass-loss rate ≳6.4 × 10-5(d/5 kpc)1.5 M⊙yr- 1. External to this is an extended aspherical ejection nebula indicative of a prior phase of significant mass-loss. Taken together, the millimetre properties of Wd1-9 show a remarkable similarity to those of the highly luminous stellar source MWC349A. We conclude that these objects are interacting binaries evolving away from the main sequence and undergoing rapid case-A mass transfer. As such they - and by extension the wider class of supergiant B[e] stars - may provide a unique window into the physics of a process that shapes the life-cycle of ˜70 per cent of massive stars found in binary systems.

  18. El perverso juego de la pederastia: Poder-violencia sobre las almas

    OpenAIRE

    Tamayo, Juan José

    2017-01-01

    Este artículo trata sobre la permisividad del delito, el silencio, la falta de castigo, el encubrimiento, la complicidad y la negativa a colaborar con la justicia que convierten la pederastia no solo en una agresión sexual individual, sino en una práctica legitimada estructural e institucionalmente –al menos de manera indirecta– por la jerarquía eclesiástica en todos sus niveles en una cadena de ocultamiento que va desde la más alta autoridad eclesiástica hasta el pederasta, pasando por los e...

  19. GRB 110715A: the peculiar multiwavelength evolution of the first afterglow detected by ALMA

    Czech Academy of Sciences Publication Activity Database

    Sánchez-Ramírez, R.; Hancock, P. J.; Johannesson, G.; Murphy, T.; de Ugarte Postigo, A.; Gorosabel, J.; Kann, D.A.; Kruehler, T.; Oates, S.R.; Japelj, J.; Thöne, C.C.; Lundgren, A.; Perley, D.A.; Malesani, D.; de Gregorio Monsalvo, I.; Castro-Tirado, A.J.; D'Elia, V.; Fynbo, J. P. U.; Garcia-Appadoo, D.; Goldoni, P.; Greiner, J.; Hu, Y.D.; Jelínek, Martin; Jeong, S.; Kamble, S.; Klose, S.; Kuindersma, S.; Llorente, A.; Martin, S.; Guelbenzu, A. N.; Rossi, A.; Schady, P.; Sparrer, G.; Sudilovsky, V.; Tello, J. C.; Updike, A.; Wiersema, K.; Zhang, B.B.

    2017-01-01

    Roč. 464, č. 4 (2017), s. 4624-4640 ISSN 0035-8711 Institutional support: RVO:67985815 Keywords : gamma-ray burst * vlt/x-shooter spectroscopy * host galaxy Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics OBOR OECD: Astronomy (including astrophysics,space science) Impact factor: 4.961, year: 2016

  20. Is the Alma Ata vision of comprehensive primary health care viable? Findings from an international project.

    Science.gov (United States)

    Labonté, Ronald; Sanders, David; Packer, Corinne; Schaay, Nikki

    2014-01-01

    The 4-year (2007-2011) Revitalizing Health for All international research program (http://www.globalhealthequity.ca/projects/proj_revitalizing/index.shtml) supported 20 research teams located in 15 low- and middle-income countries to explore the strengths and weaknesses of comprehensive primary health care (CPHC) initiatives at their local or national levels. Teams were organized in a triad comprised of a senior researcher, a new researcher, and a 'research user' from government, health services, or other organizations with the authority or capacity to apply the research findings. Multiple regional and global team capacity-enhancement meetings were organized to refine methods and to discuss and assess cross-case findings. Most research projects used mixed methods, incorporating analyses of qualitative data (interviews and focus groups), secondary data, and key policy and program documents. Some incorporated historical case study analyses, and a few undertook new surveys. The synthesis of findings in this report was derived through qualitative analysis of final project reports undertaken by three different reviewers. Evidence of comprehensiveness (defined in this research program as efforts to improve equity in access, community empowerment and participation, social and environmental health determinants, and intersectoral action) was found in many of the cases. Despite the important contextual differences amongst the different country studies, the similarity of many of their findings, often generated using mixed methods, attests to certain transferable health systems characteristics to create and sustain CPHC practices. These include:1. Well-trained and supported community health workers (CHWs) able to work effectively with marginalized communities2. Effective mechanisms for community participation, both informal (through participation in projects and programs, and meaningful consultation) and formal (though program management structures)3. Co-partnership models in program and policy development (in which financial and knowledge supports from governments or institutions are provided to communities, which retain decision-making powers in program design and implementation)4. Support for community advocacy and engagement in health and social systems decision makingThese characteristics, in turn, require a political context that supports state responsibilities for redistributive health and social protection measures.

  1. Is the Alma Ata vision of comprehensive primary health care viable? Findings from an international project

    Directory of Open Access Journals (Sweden)

    Ronald Labonté

    2014-08-01

    Full Text Available Background: The 4-year (2007–2011 Revitalizing Health for All international research program (http://www.globalhealthequity.ca/projects/proj_revitalizing/index.shtml supported 20 research teams located in 15 low- and middle-income countries to explore the strengths and weaknesses of comprehensive primary health care (CPHC initiatives at their local or national levels. Teams were organized in a triad comprised of a senior researcher, a new researcher, and a ‘research user’ from government, health services, or other organizations with the authority or capacity to apply the research findings. Multiple regional and global team capacity-enhancement meetings were organized to refine methods and to discuss and assess cross-case findings. Objective: Most research projects used mixed methods, incorporating analyses of qualitative data (interviews and focus groups, secondary data, and key policy and program documents. Some incorporated historical case study analyses, and a few undertook new surveys. The synthesis of findings in this report was derived through qualitative analysis of final project reports undertaken by three different reviewers. Results: Evidence of comprehensiveness (defined in this research program as efforts to improve equity in access, community empowerment and participation, social and environmental health determinants, and intersectoral action was found in many of the cases. Conclusions: Despite the important contextual differences amongst the different country studies, the similarity of many of their findings, often generated using mixed methods, attests to certain transferable health systems characteristics to create and sustain CPHC practices. These include: 1. Well-trained and supported community health workers (CHWs able to work effectively with marginalized communities 2. Effective mechanisms for community participation, both informal (through participation in projects and programs, and meaningful consultation and formal (though program management structures 3.Co-partnership models in program and policy development (in which financial and knowledge supports from governments or institutions are provided to communities, which retain decision-making powers in program design and implementation 4. Support for community advocacy and engagement in health and social systems decision making These characteristics, in turn, require a political context that supports state responsibilities for redistributive health and social protection measures.

  2. The Density of Mid-sized Kuiper Belt Objects from ALMA Thermal Observations

    Energy Technology Data Exchange (ETDEWEB)

    Brown, Michael E. [California Institute of Technology, 1200 E California Blvd., Pasadena CA 91125 (United States); Butler, Bryan J. [National Radio Astronomy Observatory, 1003 Lopezville Rd., Socorro NM 87801 (United States)

    2017-07-01

    The densities of mid-sized Kuiper Belt objects (KBOs) are a key constraint in understanding the assembly of objects in the outer solar system. These objects are critical for understanding the currently unexplained transition from the smallest KBOs with densities lower than that of water, to the largest objects with significant rock content. Mapping this transition is made difficult by the uncertainties in the diameters of these objects, which maps into an even larger uncertainty in volume and thus density. The substantial collecting area of the Atacama Large Millimeter Array allows significantly more precise measurements of thermal emission from outer solar system objects and could potentially greatly improve the density measurements. Here we use new thermal observations of four objects with satellites to explore the improvements possible with millimeter data. We find that effects due to effective emissivity at millimeter wavelengths make it difficult to use the millimeter data directly to find diameters and thus volumes for these bodies. In addition, we find that when including the effects of model uncertainty, the true uncertainties on the sizes of outer solar system objects measured with radiometry are likely larger than those previously published. Substantial improvement in object sizes will likely require precise occultation measurements.

  3. Mosquito vector abundance immediately before and after tropical storms Alma and Arthur, northern Belize, 2008 Abundancia de mosquitos vectores inmediatamente antes y después de las tormentas tropicales Alma y Arthur, norte de Belice, 2008

    OpenAIRE

    Meredith G Morrow; Richard N Johnson; Jorge Polanco; David M Claborn

    2010-01-01

    OBJECTIVE: To monitor adult mosquito abundance in northern Belize before/after the first tropical storm of the wet season to estimate the time required for development/recovery of potential vector populations; determine which species predominate post-storm; and compare the effectiveness of two types of mosquito traps-octenol-baited Mosquito Magnets® and U.S. Centers for Disease Control and Prevention (CDC) light traps (with/without octenol). METHODS: Field experiments were conducted in Orange...

  4. Mosquito vector abundance immediately before and after tropical storms Alma and Arthur, northern Belize, 2008 Abundancia de mosquitos vectores inmediatamente antes y después de las tormentas tropicales Alma y Arthur, norte de Belice, 2008

    Directory of Open Access Journals (Sweden)

    Meredith G Morrow

    2010-07-01

    Full Text Available OBJECTIVE: To monitor adult mosquito abundance in northern Belize before/after the first tropical storm of the wet season to estimate the time required for development/recovery of potential vector populations; determine which species predominate post-storm; and compare the effectiveness of two types of mosquito traps-octenol-baited Mosquito Magnets® and U.S. Centers for Disease Control and Prevention (CDC light traps (with/without octenol. METHODS: Field experiments were conducted in Orange Walk Town, Belize, 21 May to 3 June 2008. Incidence rate ratios and exact binomial 95% confidence intervals were reported and trap-nights calculated to compare species abundance pre- and post-storm as well as trap-type effectiveness. RESULTS: Twice as many species and three times more Anopheles spp. were trapped pre-storm versus post-storm. However, greater numbers of Aedes taeniorhynchus and Culex (Culex spp. were trapped post-storm. Mosquito Magnets® were consistently more effective than the CDC traps, obtaining twice as many Anopheles spp. and four times as many culicine species as the octenol-baited version (which collected 14 times more mosquitoes overall and 3.5 times more culicine species than the unbaited version. The unbaited CDC trap did not trap any Anopheles spp. during the study period. CONCLUSIONS: Results indicated octenol is an effective attractant for An. crucians in northern Belize; malaria risk in Belize declines immediately post-storm (i.e., mosquito abundance drops; and arboviral risk associated with the rapid increase in culicine mosquitoes post-storm may represent a greater public health threat than malaria (although further research and active disease surveillance is necessary to validate this hypothesis.OBJETIVO: Comprobar la abundancia de mosquitos adultos en el norte de Belice antes y después de la primera tormenta tropical de la temporada de lluvias, para calcular la cantidad de tiempo que necesitan las poblaciones de vectores potenciales para desarrollarse y recuperarse; determinar cuáles son las especies que predominan después de la tormenta; y comparar la eficacia de dos tipos de trampas de mosquitos: las que utilizan cebos de octenol (Mosquito Magnets® y las trampas de luz con y sin octenol de los Centros para el Control y la Prevención de Enfermedades de los Estados Unidos (CDC. MÉTODOS: Se llevaron a cabo pruebas de campo en Orange Walk Town, Belice, desde el 21 de mayo hasta el 3 de junio del 2008. Se registraron las razones de las tasas de incidencia y los intervalos de confianza binomiales exactos de 95% y se evaluaron las trampas nocturnas para comparar la abundancia de las especies y la eficacia del tipo de trampa antes y después de una tormenta. RESULTADOS: Antes de la tormenta, se atrapó el doble de las especies de mosquitos y el triple de Anopheles spp. en comparación con el período que siguió a la tormenta. Sin embargo, el número de Aedes taeniorhynchus y Culex (Culex spp. atrapados fue mayor después de la tormenta. Las trampas Mosquito Magnets® demostraron uniformemente ser más eficaces que las trampas de los CDC, ya que el número de Anopheles spp. capturados fue dos veces mayor que el de la trampa con cebo de octenol y el número de especies de culícidos fue cuatro veces mayor. En general, el número de mosquitos capturados por la trampa con octenol fue 14 veces mayor que el de la trampa sin octenol y el número de especies de culícidos fue 3,5 veces mayor. La trampa sin cebo de los CDC no capturó ningún Anopheles spp. durante el período de estudio. CONCLUSIONES: Los resultados demostraron que el octenol es un producto eficaz para atraer a la especie Anopheles crucians en el norte de Belice. En este país, el riesgo de malaria disminuye inmediatamente después de las tormentas (es decir, disminuye la abundancia de mosquitos; y el riesgo de contraer una infección por arbovirus, asociado con el rápido aumento de las especies de culícidos después de las tormentas, podría representar una mayor amenaza para la salud pública que la malaria (aunque se necesitaría más investigación y una vigilancia activa de las enfermedades para validar esta hipótesis.

  5. From Alma-Ata to the Global Fund: the history of international health policy De Alma-Ata ao Fundo Global: a história da política internacional de saúde

    Directory of Open Access Journals (Sweden)

    Gavino Maciocco

    2007-12-01

    Full Text Available 'Verticalization' of health care delivery, in one form or another, is the common theme pervading the history of international health policy over the last sixty years. It is often accompanied by radical policies of privatization of health services, everywhere resulting in people being forced to pay for all services. The failure of the vertical approach, of which the global public-private partnership initiatives are a modernized version, has been well recognized and its reasons are clear: actions on the distal determinants of disease (income, education, housing, the environment and infrastructure, etc are overlooked; distribution of services dedicated to specific diseases and interventions (such as AIDS, malaria, tuberculosis, etc. are artificially and temporarily reinforced, creating absurd and harmful forms of competition between services and making even more precarious and inefficient the work of already fragile basic health systems. This article describes the role played in this disturbing historical development by the prevailing economic ideology and its operational arm, the World Bank, with the view to reclaim international policy making processes and actors that really respond to people's health needs.A "verticalização" da assistência à saúde, de uma forma ou de outra, é o tema comum que permeia a história política internacional de saúde ao longo desses últimos sessenta nos, muitas vezes acompanhada com políticas radicais de privatização dos serviços de saúde, resultando, em todos os lugares, na obrigatoriedade de pagamento pelo povo, de todos os serviços. A falência da abordagem vertical, cujas iniciativas de parcerias globais público-privadas constituem sua versão moderna, tem sido reconhecida, tendo sido claras as suas razões: negligenciamento das ações sobre os determinantes distais das doenças (renda, educação, moradia, o ambiente e a infra-estrutura, etc.; a distribuição de serviços dirigidos para doenças específicas e intervenções (tal como AIDS, malária, tuberculose, etc. é artificial e temporariamente reforçada gerando maneiras perigosas e absurdas de competição entre os serviços e tornando o trabalho já frágil dos sistemas de saúde ainda mais precário e ineficiente. Esse artigo descreve o papel exercido neste desenvolvimento histórico perturbador ocasionando pela ideologia econômica predominante e seu braço operacional, o Banco Mundial, com o objetivo de reclamar que o processo de decisão política internacional e seus atores realmente respondam pelas necessidades de saúde do povo.

  6. Hacer caridad para el alma, organizarse para defender la fe. Las asociaciones católicas bogotanas (1863-1885

    Directory of Open Access Journals (Sweden)

    Sindy Paola Veloza Morales

    2014-01-01

    Full Text Available El presente artículo ahonda en el por qué, cómo y dónde de las asociaciones católicas bogotanas, en el periodo de 1863-1885, examinándolas como entidades que además de su labor religiosa y caritativa, funcionaron como espacios de participación política a partir de los cuales se generaron nuevas formas de organización y acción, así como discursos y propuestas alternativas. Concretamente el trabajo se enfoca en las sociedades de San Vicente de Paúl, Juventud Católica, Sagrado Corazón de Jesús e Hijas de María, todas estas organizaciones católicas integradas por miembros de la elite capitalina.

  7. ALMA 690 GHz OBSERVATIONS OF IRAS 16293-2422B: INFALL IN A HIGHLY OPTICALLY THICK DISK

    Energy Technology Data Exchange (ETDEWEB)

    Zapata, Luis A.; Loinard, Laurent; Rodriguez, Luis F.; Hernandez-Hernandez, Vicente [Centro de Radioastronomia y Astrofisica, UNAM, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacan (Mexico); Takahashi, Satoko; Trejo, Alfonso [Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 10617, Taiwan (China); Parise, Berengere [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany)

    2013-02-10

    We present sensitive, high angular resolution ({approx}0.''2) submillimeter continuum and line observations of IRAS 16293-2422B made with the Atacama Large Millimeter/Submillimeter Array. The 0.45 mm continuum observations reveal a single and very compact source associated with IRAS 16293-2422B. This submillimeter source has a deconvolved angular size of about 400 mas (50 AU) and does not show any inner structure inside of this diameter. The H{sup 13}CN, HC{sup 15}N, and CH{sub 3}OH line emission regions are about twice as large as the continuum emission and reveal a pronounced inner depression or ''hole'' with a size comparable to that estimated for the submillimeter continuum. We suggest that the presence of this inner depression and the fact that we do not see an inner structure (or a flat structure) in the continuum are produced by very optically thick dust located in the innermost parts of IRAS 16293-2422B. All three lines also show pronounced inverse P-Cygni profiles with infall and dispersion velocities larger than those recently reported from observations at lower frequencies, suggesting that we are detecting faster and more turbulent gas located closer to the central object. Finally, we report a small east-west velocity gradient in IRAS 16293-2422B that suggests that its disk plane is likely located very close to the plane of the sky.

  8. Public participation as a mechanism for promoting sustainable waste management service delivery in Sedibeng District Municipality / Nompazamo Alma Ludidi

    OpenAIRE

    Ludidi, Nompazamo Alma

    2013-01-01

    The purpose of this research is to determine the extent of public participation in waste management, willingness of the community to assist the municipality in waste management and how the officials involve the community as partners in waste management. Waste management has become a big environmental challenge in Sedibeng District Municipality due to rural- urban drift leading to population increase in the region. In cities and towns where there is population increase there is excessive gener...

  9. Corinna von List, Résistantes, traduit de l’allemand par Solveig Kahnt, Paris, Alma Editeur, 2012, 376 p.

    Directory of Open Access Journals (Sweden)

    Isabelle Ernot

    2012-06-01

    Full Text Available L’ouvrage, paru en Allemagne en 2010 sous le titre, Frauen in der Resistance, 1940-1944, est issu d’une thèse soutenue à l’Université de Potsdam. La recherche, qui ne concerne que la résistance féminine sur le territoire français, portée aussi bien par des Françaises que par des étrangères, a été récompensée en 2006 par le prix Guillaume Fichet - Octave Simon. L’auteure part du constat que « les missions que les femmes ont accomplies dans la Résistance n’ont été reconnues que lorsqu’elles cad...

  10. On the detection of high-redshift black holes with ALMA through CO and H(2) emission

    NARCIS (Netherlands)

    Spaans, Marco; Meijerink, Rowin

    2008-01-01

    Many present-day galaxies are known to harbor supermassive, >= 10(6) M(circle dot), black holes. These central black holes must have grown through accretion from less massive seeds in the early universe. The molecules CO and H 2 can be used to trace this young population of accreting massive black

  11. MÁQUINAS CON ALMA. LO TÉCNICO Y LO HUMANO EN SIMONDON Y EN LA CULTURA DEL ANIME.

    Directory of Open Access Journals (Sweden)

    Alba Gonzalez Torrents

    2013-06-01

    Full Text Available En el imaginario del anime contemporáneo de ciencia ficción encontramos algunos ejemplos claros de una reinterpretación de la relación entre ser humano y tecnología  en términos no-clásicos. La filosofía de la individuación de Gilbert Simondon, con su crítica radical al individualismo y al sustancialismo, y en especial su filosofía de la técnica, centrada en la denuncia del olvido cultural de los aspectos humanos de la técnica, ofrecen una clave filosófica idónea para la exploración de ese imaginario. Mediante la aplicación de los conceptos desarrollados por Simondon en sus análisis del modo de existencia de los objetos técnico a los animes Akira, Evangelion, Ghost in The Shell y Serial Experiments Lain, muestro que existe en ellos una visión coherente e innovadora de la relación entre humanidad y técnica, que coincide en muchos aspectos con las críticas y propuestas elaboradas por el mismo Simondon. Los más importantes de estos aspectos se relacionan con la idea de la extensión tecnológica de lo humano y con los grados de integración o separación existentes entre el dominio de lo técnico y el de la espiritualidad y la religión.

  12. Constraining the nature of two Lyα emitters detected by ALMA at z = 4.7

    Science.gov (United States)

    Williams, R. J.; Wagg, J.; Maiolino, R.; Foster, C.; Aravena, M.; Wiklind, T.; Carilli, C. L.; McMahon, R. G.; Riechers, D.; Walter, F.

    2014-04-01

    We report optical spectroscopy from the Very Large Telescope/FOcal Reducer and low dispersion spectroscopy of the two Lyα emitters (LAEs) companions to the quasi-stellar object-sub-millimetre galaxy system BRI1202-0725 at z = 4.7, which have recently been detected in the [C II]158 μm line by the Atacama Large Millimetre/Sub-millimetre Array. We detect Lyα emission from both sources and so confirm that these LAE candidates are physically associated with the BRI1202-0725 system. We also report the lack of detection of any high-ionization emission lines (N V λ1240, Si IV λ1396, C IV λ1549 and He II λ1640) and find that these systems are likely not photoionized by the quasar, leaving in situ star formation as the main powering source of these LAEs. We also find that both LAEs have Lyα emission much broader (˜1300 km s-1) than the [C II] emission and broader than most LAEs. In addition, both LAEs have roughly symmetric Lyα profiles implying that both systems are within the H II sphere produced by the quasar. This is the first time that the proximity zone of a quasar is probed by exploiting nearby LAEs. We discuss the observational properties of these galaxies in the context of recent galaxy formation models.

  13. Pipeline welding with Flux Cored and Metal Cored Wire; Soldagem de dutos com processos Arame Tubular e de Alma Metalica

    Energy Technology Data Exchange (ETDEWEB)

    Costa, Ubirajara Pereira da [ITW Soldagem Brasil Miller-Hobart, Sao Paulo, SP (Brazil)

    2003-07-01

    Different welding process like SMAW, Semi-Automatic FCAW Gas-shielded and Self-shielded and Mechanized GMAW-MAG with Solid Wire are suggested to weld Transmission Pipelines. Presently, the largest extensions of Transmission Pipelines under construction, are in China like Lines West-East, Zong-Wu, Shan-Jing Fuxian and some others, totalizing about 8.000 km, and all using Semi-Automatic Self Shielded Flux Cored Arc Welding Process. Also, several papers and magazines that covers Transmission Pipelines Welding, not frequently mention Operational aspects of the process and some other variables like environment and site geography. This presentation intends to cover some of the Operational aspects of the Flux Cored Arc Welding and GMAW-Metal Cored in order to give sufficient information for Construction, Engineering, Projects e Contractors so they can evaluate these Process against the SMAW or even Mechanized Systems, considering the Operation Factor, Efficiency and Deposition Rate. We will not cover operational details of the GMAW Mechanized Systems but only suggest that be evaluated the possibility to replace the GMAW-Solid Wire by the GMAW-Metal Cored Wire. (author)

  14. ALMA MEASUREMENTS OF THE HNC AND HC{sub 3}N DISTRIBUTIONS IN TITAN'S ATMOSPHERE

    Energy Technology Data Exchange (ETDEWEB)

    Cordiner, M. A.; Nixon, C. A.; Serigano, J.; Charnley, S. B.; Milam, S. N.; Mumma, M. J.; Villanueva, G.; Paganini, L. [NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States); Teanby, N. A. [School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen' s Road, Bristol BS8 1RJ (United Kingdom); Irwin, P. G. J. [Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, University of Oxford, Parks Road, Oxford OX1 3PU (United Kingdom); Lis, D. C. [Sorbonne Universités, Université Pierre et Marie Curie, Paris 6, CNRS, Observatoire de Paris, UMR 8112, LERMA, F-75014 Paris (France); Kuan, Y.-J. [National Taiwan Normal University, Taipei 116, Taiwan, ROC (China); Remijan, A. J., E-mail: martin.cordiner@nasa.gov [National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States)

    2014-11-10

    We present spectrally and spatially resolved maps of HNC and HC{sub 3}N emission from Titan's atmosphere, obtained using the Atacama Large Millimeter/submillimeter Array on 2013 November 17. These maps show anisotropic spatial distributions for both molecules, with resolved emission peaks in Titan's northern and southern hemispheres. The HC{sub 3}N maps indicate enhanced concentrations of this molecule over the poles, consistent with previous studies of Titan's photochemistry and atmospheric circulation. Differences between the spectrally integrated flux distributions of HNC and HC{sub 3}N show that these species are not co-spatial. The observed spectral line shapes are consistent with HNC being concentrated predominantly in the mesosphere and above (at altitudes z ≳ 400 km), whereas HC{sub 3}N is abundant at a broader range of altitudes (z ≈ 70-600 km). From spatial variations in the HC{sub 3}N line profile, the locations of the HC{sub 3}N emission peaks are shown to be variable as a function of altitude. The peaks in the integrated emission from HNC and the line core (upper atmosphere) component of HC{sub 3}N (at z ≳ 300 km) are found to be asymmetric with respect to Titan's polar axis, indicating that the mesosphere may be more longitudinally variable than previously thought. The spatially integrated HNC and HC{sub 3}N spectra are modeled using the NEMESIS planetary atmosphere code and the resulting best-fitting disk-averaged vertical mixing ratio profiles are found to be in reasonable agreement with previous measurements for these species. Vertical column densities of the best-fitting gradient models for HNC and HC{sub 3}N are 1.9 × 10{sup 13} cm{sup –2} and 2.3 × 10{sup 14} cm{sup –2}, respectively.

  15. Retreat from Alma Ata? The WHO's report on Task Shifting to community health workers for AIDS care in poor countries.

    Science.gov (United States)

    Campbell, C; Scott, K

    2011-01-01

    This paper examines the potential of community health worker (CHW) programmes, as proposed by the 2008 World Health Organisation (WHO) document Task Shifting to tackle health worker shortages, to contribute to HIV/AIDS prevention and treatment and various Millennium Development Goals in low-income countries. It examines the WHO proposal through a literature review of factors that have facilitated the success of previous CHW experiences. The WHO has taken account of five key lessons learnt from past CHW programmes (the need for strong management, appropriate selection, suitable training, adequate retention structures and good relationships with other healthcare workers). It has, however, neglected to emphasise the importance of a sixth lesson, the 'community embeddedness' of CHWs, found to be of critical importance to the success of past CHW programmes. We have no doubt that the WHO plans will increase the number of workers able to perform medically oriented tasks. However, we argue that without community embeddedness, CHWs will be unable to successfully perform the socially oriented tasks assigned to them by the WHO, such as health education and counselling. We locate the WHO's neglect of community embeddedness within the context of a broader global public health trend away from community-focused primary healthcare towards biomedically focused selective healthcare.

  16. De corpo e alma na margem: catolicismo, santidade e medicina no Norte de Portugal (c. 1900 - c. 1950

    Directory of Open Access Journals (Sweden)

    Tiago Pires Marques

    Full Text Available Num primeiro olhar, a personalidade religiosa da beata Alexandrina Maria da Costa surge como estranha e desconcertante. Este artigo propõe um exercício de compreensão histórica e antropológica que reduz essa estranheza. Sustenta-se que este caso reflete a história de uma comunidade com uma identidade religiosa forte, onde um catolicismo devocional convivia com investidas clericais visando promover uma subjetividade espiritual. Ao mesmo tempo, a medicina e a psiquiatria forneceram novas grelhas de interpretação da experiência religiosa. Este conjunto heterogêneo de elementos formou uma mística vernacular que atribuiu novos significados às entidades liminais próprias do universo religioso do Norte de Portugal. A linguagem da mística vernacular construiu a interioridade de uma experiência que, em sua singularidade, foi sempre fortemente socializada.

  17. Psicodinâmica das relações incestuosas: assassinato e renascimento da alma em Preciosa

    Directory of Open Access Journals (Sweden)

    Tales Vilela Santeiro

    2014-03-01

    Full Text Available A linguagem dos filmes é vigorosa em facilitar processos formativos na clínica de orientação psicanalítica, pois metaforiza situações e contextos humanos, inclusive relações familiares incestuosas (RFIs. O trabalho teve como objetivo discutir um caso fílmico que focaliza RFsI encenadas por um casal parental e por uma filha. Preciosa: uma história de esperança, filme estadunidense dirigido e produzido por Lee Daniels em 2009, foi analisado qualitativamente por meio de teorias e discussões clínicas sobre a psicodinâmica familiar. A família de Preciosa é entendida de modo integrado, havendo mutualidade de influências entre seus diferentes membros, que se relacionam conforme os limites e potencialidades impostos pelo desenvolvimento psicossexual de cada um deles. Todos os envolvidos nas RFIs precisam enfrentar a tarefa de elaborar segredos familiares, os quais são transmitidos por via inconsciente de geração a geração. Preciosa ilustra a importância das funções familiares para a constituição das subjetividades e retrata desafios contemporâneos que se apresentam ao trabalho do clínico.

  18. Plotino y la potencia desasosegada del Alma: ¿dispersión o contemplación?

    Directory of Open Access Journals (Sweden)

    Fernando Martín

    2015-06-01

    Full Text Available El presente trabajo intenta recuperar la noción de contemplación inherente a la naturaleza, potencia generativa de la tercera hipóstasis del sistema filosófico de Plotino. En vista de este propósito, se tomará como materia de investigación dos tratados del corpus eneádico, a saber III 7 y III 8, cuyas líneas brindan aportes significativos a fin de reflexionar sobre la pregunta inicial de esta exposición: si la naturaleza, en la doctrina de Plotino, implica sólo ideas tales como la dispersión y la multiplicidad o bien sugiere otras categorías. Para ello, se seguirá un estudio analítico y descriptivo, acompañado de una lectura a la vez hermenéutica y crítica de las fuentes y también de la bibliografía secundaria.

  19. ALMA 690 GHz OBSERVATIONS OF IRAS 16293–2422B: INFALL IN A HIGHLY OPTICALLY THICK DISK

    International Nuclear Information System (INIS)

    Zapata, Luis A.; Loinard, Laurent; Rodríguez, Luis F.; Hernández-Hernández, Vicente; Takahashi, Satoko; Trejo, Alfonso; Parise, Bérengère

    2013-01-01

    We present sensitive, high angular resolution (∼0.''2) submillimeter continuum and line observations of IRAS 16293–2422B made with the Atacama Large Millimeter/Submillimeter Array. The 0.45 mm continuum observations reveal a single and very compact source associated with IRAS 16293–2422B. This submillimeter source has a deconvolved angular size of about 400 mas (50 AU) and does not show any inner structure inside of this diameter. The H 13 CN, HC 15 N, and CH 3 OH line emission regions are about twice as large as the continuum emission and reveal a pronounced inner depression or ''hole'' with a size comparable to that estimated for the submillimeter continuum. We suggest that the presence of this inner depression and the fact that we do not see an inner structure (or a flat structure) in the continuum are produced by very optically thick dust located in the innermost parts of IRAS 16293–2422B. All three lines also show pronounced inverse P-Cygni profiles with infall and dispersion velocities larger than those recently reported from observations at lower frequencies, suggesting that we are detecting faster and more turbulent gas located closer to the central object. Finally, we report a small east-west velocity gradient in IRAS 16293–2422B that suggests that its disk plane is likely located very close to the plane of the sky.

  20. Pedaços de alma: emoções e gênero nos discursos da resistência

    Directory of Open Access Journals (Sweden)

    Cristina Scheibe Wolff

    2015-11-01

    Full Text Available Neste trabalho analiso diversos materiais produzidos por grupos de familiares de presos e desaparecidos políticos, e outras organizações de resistência aos regimes militares dos países do Cone Sul, buscando mostrar como as emoções e o gênero se entrelaçam em uma retórica que apela para os sentimentos da opinião pública com objetivos políticos. As organizações e associações, em muitos de seus materiais, agenciavam o gênero de forma a atingir o público em seus sentimentos, construindo uma retórica que se aproxima e encampa a questão dos direitos humanos, de forma a combater, por um lado, a tortura e o extermínio de militantes políticos e, de outro, ajudar a desacreditar e enfraquecer os regimes militares, tendo auxiliado na sua queda ao longo dos anos 1980 em todo o Cone Sul.

  1. Quiescent Prominences in the Era of ALMA: Simulated Observations Using the 3D Whole-prominence Fine Structure Model

    Czech Academy of Sciences Publication Activity Database

    Gunár, Stanislav; Heinzel, Petr; Mackay, D. H.; Anzer, U.

    2016-01-01

    Roč. 833, č. 2 (2016), 141/1-141/11 ISSN 0004-637X R&D Projects: GA ČR(CZ) GA16-17586S EU Projects: European Commission(XE) 328138 - COMBINED MHD AND RT Institutional support: RVO:67985815 Keywords : numerical methods * radiative transfer * filaments Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics Impact factor: 5.533, year: 2016

  2. Producción del libro fotográfico "Retratos Asilo Cristo Rey" una sonrisa para el alma

    OpenAIRE

    Mora Campoverde, Andrea Paulina

    2018-01-01

    El contenido de esta obra guarda muchas memorias; la investigación de tipo exploratorio ha permitido reconocer la belleza espiritual y física que aún conservan los ancianos, a pesar de los años y su experiencia en vivir. Los invito a que disfruten de la lectura y de las imágenes fotográficas captadas, pero sobre todo de las historias de vida, tanto como lo hice yo. The content of this work keeps a lot of memories; the exploratory investigation has allowed to recognize the spiritual and phy...

  3. The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] Line and Dust Emission in 6

    Science.gov (United States)

    Aravena, M.; Decarli, R.; Walter, F.; Bouwens, R.; Oesch, P. A.; Carilli, C. L.; Bauer, F. E.; Da Cunha, E.; Daddi, E.; Gónzalez-López, J.; Ivison, R. J.; Riechers, D. A.; Smail, I.; Swinbank, A. M.; Weiss, A.; Anguita, T.; Bacon, R.; Bell, E.; Bertoldi, F.; Cortes, P.; Cox, P.; Hodge, J.; Ibar, E.; Inami, H.; Infante, L.; Karim, A.; Magnelli, B.; Ota, K.; Popping, G.; van der Werf, P.; Wagg, J.; Fudamoto, Y.

    2016-12-01

    We present a search for [C II] line and dust continuum emission from optical dropout galaxies at z > 6 using ASPECS, our Atacama Large Millimeter submillimeter Array Spectroscopic Survey in the Hubble Ultra-deep Field (UDF). Our observations, which cover the frequency range of 212-272 GHz, encompass approximately the range of 6 4.5σ, two of which correspond to blind detections with no optical counterparts. At this significance level, our statistical analysis shows that about 60% of our candidates are expected to be spurious. For one of our blindly selected [C II] line candidates, we tentatively detect the CO(6-5) line in our parallel 3 mm line scan. None of the line candidates are individually detected in the 1.2 mm continuum. A stack of all [C II] candidates results in a tentative detection with S 1.2 mm = 14 ± 5 μJy. This implies a dust-obscured star-formation rate (SFR) of (3 ± 1) M ⊙ yr-1. We find that the two highest-SFR objects have candidate [C II] lines with luminosities that are consistent with the low-redshift L [C II] versus SFR relation. The other candidates have significantly higher [C II] luminosities than expected from their UV-based SFR. At the current sensitivity, it is unclear whether the majority of these sources are intrinsically bright [C II] emitters, or spurious sources. If only one of our line candidates was real (a scenario greatly favored by our statistical analysis), we find a source density for [C II] emitters at 6 universe.

  4. ALMA Reveals Molecular Cloud N55 in the Large Magellanic Cloud as a Site of Massive Star Formation

    Science.gov (United States)

    Naslim, N.; Tokuda, K.; Onishi, T.; Kemper, F.; Wong, T.; Morata, O.; Takada, S.; Harada, R.; Kawamura, A.; Saigo, K.; Indebetouw, R.; Madden, S. C.; Hony, S.; Meixner, M.

    2018-02-01

    We present the molecular cloud properties of N55 in the Large Magellanic Cloud using 12CO(1–0) and 13CO(1–0) observations obtained with Atacama Large Millimeter Array. We have done a detailed study of molecular gas properties, to understand how the cloud properties of N55 differ from Galactic clouds. Most CO emission appears clumpy in N55, and molecular cores that have young stellar objects (YSOs) show larger linewidths and masses. The massive clumps are associated with high and intermediate mass YSOs. The clump masses are determined by local thermodynamic equilibrium and virial analysis of the 12CO and 13CO emissions. These mass estimates lead to the conclusion that (a) the clumps are in self-gravitational virial equilibrium, and (b) the 12CO(1–0)-to-H2 conversion factor, {X}{CO}, is 6.5 × 1020 cm‑2 (K km s‑1)‑1. This CO-to-H2 conversion factor for N55 clumps is measured at a spatial scale of ∼0.67 pc, which is about two times higher than the {X}{CO} value of the Orion cloud at a similar spatial scale. The core mass function of N55 clearly show a turnover below 200 {M}ȯ , separating the low-mass end from the high-mass end. The low-mass end of the 12CO mass spectrum is fitted with a power law of index 0.5 ± 0.1, while for 13CO it is fitted with a power law index 0.6 ± 0.2. In the high-mass end, the core mass spectrum is fitted with a power index of 2.0 ± 0.3 for 12CO, and with 2.5 ± 0.4 for 13CO. This power law behavior of the core mass function in N55 is consistent with many Galactic clouds.

  5. Molecular line emission in NGC 1068 imaged with ALMA : I. An AGN-driven outflow in the dense molecular gas

    NARCIS (Netherlands)

    García-Burillo, S.; Combes, F.; Usero, A.; Aalto, S.; Krips, M.; Viti, S.; Alonso-Herrero, A.; Hunt, L. K.; Schinnerer, E.; Baker, A. J.; Boone, F.; Casasola, V.; Colina, L.; Costagliola, F.; Eckart, A.; Fuente, A.; Henkel, C.; Labiano, A.; Martín, S.; Márquez, I.; Muller, S.; Planesas, P.; Ramos Almeida, C.; Spaans, M.; Tacconi, L. J.; van der Werf, P. P.

    Aims: We investigate the fueling and the feedback of star formation and nuclear activity in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy, by analyzing the distribution and kinematics of the molecular gas in the disk. We aim to understand if and how gas accretion can self-regulate.

  6. ALMA Cycle 1 Observations of the HH46/47 Molecular Outflow: Structure, Entrainment, and Core Impact

    Science.gov (United States)

    Zhang, Yichen; Arce, Héctor G.; Mardones, Diego; Cabrit, Sylvie; Dunham, Michael M.; Garay, Guido; Noriega-Crespo, Alberto; Offner, Stella S. R.; Raga, Alejandro C.; Corder, Stuartt A.

    2016-12-01

    We present Atacama Large Millimeter/sub-millimeter Array Cycle 1 observations of the HH 46/47 molecular outflow using combined 12 m array and Atacama Compact Array observations. The improved angular resolution and sensitivity of our multi-line maps reveal structures that help us study the entrainment process in much more detail and allow us to obtain more precise estimates of outflow properties than in previous observations. We use {}13{{CO}} (1-0) and {{{C}}}18{{O}} (1-0) emission to correct for the {}12{{CO}} (1-0) optical depth to accurately estimate the outflow mass, momentum, and kinetic energy. This correction increases the estimates of the mass, momentum, and kinetic energy by factors of about 9, 5, and 2, respectively, with respect to estimates assuming optically thin emission. The new {}13{{CO}} and {{{C}}}18{{O}} data also allow us to trace denser and slower outflow material than that traced by the {}12{{CO}} maps, and they reveal an outflow cavity wall at very low velocities (as low as 0.2 {\\text{km s}}-1 with respect to the core’s central velocity). Adding the slower material traced only by {}13{{CO}} and {{{C}}}18{{O}}, there is another factor of three increase in the mass estimate and 50% increase in the momentum estimate. The estimated outflow properties indicate that the outflow is capable of dispersing the parent core within the typical lifetime of the embedded phase of a low-mass protostar and that it is responsible for a core-to-star efficiency of 1/4 to 1/3. We find that the outflow cavity wall is composed of multiple shells associated with a series of jet bow-shock events. Within about 3000 au of the protostar the {}13{{CO}} and {{{C}}}18{{O}} emission trace a circumstellar envelope with both rotation and infall motions, which we compare with a simple analytic model. The CS (2-1) emission reveals tentative evidence of a slowly moving rotating outflow, which we suggest is entrained not only poloidally but also toroidally by a disk wind that is launched from relatively large radii from the source.

  7. ALMA observations of cold molecular gas in AGN hosts at z ˜ 1.5 - evidence of AGN feedback?

    Science.gov (United States)

    Kakkad, D.; Mainieri, V.; Brusa, M.; Padovani, P.; Carniani, S.; Feruglio, C.; Sargent, M.; Husemann, B.; Bongiorno, A.; Bonzini, M.; Piconcelli, E.; Silverman, J. D.; Rujopakarn, W.

    2017-07-01

    Similarly to the cosmic star formation history, the black hole accretion rate density of the Universe peaked at 1 99 per cent probability of lower depletion time-scales and lower molecular gas fractions in AGN hosts with respect to the non-AGN comparison sample. We discuss the implications of these observations on the impact that AGN feedback may have on star formation efficiency of z >1 galaxies.

  8. Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): Fast-Scan Single-Dish Mapping

    Czech Academy of Sciences Publication Activity Database

    White, S.M.; Iwai, N.; Phillips, N.; Hills, R.E.; Hirota, A.; Yagoubov, P.; Siringo, G.; Shimojo, M.; Bastian, T.S.; Hales, A.S.; Sawada, T.; Asayama, S.; Sugimoto, M.; Marson, R.; Kawasaki, W.; Muller, E.; Nakazato, T.; Sugimoto, K.; Brajsa, R.; Skokić, Ivica; Bárta, Miroslav; Kim, S.; Remijan, A.; de Gregorio, I.; Corder, S.; Hudson, H. S.; Loukitcheva, M.; Chen, B.; de Pontieu, B.; Fleishmann, G. D.; Gary, D. E.; Kobelski, A.; Wedemeyer, S.; Yan, Y.

    2017-01-01

    Roč. 292, č. 7 (2017), 88/1-88/28 ISSN 0038-0938 R&D Projects: GA MŠk(CZ) LM2015067 Institutional support: RVO:67985815 Keywords : millimeter wavelengths * solar atmosphere * radiometric standard Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics OBOR OECD: Astronomy (including astrophysics,space science) Impact factor: 2.682, year: 2016

  9. ALMA Shows that Gas Reservoirs of Star-forming Disks over the Past 3 Billion Years Are Not Predominantly Molecular

    Energy Technology Data Exchange (ETDEWEB)

    Cortese, Luca; Catinella, Barbara; Janowiecki, Steven, E-mail: luca.cortese@uwa.edu.au [International Centre for Radio Astronomy Research, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009 (Australia)

    2017-10-10

    Cold hydrogen gas is the raw fuel for star formation in galaxies, and its partition into atomic and molecular phases is a key quantity for galaxy evolution. In this Letter, we combine Atacama Large Millimeter/submillimeter Array and Arecibo single-dish observations to estimate the molecular-to-atomic hydrogen mass ratio for massive star-forming galaxies at z ∼ 0.2 extracted from the HIGHz survey, i.e., some of the most massive gas-rich systems currently known. We show that the balance between atomic and molecular hydrogen in these galaxies is similar to that of local main-sequence disks, implying that atomic hydrogen has been dominating the cold gas mass budget of star-forming galaxies for at least the past three billion years. In addition, despite harboring gas reservoirs that are more typical of objects at the cosmic noon, HIGHz galaxies host regular rotating disks with low gas velocity dispersions suggesting that high total gas fractions do not necessarily drive high turbulence in the interstellar medium.

  10. Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): High-Resolution Interferometric Imaging

    Czech Academy of Sciences Publication Activity Database

    Shimojo, M.; Bastian, T.S.; Hales, A.S.; White, S. M.; Iwai, N.; Hills, R.E.; Hirota, A.; Phillips, N.; Sawada, T.; Yagoubov, P.; Siringo, G.; Asayama, S.; Sugimoto, M.; Brajša, R.; Skokić, Ivica; Bárta, Miroslav; Kim, S.; De Gregorio-Monsalvo, I.; Corder, S.; Hudson, H. S.; Wedemeyer, S.; Gary, D. E.; de Pontieu, B.; Loukitcheva, M.; Fleishman, G.; Chen, B.; Kobelski, A.; Yan, Y.

    2017-01-01

    Roč. 292, č. 7 (2017), 87/1-87/28 ISSN 0038-0938 R&D Projects: GA MŠk(CZ) 7E13003; GA MŠk(CZ) LM2015067 EU Projects: European Commission(XE) 312495 - SOLARNET Grant - others:European Commission - EC(XE) 682462 Institutional support: RVO:67985815 Keywords : compact array * correlator * field Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics OBOR OECD: Astronomy (including astrophysics,space science) Impact factor: 2.682, year: 2016

  11. Schibsted heidab Bonnierile kinda / Sirje Rank

    Index Scriptorium Estoniae

    Rank, Sirje, 1966-

    2004-01-01

    Norra meediakontsern Schibsted tegi ostupakkumise Soome suuruselt teisele meediakontsernile Alma Media, mille suurim aktsionär on Rootsi Bonnieri kontsern. Diagrammid: Alma Media käive ja kasum. Skeem: Alma Media Oyj. Kommenteerib Mart Kadastik

  12. Diseño y Análisis de desempeño de un inversor de voltaje utilizando controladores inteligentes

    Directory of Open Access Journals (Sweden)

    Juan jose Salazar

    2013-11-01

    Full Text Available El presente documento describe el desarrollo de controladores inteligentes, para la supresión de armónicos en inversores monofásicos con modulación senoidal por ancho de pulso (SPWM. En la primera fase se diseño un controlador PI que sirve como modelo de referencia para la obtención de los patrones de entrenamiento de la red neuronal. Posteriormente se diseño un controlador PD lógico difuso utilizando una base de 25 reglas. Las simulaciones realizadas con el mkodelo matemático del inversor y utilizando "SimPowerSystems" de MATLAB indican que es posible obtener una onda senoidal pura con un mínimo de distorsión armónica total (THD mediante el uso de los controladores inteligentes propuestos.

  13. Susceptibilidade larval de populações de Aedes aegypti e Culex quinquefasciatus a inseticidas químicos

    OpenAIRE

    Campos Jairo; Andrade Carlos F S

    2003-01-01

    OBJETIVO: Avaliar a susceptibilidade a inseticidas químicos de larvas de Culex quinquefasciatus e Aedes aegypti, provenientes de áreas sujeitas ou não a tratamentos de controle. MÉTODOS: Foram coletadas larvas de mosquitos em uma área não sujeita a tratamentos com inseticidas (Campinas, SP) e em áreas sujeitas a esses tratamentos (Campo Grande, MS e Cuiabá, MT). Foram usados bioensaios com concentrações diagnóstico e concentrações múltipla de inseticidas organofosforados e piretróides, segund...

  14. Uma nova subespécie de Parides bunichus (Hübner (Lepidoptera, Papilionidae, Troidini do interior da Bahia, Brasil A new subspecis of Parides bunichus (Hübner (Lepidoptera, Papilionidae, Troidini from the interior of Bahia, Brazil

    Directory of Open Access Journals (Sweden)

    Mirna M. Casagrande

    2007-09-01

    Full Text Available Parides bunichus almas ssp.nov. é descrita com base em material coletado no Pico das Almas, Rio de Contas, Bahia, Brasil.Parides bunichus almas ssp.nov. is described from Pico das Almas, Rio de Contas, Bahia, Brazil.

  15. A organização da alma: Elias e Foucault sobre a disciplina e o eu, de Robert Van Krieken

    Directory of Open Access Journals (Sweden)

    Anamaria Cristina Schindler

    1996-11-01

    Full Text Available O autor aborda o debate recente sobre o conceito de disciplina, a partir das obras de Foucault e Elias. Remete-as à noção weberiana de "gaiola de ferro", ressaltando o desenvolvimento que ambos fizeram em direção ao processo de disciplinarização dos indivíduos. É comum aos três pensadores a visão de uma tendência crescente à autodisciplina nas sociedades cada vez mais racionalizadas, mas há distinções de ênfase. Enquanto para Weber o mais importante são as mudanças sociais e políticas, Elias enfatiza as mudanças nas interdependências humanas e na estrutura da conduta, e Foucault insiste na capacidade do poder disciplinar em "libertar" a energia psíquica e libidinal de modo a aproximá-las dos interesses da economia capitalista. O artigo continua abordando as distintas visões dos autores em relação à Idade Média e do "processo civilizatório". Ao Final, levanta questões que deixaram de ser respondidas pelos três

  16. ALMA [N ii] 205 μ m Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7

    International Nuclear Information System (INIS)

    Lu, Nanyao; Xu, C. Kevin; Zhu, Lei; Zhao, Yinghe; Díaz-Santos, Tanio; Charmandaris, Vassilis; Gao, Yu; Van der Werf, Paul P.; Privon, George C.; Inami, Hanae; Rigopoulou, Dimitra; Sanders, David B.

    2017-01-01

    We present the results from Atacama Large Millimeter/submillimeter Array imaging in the [N ii] 205 μ m fine-structure line (hereafter [N ii]) and the underlying continuum of BRI 1202-0725, an interacting galaxy system at z = 4.7, consisting of a quasi-stellar object (QSO), a submillimeter galaxy (SMG), and two Ly α emitters, all within ∼25 kpc of the QSO. We detect the QSO and SMG in both [N ii] and continuum. At the ∼1″ (or 6.6 kpc) resolution, both the QSO and SMG are resolved in [N ii], with the de-convolved major axes of ∼9 and ∼14 kpc, respectively. In contrast, their continuum emissions are much more compact and unresolved even at an enhanced resolution of ∼0.″7. The ratio of the [N ii] flux to the existing CO(7−6) flux is used to constrain the dust temperature ( T dust ) for a more accurate determination of the FIR luminosity L FIR . Our best estimated T dust equals 43 (±2) K for both galaxies (assuming an emissivity index β = 1.8). The resulting L CO(7−6) / L FIR ratios are statistically consistent with that of local luminous infrared galaxies, confirming that L CO(7−6) traces the star formation (SF) rate (SFR) in these galaxies. We estimate that the ongoing SF of the QSO (SMG) has an SFR of 5.1 (6.9) × 10 3 M ⊙ yr −1 (±30%) assuming Chabrier initial mass function, takes place within a diameter (at half maximum) of 1.3 (1.5) kpc, and will consume the existing 5 (5) × 10 11 M ⊙ of molecular gas in 10 (7) × 10 7 years.

  17. [Review of: J. Hilton, A. Gosling Alma parens originalis? The receptions of classical literature and thought in Africa, Europe, the United States, and Cuba

    NARCIS (Netherlands)

    van Weyenberg, A.

    2009-01-01

    This collection of articles derives in part from the papers presented at the 26th biennial conference of the Classical Association of South Africa held at Durban and Pietermaritzburg in 2005. John Hilton explains in the introduction that the conference's theme, 'The Classical Tradition / Classical

  18. Cuerpos místicos, almas ascéticas. Regulaciones del espíritu en la experiencia de Teresa de Ávila (1515-1582.

    Directory of Open Access Journals (Sweden)

    Mònica Balltondre

    2009-11-01

    Full Text Available En esta tesis se investiga la antropología que subyace a la espiritualidad mística femenina de mediados del siglo XVI castellano, de la mano de Teresa de Ávila, conocida como Teresa de Jesús. Ella construyó una forma espiritual de vivirse que le permitió encuadrar sus experiencias a partir de tradiciones teológicas, como la mística, y de otros saberes como la filosofía natural y la medicina de su tiempo. Se examinan para ver cómo conceptualizó sus relaciones sobrenaturales y qué le aportaron en la construcción de sí misma. Por ejemplo, analizo sus propuestas de oración y meditación para entender la construcción psíquica que había detrás; los significados teológicos que atribuyó a las enfermedades de su cuerpo; su uso del dolor, etc. Además, exploro cómo funcionó su programa espiritual en sus fundaciones. Al revisar las implicaciones que estos discursos espirituales tuvieron en la forma de determinar procesos vivenciales, dentro de su producción histórica, damos cuenta de algunas de las categorías y prácticas que configuraron un cierto sujeto moderno.

  19. Para gozar a esta mujer diera el alma. El mito fáustico y sus rescrituras en la literatura española

    Directory of Open Access Journals (Sweden)

    Hernández, Isabel

    2011-12-01

    Full Text Available This article aims to explore the reception of the figure of Faust in Spanish literature based on the Volksbuch as well as on Goethe’s later drama version, considering those moments in time, in particular, when this literary myth was the object of greater attention, and highlighting the possible reasons which could have produced its reception.El presente artículo trata de indagar en la recepción del personaje de Fausto en las letras españolas a partir del libro popular alemán, así como de de la posterior versión teatral realizada por Goethe, haciendo un especial hincapié en las épocas en que este mito literario ha despertado una mayor atención e incidiendo en los motivos que pudieron provocar su recepción.

  20. Lietuvos bibliotekininkụ draugija : Tarptautinis Baltijos šaliụ bibliotekininkụ kongresas CoBaL10 / Simona Žilienė, Alma Masevičienė

    Index Scriptorium Estoniae

    Žilienė, Simona

    2015-01-01

    Riia Läti Rahvusraamatukogus 12.-13. oktoobril 2015 toimunud Balti raamatukoguhoidjate 10. kongressist „Libraries in communities", kus osalesid ka Eesti Rahvusraamatukogu peadirektor Janne Andresoo ja Eesti Raamatukoguhoidjate Ühingu juhatuse esinaine Katre Riisalu

  1. Actitud clínica ante la dislipemia en pacientes con elevado riesgo cardiovascular en España. Estudio ALMA

    Directory of Open Access Journals (Sweden)

    Xavier Pintó

    2018-01-01

    Conclusiones: Aunque el cálculo del RCV se acepta de forma general, existe disparidad en los objetivos del cLDL. Los MAE consideran unos objetivos más ambiciosos y la asociación de fármacos hipolipemiantes con más frecuencia que los MAP.

  2. OBJETOS RELACIONAIS AMERÍNDIOS: SOBRE A (INVISIBILIDADE DA ARTE KADIWÉU NA NOVELA ALMA GÊMEA DA REDE GLOBO

    Directory of Open Access Journals (Sweden)

    LISIANE KOLLER LECZNIESKI

    2010-06-01

    Full Text Available RESUMO: Este texto é uma reflexão sobre o papel da cerâmica na vida social dos índios Kadiwéu que vivem na aldeia Bodoquena, situada no Pantanal sul-matogrossense, Brasil. A partir de exemplos etnográficos analiso as relações entre o mundo das artes e o mundo social, argumentando que a cerâmica atua como um eixo central em torno do qual os Kadiwéu tem articulado e dinamizado suas relações com o mundo externo, especialmente o “mundo dos brancos”. Esta compreensão marcadamente relacional dos objetos também aponta, de forma reflexiva, para aspectos cruciais da dinâmica ocidental em torno dos objetos, lançando um olhar crítico sobre as nossas concepções de relação humana.ABSTRACT: This work examines the role of ceramics in Kadiwéu social life. The Kadiwéu are Amerindians who live in the southern part of Pantanal Matogrossense, Brazil. The relations between art and social world will be described and analyzed through ethnographic examples,showing how the Kadiwéu understand their ceramic as a special way of relating to the external world, markedly the “world of the “whites”. This relational understanding of objects also points out, in a reflexive and critical manner, to crucial aspects of western conceptions of human relations.

  3. ALMA + VLT observations of a damped Lyman-α absorbing galaxy: massive, wide CO emission, gas-rich but with very low SFR

    Science.gov (United States)

    Møller, P.; Christensen, L.; Zwaan, M. A.; Kanekar, N.; Prochaska, J. X.; Rhodin, N. H. P.; Dessauges-Zavadsky, M.; Fynbo, J. P. U.; Neeleman, M.; Zafar, T.

    2018-03-01

    We are undertaking an Atacama Large Millimeter Array survey of molecular gas in galaxies selected for their strong H I absorption, so-called damped Lyα absorber (DLA)/sub-DLA galaxies. Here, we report CO(2-1) detection from a DLA galaxy at z = 0.716. We also present optical and near-infrared (NIR) spectra of the galaxy revealing [O II], Hα, and [N II] emission lines shifted by ˜170 km s-1 relative to the DLA, and providing an oxygen abundance 3.2 times solar, similar to the absorption metallicity. We report low unobscured SFR˜1 M⊙ yr-1 given the large reservoir of molecular gas, and also modest obscured SFR =4.5_{-2.6}^{+4.4} M⊙ yr-1 based on far-IR and sub-millimetre data. We determine mass components of the galaxy: log[M*/M_{&sun} ]= 10.80^{+0.07}_{-0.14}, log[Mmol-gas/M⊙] = 10.37 ± 0.04, and log[Mdust/M_{⊙} ]= 8.45^{+0.10}_{-0.30}. Surprisingly, this H I absorption-selected galaxy has no equivalent objects in CO surveys of flux-selected samples. The galaxy falls off current scaling relations for the star formation rate (SFR) to molecular gas mass and CO Tully-Fisher relation. Detailed comparison of kinematical components of the absorbing, ionized, and molecular gas, combined with their spatial distribution, suggests that part of the CO gas is both kinematically and spatially decoupled from the main galaxy. It is thus possible that a major starburst in the past could explain the wide CO profile as well as the low SFR. Support for this also comes from the spectral energy distribution favouring an instantaneous burst of age ≈0.5 Gyr. Our survey will establish whether flux-selected surveys of molecular gas are missing a key stage in the evolution of galaxies and their conversion of gas to stars.

  4. Women in body and soul: biopsychosocial factors in menopause / Mulheres de corpo e alma: aspectos biopsicossociais da meia-idade feminina

    Directory of Open Access Journals (Sweden)

    Maria Elizabeth Mori

    2004-01-01

    Full Text Available This study investigated biological, psychological and sociocultural aspects that interact in middle-aged women in order to better understand their feelings and experiences. The advent of the menopause — characterized by the end of the menstruation and by psychic and physical manifestations — imposes fundamental questions that, on the limit, may elicit depressive symptoms. Hormonal changes are implicated in the aging process, that point to the finitude. A feeling of not being themselves makes many women experience difficulties with losses inherent to this life period.

  5. Mulheres de corpo e alma: aspectos biopsicossociais da meia-idade feminina Women in body and soul: biopsychosocial factors in menopause

    Directory of Open Access Journals (Sweden)

    Maria Elizabeth Mori

    2004-01-01

    Full Text Available Este trabalho investigou na literatura científica os aspectos biológicos, psicológicos e socioculturais que se estão em jogo na etapa da meia-idade feminina a fim de melhor compreender a vivência dessa mulher. O evento da menopausa - caracterizada pela cessação da ovulação e por manifestações físicas e psíquicas - marca este momento vital e impõe questões que, se não forem bem trabalhadas, podem, no limite, ocasionar sintomas depressivos. As mudanças hormonais condicionam o processo de envelhecimento que aponta para a finitude. Um certo estranhamento em relação a si mesma faz com que muitas mulheres tenham dificuldades em lidar com as perdas inerentes a esta fase de vida.This study investigated biological, psychological and sociocultural aspects that interact in middle-aged women in order to better understand their feelings and experiences. The advent of the menopause - characterized by the end of the menstruation and by psychic and physical manifestations - imposes fundamental questions that, on the limit, may elicit depressive symptoms. Hormonal changes are implicated in the aging process, that point to the finitude. A feeling of not being themselves makes many women experience difficulties with losses inherent to this life period.

  6. Da Dor no Corpo à Dor na Alma: O Conceito de Violências Psicológicas da Lei Maria Da Penha

    Directory of Open Access Journals (Sweden)

    Isadora Vier Machado

    2015-05-01

    Full Text Available Este artigo expõe os resultados de pesquisa de campo, realizada entre dezembro de 2010 e julho de 2011 em uma cidade do Sul do Brasil, a respeito da instrumentalização do conceito de violências psicológicas, trazido pela Lei Maria da Penha (Lei 11.340/06, a fim de construir uma leitura da lei a partir deste conceito. Os dados são referentes às/aos agentes que compõem o corpus da polícia, na Delegacia da Mulher e do Ministério Público do município, prioritariamente. Nesses locais, buscou-se compreender como o conceito de violências psicológicas é trabalhado pelas/os agentes e qual o significado teórico-prático que o subjaz. Enfim, coloca-se este dispositivo da lei em posição de questionar a sua própria implementação, de pensar as mudanças que se operam na condição de mulheres em situação de violências e de problematizar as relações entre local e global no campo estudado. A metodologia utilizada foi composta por pesquisa de inspiração etnográfica e levantamento bibliográfico nos campos do Direito, da Psicologia e da Antropologia.

  7. Genellenebilirlik Kuramıyla Dikiş Atma ve Alma Becerileri İstasyonu Güvenirliğinin Değerlendirilmesi

    Directory of Open Access Journals (Sweden)

    Funda NALBANTOĞLU YILMAZ

    2015-06-01

    Full Text Available The aim of the study is to determine the reliability of performance scores of the medical education students in the skills by suturing and removal of suture and to investigate the scoring reliability of unbalanced data regarding students, raters, skills, tasks and their interactions by using generalizability theory. The study group consisted of 309 students who attended the Objective Structural Clinical Exam (OSCE at Hacettepe University. 11 raters from the medical field took part in the assessment of the performance of students. Unbalanced (ö:px(g:b design (ö: student, p: rater, g: task and b: skill was used in this study. As a result, the variability of raters didn’t cause any differences in scoring. There is no difference in both skills and at each task of skills originating from rater effect. Reliability coefficients obtained by generalizability theory for the performance assessment process of the students’skills of suturing and removal of suture are at the acceptable level

  8. Landscape structure and management alter the outcome of a pesticide ERA: evaluating impacts of endocrine disruption using the ALMaSS European Brown Hare model

    DEFF Research Database (Denmark)

    Topping, Christopher John; Dalby, Lars; Skov, Flemming

    2016-01-01

    There is a gradual change towards explicitly considering landscapes in regulatory risk assessment. To realise the objective of developing representative scenarios for risk assessment it is necessary to know how detailed a landscape representation is needed to generate a realistic risk assessment...

  9. Landscape structure and management alter the outcome of a pesticide ERA: Evaluating impacts of endocrine disruption using the ALMaSS European Brown Hare model.

    Science.gov (United States)

    Topping, Chris J; Dalby, Lars; Skov, Flemming

    2016-01-15

    There is a gradual change towards explicitly considering landscapes in regulatory risk assessment. To realise the objective of developing representative scenarios for risk assessment it is necessary to know how detailed a landscape representation is needed to generate a realistic risk assessment, and indeed how to generate such landscapes. This paper evaluates the contribution of landscape and farming components to a model based risk assessment of a fictitious endocrine disruptor on hares. In addition, we present methods and code examples for generation of landscape structures and farming simulation from data collected primarily for EU agricultural subsidy support and GIS map data. Ten different Danish landscapes were generated and the ERA carried out for each landscape using two different assumed toxicities. The results showed negative impacts in all cases, but the extent and form in terms of impacts on abundance or occupancy differed greatly between landscapes. A meta-model was created, predicting impact from landscape and farming characteristics. Scenarios based on all combinations of farming and landscape for five landscapes representing extreme and middle impacts were created. The meta-models developed from the 10 real landscapes failed to predict impacts for these 25 scenarios. Landscape, farming, and the emergent density of hares all influenced the results of the risk assessment considerably. The study indicates that prediction of a reasonable worst case scenario is difficult from structural, farming or population metrics; rather the emergent properties generated from interactions between landscape, management and ecology are needed. Meta-modelling may also fail to predict impacts, even when restricting inputs to combinations of those used to create the model. Future ERA may therefore need to make use of multiple scenarios representing a wide range of conditions to avoid locally unacceptable risks. This approach could now be feasible Europe wide given the landscape generation methods presented.

  10. ALMA [N ii] 205 μ m Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7

    Energy Technology Data Exchange (ETDEWEB)

    Lu, Nanyao; Xu, C. Kevin; Zhu, Lei [National Astronomical Observatories, Chinese Academy of Sciences (CAS), Beijing 100012 (China); Zhao, Yinghe [Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011 (China); Díaz-Santos, Tanio [Nucleo de Astronomia de la Facultad de Ingenieria, Universidad Diego Portales, Av. Ejercito Libertador 441, Santiago (Chile); Charmandaris, Vassilis [Department of Physics, University of Crete, GR-71003 Heraklion (Greece); Gao, Yu [Purple Mountain Observatory, CAS, Nanjing 210008 (China); Van der Werf, Paul P. [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Privon, George C. [Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción (Chile); Inami, Hanae [Centre de Recherche Astrophysique de Lyon (CRAL), Observatoire de Lyon, CNRS, UMR5574, F-69230, Saint-Genis-Laval (France); Rigopoulou, Dimitra [Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom); Sanders, David B., E-mail: nanyao.lu@gmail.com [University of Hawaii, Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

    2017-06-20

    We present the results from Atacama Large Millimeter/submillimeter Array imaging in the [N ii] 205 μ m fine-structure line (hereafter [N ii]) and the underlying continuum of BRI 1202-0725, an interacting galaxy system at z = 4.7, consisting of a quasi-stellar object (QSO), a submillimeter galaxy (SMG), and two Ly α emitters, all within ∼25 kpc of the QSO. We detect the QSO and SMG in both [N ii] and continuum. At the ∼1″ (or 6.6 kpc) resolution, both the QSO and SMG are resolved in [N ii], with the de-convolved major axes of ∼9 and ∼14 kpc, respectively. In contrast, their continuum emissions are much more compact and unresolved even at an enhanced resolution of ∼0.″7. The ratio of the [N ii] flux to the existing CO(7−6) flux is used to constrain the dust temperature ( T {sub dust}) for a more accurate determination of the FIR luminosity L {sub FIR}. Our best estimated T {sub dust} equals 43 (±2) K for both galaxies (assuming an emissivity index β = 1.8). The resulting L {sub CO(7−6)}/ L {sub FIR} ratios are statistically consistent with that of local luminous infrared galaxies, confirming that L {sub CO(7−6)} traces the star formation (SF) rate (SFR) in these galaxies. We estimate that the ongoing SF of the QSO (SMG) has an SFR of 5.1 (6.9) × 10{sup 3} M {sub ⊙} yr{sup −1} (±30%) assuming Chabrier initial mass function, takes place within a diameter (at half maximum) of 1.3 (1.5) kpc, and will consume the existing 5 (5) × 10{sup 11} M {sub ⊙} of molecular gas in 10 (7) × 10{sup 7} years.

  11. Lo que es la atención primaria de la salud: algunas consideraciones a casi treinta y cinco años de Alma-Ata

    Directory of Open Access Journals (Sweden)

    David A Tejada de Rivero

    Full Text Available La atención primaria de la salud fue concebida en la década de los 70 como una estrategia política para lograr la meta social de “Salud para todos”. Respondió a importantes cambios en los terrenos social, político y económico que ocurrieron a nivel global después la segunda guerra mundial, y que siguen ocurriendo hasta la actualidad. Por una desafortunada mala traducción del inglés al español y una errada interpretación de términos, la atención primaria de la salud ha sido malentendida por muchos como “atención en el nivel primario de salud” o como la “dotación de un paquete de prestaciones básicas pero insuficientes a los más pobres”, conceptos erróneos que mantienen las inaceptables inequidades sociales y de salud que hoy seguimos sufriendo. Este artículo explicita lo que es y lo que no es la atención primaria de la salud para abordar el tema desde su verdadero contexto, y hacia su verdadero norte.

  12. Poder-saber-querer: os terrenos disciplinares da alma e do autogoverno no primeiro mapa das ciências da educação (1879-1911

    Directory of Open Access Journals (Sweden)

    Jorge Ramos do Ó

    2012-02-01

    Full Text Available Este artigo procura mostrar que a sedimentação histórica de um discurso coerente, quer sobre o estatuto científico da pedagogia, quer sobre os fins do ato educativo moderno, pode ser igualmente discutida no quadro geral da secularização da moral e da expansão do princípio político do self-government. Para tanto nele se defende que uma formação discursiva de caráter pedagógico assumiu em finais do século XIX a centralidade do material ético, assimilando-o ao axioma do poder iluminista-humanista em que o comportamento cívico do cidadão deve decorrer dos compromissos e decisões da esfera privada da sua consciência. Como é analisada aqui, a psicopedagogia moderna foi estruturada historicamente como mais um regime do eu.

  13. The evolution of CNO isotopes: a new window on cosmic star formation history and the stellar IMF in the age of ALMA

    Science.gov (United States)

    Romano, D.; Matteucci, F.; Zhang, Z.-Y.; Papadopoulos, P. P.; Ivison, R. J.

    2017-09-01

    We use state-of-the-art chemical models to track the cosmic evolution of the CNO isotopes in the interstellar medium of galaxies, yielding powerful constraints on their stellar initial mass function (IMF). We re-assess the relative roles of massive stars, asymptotic giant branch (AGB) stars and novae in the production of rare isotopes such as 13C, 15N, 17O and 18O, along with 12C, 14N and 16O. The CNO isotope yields of super-AGB stars, novae and fast-rotating massive stars are included. Having reproduced the available isotope enrichment data in the solar neighbourhood, and across the Galaxy, and having assessed the sensitivity of our models to the remaining uncertainties, e.g. nova yields and star formation history, we show that we can meaningfully constrain the stellar IMF in galaxies using C, O and N isotope abundance ratios. In starburst galaxies, where data for multiple isotopologue lines are available, we find compelling new evidence for a top-heavy stellar IMF, with profound implications for their star formation rates and efficiencies, perhaps also their stellar masses. Neither chemical fractionation nor selective photodissociation can significantly perturb globally averaged isotopologue abundance ratios away from the corresponding isotope ones, as both these processes will typically affect only small mass fractions of molecular clouds in galaxies. Thus, the Atacama Large Millimeter Array now stands ready to probe the stellar IMF, and even the ages of specific starburst events in star-forming galaxies across cosmic time unaffected by the dust obscuration effects that plague optical/near-infrared studies.

  14. The Structure and Dynamics of An Active Galactic Nucleus Torus : CO Line Predictions for ALMA from Three-dimensional Hydrodynamical Simulations with X-ray-driven Chemistry

    NARCIS (Netherlands)

    Perez Beaupuits, J.P.; Wada, K.; Spaans, M.

    2011-01-01

    Several attempts have been made to model the mass distribution and dynamical evolution of the circumnuclear gas in active galactic nuclei (AGNs). However, chemical evolution is not included in detail in three-dimensional (3D) hydrodynamic simulations. The X-ray radiation from the AGN can drive the

  15. Eugenizar a alma: a constituição da euphrenia no projeto de higiene mental voltado à infância da Liga Brasileira de Hygiene Mental

    Directory of Open Access Journals (Sweden)

    Cristiane Oliveira

    2011-12-01

    Full Text Available O presente artigo analisa a constituição da "euphrenia" como um novo domínio para a psiquiatria brasileira na sua abordagem eugênica e higiênica da infância. A análise de saberes médicos e psicológicos acerca do psiquismo infantil no Brasil das décadas de 1920 e 1930 descortina a intensa circulação afetiva intrafamiliar como ponto de ancoragem para um projeto de normalização social, ainda centrado na eugenia, mas já atravessado por uma psicologia da adaptação.

  16. A educação de corpo e alma como elemento para a produção do sujeito saudável

    Directory of Open Access Journals (Sweden)

    Rogério Rodrigues

    Full Text Available Pensar a relação entre a educação do corpo e a produção do sujeito saudável é poder pensar uma educação física cuja prática proporcione condições de saúde para o sujeito. Compreende-se que o corpo se constitui como meio de representação permanente para que o sujeito possa significar a si mesmo um ser saudável. O objetivo desta reflexão é compreender a educação das práticas corporais como algo que permita ao sujeito representar sua concepção de corpo saudável. Neste aspecto, parte-se da hipótese de que seria de fundamental importância a construção de processos analíticos críticos sobre as diversas práticas corporais educativas que se instituem no cotidiano, tendo como referência as condições que subordinam o sujeito à ordem social.

  17. Do cuidado da alma ao cuidado do corpo: uma nova compreensão da história da enfermagem

    Directory of Open Access Journals (Sweden)

    Maria Itayra Coelho de Souza Padilha

    1998-09-01

    Full Text Available O estudo aborda o nascimento e desenvolvimento da Companhia das Irmãs de Caridade de São Vicente de Paulo, na França, a partir de 1633. Tem como objetivos reconstruir historicamente o processo de criação da Companhia das Irmãs de Caridade de São Vicente de Paulo e o papel de Luiza de Marillac e Padre Vicente de Paulo neste processo; e discutir a importância da Companhia na proposição de um cuidado de enfermagem pré-profissional, imprimindo as bases do que seria chamado posteriormente de técnicas de enfermagem. É um estudo de natureza sócio-histórica, para o qual utilizarei as idéias preconizadas por Michel Foucault, com relação à análise e discussão dos documentos à luz da análise genealógica. Enfoca principalmente os aspectos que tratam da implementação de uma prática de enfermagem voltada para o cuidado do corpo doente e para a catequização dos pobres e enfermos. Enfatiza-se também a importância de Luiza de Marillac como enfermeira, mestre e guia das demais Irmãs.

  18. Exploring the molecular chemistry and excitation in obscured luminous infrared galaxies. An ALMA mm-wave spectral scan of NGC 4418

    NARCIS (Netherlands)

    Costagliola, F.; Sakamoto, K.; Muller, S.; Martín, S.; Aalto, S.; Harada, N.; van der Werf, P.; Viti, S.; Garcia-Burillo, S.; Spaans, M.

    2015-01-01

    Context. Extragalactic observations allow the study of molecular chemistry and excitation under physical conditions which may differ greatly from those found in the Milky Way. The compact, obscured nuclei (CON) of luminous infrared galaxies (LIRG) combine large molecular columns with intense

  19. La Virgen con el Niño y las Almas del Purgatorio de Pedro Machuca y su vinculación italiana

    Directory of Open Access Journals (Sweden)

    Ávila, Ana

    2012-06-01

    Full Text Available The author examines the incorporation of this painting into the collections of the Prado Museum in 1935, which generated the scrutiny of the state of knowledge concerning the painter at the time and the consolidation of his artistic reputation. The painting probably came from Naples, thereby explaining the idiosyncratic Italian iconography, common in the Viceroyalty.Se estudia el ingreso del cuadro en el Museo del Prado en 1935 –lo cual motiva el estado de la cuestión del artista en esos momentos y la consolidación de su imagen como pintor– y su probable procedencia napolitana, resaltando la idiosincrasia italiana de su iconografía, común en el Virreinato.

  20. Louis Vuitton: El alma del viaje. El viaje como concepto idealista de una marca a través de la publicidad

    OpenAIRE

    González Revuelta, Paula

    2014-01-01

    La publicidad del sector de la moda y concretamente de Louis Vuitton presenta en la actualidad un nivel de sofisticación y notoriedad elevado porque introduce un lenguaje onírico, simbólico y emocional en sus relatos. La investigación sitúa y da significado a la simbología del concepto del viaje presente en las campañas publicitarias y en la esencia de la marca Louis Vuitton, y su constante evocación al pasado. Tomando como objeto de análisis las campañas gráficas realizadas desde los inicios...

  1. TEDARİKÇİ GELİŞTİRMENİN SATIN ALMA PERFORMANSINA ETKİSİNE YÖNELİK YAPISAL MODEL ÖNERİSİ

    OpenAIRE

    USTASÜLEYMAN, Talha

    2009-01-01

    Tedarik zinciri yönetimi, tedarik zincirindeki farklı taraflar arasındaki ilişki ve faaliyetleri yöneten sistematik ve bütünleştirici bir yaklaşımdır. Tedarik zinciri yönetiminin başarılı bir şekilde uygulanmasında ise tedarikçi geliştirme önemli bir rol oynamaktadır. Tedarikçi geliştirme temel tedarikçi geliştirme ve ileri tedarikçi geliştirme olmak üzere iki farklı açıdan ele alınabilmektedir. Temel tedarikçi geliştirme firma kaynaklarına minimum yatırım yapmayı ve en sınırlı seviyede firma...

  2. 4.TÜKETİCİLERİN KÜRESEL MARKA ALGISI VE SATIN ALMA NİYETİ ÜZERİNDEKİ ETKİSİ

    OpenAIRE

    TAŞKIN, Ercan; SÖYLEMEZ, Cevat

    2015-01-01

    Consumers are the most important actors that dominate the marketing activities of business today. Therefore, it is very important to meet the expectations of consumers. The consumption behaviours of the consumers should be analysed and the factors that influence these behaviours should be determined in detail. This is a necessity brought forward by the consumption habits that change due to the effects of globalisation. In this sense, especially global brands should determine the consumption h...

  3. Ilusiones ópticas del alma: conflictos en torno a la representación en la obra de Gómez de Avellaneda (1860-1864

    Directory of Open Access Journals (Sweden)

    Suquet Martínez, Mirta

    2014-12-01

    Full Text Available This article focuses on the texts Gertrudis Gómez de Avellaneda’s wrote during her stay in Cuba (1860-1864, in order to clarify some discursive strategies used by the author to avoid the claims of her nationalist compatriots. Faced with the demands of objectivity of the nationalist authors, Gómez de Avellaneda chooses to avert her gaze and to approach the Island from caution and distance in her poems. Gómez de Avellaneda defends the re-working of perception in her literary criticism and her novel El artista barquero from a poetics of the emotions that resists the nationalist “positivism”.Este artículo estudia textos de Gertrudis Gómez de Avellaneda escritos en su estancia en Cuba (1860-1864, con el objetivo de explicar las estrategias discursivas utilizadas por la autora para esquivar los reclamos nacionalistas de sus compatriotas. Frente a la política de la visión que da cuerpo a las demandas de objetividad de los nacionalistas, Avellaneda opta, en sus poemas de esta fecha, por un enfoque de la Isla desde la cautela y la distancia. En textos de crítica literaria y en la novela El artista barquero, Avellaneda defiende la reelaboración de la percepción a partir de una poética de las emociones que contrarreste el “positivismo” nacionalista.

  4. Alma sensible, romanticismo exaltado y suicidio. Sobre la novela Voyleano o la exaltación de las pasiones (1827, de Estanislao de Cosca Vayo y Lamarca

    Directory of Open Access Journals (Sweden)

    Sebold, Russel P.

    2014-12-01

    Full Text Available The character Voyleano has models in the suicide Werther, by Goethe, and in the death-desiring Tediato in the Lugubrious Nights, by Cadalso. The creation of the figure of Voyleano depends on the new sensibility of the Enlightenment, romantic cosmic grief, and the exaltation of romantic psychology. In the novel by Vayo the Napoleonic invasion of Spain is depicted, and this atmosphere lends itself to libertine seductions, betrayals, great disillusionments, and the loss of faith. Voyleano, like don Quijote, like Julien Sorel, like Emma Bovary, and like several characters from Larra and Mesonero Romanos has sought a model or logos in an earlier character. After don Quijote Voyleano is the first of all of them. Voyleano considers the physical act of suicide lacking in nobility and cowardly, and although he is inspired by Werther, he is attracted to Tediato’s way of committing suicide while avoiding the physical act of suicide.El personaje Voyleano tiene modelos en el suicida Werther, de Goethe, y en el deseoso de morir Tediato de las Noches lúgubres, de Cadalso. Entran en la confección de la figura de Voyleano la nueva sensibilidad de la Ilustración, el dolor cósmico romántico y la exaltación de la psicología romántica. En la novela de Vayo se vive la invasión napoleónica de España, y tal ambiente se presta a seducciones libertinas, traiciones, grandes desilusiones y pérdida de la fe. Voyleano, como don Quijote, como Julien Sorel, como Emma Bovary y como varios personajes de Larra y Mesonero Romanos ha buscado un modelo o logos en un personaje anterior. Después de don Quijote, Voyleano es el primero de todos ellos. A Voyleano le parece poco noble y cobarde el acto físico del suicidio, y aunque se inspira en Werther, le atrae en Tediato el modo de suicidarse evitando el acto físico del suicidio.

  5. Fuente de corriente alterna controlable entre 1 Hz y 50 kHz para aplicaciones de congelación magnética: diseño e implementación de la etapa de potencia

    OpenAIRE

    Fuente Taravillo, Guillermo

    2017-01-01

    El propósito de este Trabajo Fin de Grado es diseñar un dispositivo capaz de suministrar una intensidad de corriente senoidal a una carga inductiva con el fin de generar un campo magnético en su interior. El dispositivo en cuestión es un convertidor de tensión continua a alterna (CC-CA), también conocido corno inversor electrónico. El campo magnético generado servirá en un futuro para investigar la influencia de este en el proceso de congelación de matrices alimentarias y otros tejidos. E...

  6. Sistema de geração fotovoltaico multifuncional

    OpenAIRE

    Brandão, Danilo Iglesias [UNESP

    2013-01-01

    O objetivo deste trabalho foi desenvolver um sistema de geração fotovoltaico híbrido, ou seja, capaz de funcionar tanto interligado à rede elétrica como desconectado (ilhado) desta. Quanto ilhado, este sistema fornece potência e uma tensão senoidal para a carga, desde que haja energia solar nos módulos fotovoltaicos e/ou energia armazenada no banco de baterias. Quando conectado, o sistema de geração fotovoltaico é capaz de fornecer potência ativa para a carga e/ou rede elétrica e, simultaneam...

  7. Modelagem matemática do comportamento mecânico do detector de ondas gravitacionais "Mario Schenberg"

    OpenAIRE

    Cesar Augusto Costa

    2002-01-01

    O objetivo principal deste trabalho é modelar matematicamente o comportamento mecânico do detector de ondas gravitacionais Mario Schenberg. São estudados os parâmetros físicos que afetam este comportamento. O modelo prevê as frequências de ressonância do sistema, quando são acoplados ressonadores mecânicos unidimensionais de dois modos, obedecendo a configuração sugerida por Johnson e Merkowitz. Prevê, também, como o sistema se comporta frente a um trem de onda gravitacional senoidal. Uma est...

  8. Control de un motor brushless con aumento de la resolución del resolver mediante "oversampling"

    OpenAIRE

    Gross Igor, Gabriel

    2004-01-01

    Premi al millor Projecte de Fi de Carrera presentat durant el curs 2003-2004 en l'àmbit d'Electricitat-Electrònica-Automàtica que atorga SCHNEIDER ELECTRIC En este proyecto se ha diseñado y montado el control completo de un motor brushless senoidal con un DSP (Digital Signal Processor). En el DSP no se solo se ha programado el control propiamente dicho, sino también un algoritmo para adquirir la posición del motor con más resolución de la que nos permite el algoritmo tradicional (basado en...

  9. UNA PERSONA ENTREGADA EN CUERPO Y ALMA A LA REVOLUCIÓN ¿Quiénes eran los Guerrilleros del PRT-ERP de Argentina?UMA PESSOA DEDICADA DE CORPO E ALMA À REVOLUÇÃO Quem eram os Guerrilheiros da PRT-ERP da Argentina?

    Directory of Open Access Journals (Sweden)

    Pablo Alejandro Pozzi

    2009-12-01

    Full Text Available El  PRT-ERP fue una de las principales organizaciones guerrilleras argentinas entre  1969 y 1977. Uno de los principales problemas en todo tipo de análisis de  organizaciones clandestinas y perseguidas, como el PRT-ERP, tiene que ver con  definir quiénes las integraron. Esto es particularmente complejo porque la  cantidad de datos disponibles es escasa. En este estudio intentamos reconstruir  el perfil de los militantes del PRT-ERP. En este sentido buscamos centrarnos en  las cuestiones de quiénes fueron, de dónde provenían, cuál era su historia  familiar y laboral, cuál fue el proceso de politización y qué factores  incidieron en el mismo, porqué se incorporaron a esta organización y no a otra.  En función de lo anterior, intentamos reconstruir la historia de vida de una  cantidad de militantes, aspirantes y simpatizantes de la organización entre  1968 y 1976 y, así, esta reconstrucción se hizo sobre  la base de una serie de fuentes de información muy variada, incluyendo  documentos partidarios y testimonios de militantes. Palabras-Clave: Argentina. Guerrilla.  Militancia. Historia de Vida. Lucha Armada.   Resumo O  PRT-ERP foi uma das principais organizações guerrilheiras argentinas entre 1969  e 1977. Um dos principais problemas de todo tipo de análise de organizações  clandestinas e perseguidas, tal como PRT-ERP, está asociado ao perfil de seus  integrantes. Isto é particularmente complexo porque a quantidade de dados  disponíveis são escassos. Neste estudo procuramos reconstruir o perfil dos  militantes do PRT-ERP. Neste sentido, procuramos centrar a análise na  identificação dos integrantes, de onde provinham, qual era sua história  familiar e laboral, qual foi o seu processo de politização e quais fatores  incidiram no mesmo, por que se incorporaram a esta organização e não a outra.  Em função disto, procuramos reconstruir a história de vida de uma quantidade de  militantes, aspirantes e simpatizantes da organização entre 1968 e 1976 e,  assim, esta reconstrução foi feita tendo em vista uma série de fontes de  informações muito variadas, incluindo documentos partidários e testemunhos de  militantes. Palavras-Chave: Argentina. Guerrilha. Militância. História de Vida.  Luta Armada.   Abstract: The PRT-ERP was one of Argentina’s  main guerrilla organizations between 1969 and 1977. Due to their clandestine  nature, a problem found in the analysis of these groups was to define who joined  it and why. This is particularly complicated due to the scarcity of available  hard data. This study seeks to answer who the PRT-ERP militants were, where  they came from, what their family and work background was, what their process  of politicization was, and why they joined this specific organization. As such,  the study seeks to reconstruct life histories of several hundred PRT  guerrillas. This effort is based on a variety of sources including party  documentation, and dozens of interviews with former militants. Keywords: Argentina.  Guerrilla. Militancy. Life Stories. Armed  Struggle.

  10. Urinary excretion of N-acetyl-S-allyl-L-cystein upon garlic consumption by human volunteers.

    NARCIS (Netherlands)

    de Rooij, B.M.; Boogaard, P.J.; Rijksen, D.A.; Commandeur, J.N.M.; Vermeulen, N.P.E.

    1996-01-01

    N-Acetyl-S-allyl-L-cysteine (allylmercapturic acid, ALMA) was previously detected in urine from humans consuming garlic. Exposure of rats to allyl halides is also known to lead to excretion of ALMA in urine. ALMA is a potential biomarker for exposure assessment of workers exposed to allyl halides.

  11. Nooruslik kaupmeheemand kavatseb äri laiendada / Hille Tänavsuu

    Index Scriptorium Estoniae

    Tänavsuu, Hille, 1941-2014

    2006-01-01

    Vt. ka Postimees : na russkom jazõke 23. märts lk. 8. Tallinnas Vana-Kalamaja tänaval paikneva Alma Äri omanik Alma Sooäär avas oma esimese poe enam kui 15 aastat tagasi Nõmmel, praegu plaanib poeomanik majapidamistarvete äri laiendamist. Kaart: Alma Äri

  12. Projeto de pontes mistas de aço e betão

    OpenAIRE

    Cardoso, Renato Azevedo

    2015-01-01

    O trabalho aqui apresentado visa dar uma compreensão didática do dimensionamento de pontes mistas de aço e betão, assim como avaliar a resposta estrutural sob condições de serviço de pontes mistas, quando sujeitas a diferentes processos construtivos. Tendo isto em consideração, é apresentada uma descrição teórica, seguindo-se um exemplo numérico e um estudo focado no comportamento em serviço de pontes mistas, quando sujeitas a diferentes processos construtivos. A descriçã...

  13. VİRAL PAZARLAMA ARACI OLARAK E-POSTA: E-POSTA ALMA VE GÖNDERMENİN GERİSİNDEKİ DUYGULAR ÜZERİNE BİR ARAŞTIRMA

    OpenAIRE

    YILMAZ, Burcu Selin

    2009-01-01

    İnternetin yaygınlaşması, tüketicilere ürün ve hizmetler hakkında diğer tüketicilerden bilgi edinmenin yeni yollarını sunmaktadır. Bu tür iletişim ağızdan ağza iletişimin bir türü olarak görülmekte, ağızdan fareye ya da çevrimiçi ağızdan ağza iletişim olarak adlandırılırken, tüketicilere de güç kazandırmaktadır. Tüketiciler, bağlantıda oldukları bireyler ile görüşlerini eposta gönderme, web sitelerine ve forumlara yorumlar ve geribildirimler gönderme, çevrimiçi bloglar oluşturma ve internette...

  14. TURİSTİK ÜRÜN SATIN ALMA DAVRANIŞININ TEKNOLOJİ KABUL MODELİ İLE İNCELENMESİ (INVESTIGATION OF TOURISM PRODUCT PURCHASING BEHAVIOUR BY THECHNOLOGY ACCEPTANCE MODEL

    Directory of Open Access Journals (Sweden)

    Ali TÜRKER

    2013-04-01

    Full Text Available Today, the quickly spreading of Internets’ using throughout all part of the community, changed the individuals habits and behaviors as a consumer as well as their lives. One of the important phenomena occurring In recent years, shopping over the Internet, could affect the tourists’ purchase decision process and exist as being a determining factor in the decision process stages, so it is becoming a controversial issue and increasingly important issue on the tourism product buying decision. In Turkey the number of research topics examining the shopping behavior of tourists over the Internet, is yet very insufficient. This study is being done in order to determine the behavior and tendencies of tourist coming to Turkey related to e-shopping, but also to discuss the efficiency of TAMs’ explaining the behavior of tourists through buying on internet.The main objective of this study is to examine the tourist product purchase behavior with the Technology Acceptance Model. The determination of the factors on touristic buying behavior and the directions and rates, will shed the light over electronic marketing activities.

  15. Entre reses e almas: questões sobre urbanização, arquitetura e arte das missões jesuíticas dos sertões das capitanias do norte

    Directory of Open Access Journals (Sweden)

    Esdras Arraes

    2015-02-01

    Full Text Available O povoamento e a instituição da rede urbana dos sertões das capitanias do Norte surgiram com o apoio régio ao duplo movimento realizado por criadores de gado e missionários, a partir de meados do século 17. Sendo assim, este ensaio busca interpretar, por meio de evidências materiais, como os encontros - simbióticos e/ou conflituosos - entre pecuária e catequese jesuítica estruturaram os fenômenos urbano, arquitetônico e artístico, em uma região considerada pela historiografia clássica como “periférica” aos interesses políticos da Coroa Portuguesa. Interpretaremos, no território, como as estratégias de conversão do indígena criaram uma malha de aldeamentos missioneiros precisamente locados na área. Ainda apontaremos, em linhas gerais, como as edificações jesuíticas seguiram modelos formais encontrados nos principais centros de irradiação cultural da colônia e da Europa. Sem esquecer, portanto, a consideração que tiveram os padres em “dialogar” tais arquiteturas com os condicionantes geográficos, naturais e sociais daquelas vastidões.

  16. El alma en venta: Apuntes para un debate teórico sobre el trabajo de cuello blanco en empresas multinacionales Souls on Sale: Notes for a Theoretical Debate about White Collar work in Multinacional Enterprises

    Directory of Open Access Journals (Sweden)

    Diego Szlechter

    2011-06-01

    Full Text Available La Segunda Guerra mundial provoca la desaparición de viejos estilos de vida en el mundo occidental. Una de las causas de este fenómeno se compone de drásticos cambios en la estructura ocupacional de occidente, especialmente en EEUU, que resultaron en una nueva clase media de administradores surgidos de los college devenidos muchos de ellos gerentes de las grandes corporaciones. La emergencia de los gerentes como asalariados pone en cuestión la idea de una clase asalariada homogénea al estilo marxista debido a la expansión de actores tales como burócratas, profesionales, que no se agotan en una explicación dualista o dicotómica de la sociedad. Los estudios acerca del trabajo gerencial se enmarcan dentro de los debates acerca de la transición del llamado "fordismo" hacia el "posfordismo" o de producción en masa a la producción flexible. Estas discusiones suelen soslayar o relegar a un papel secundario la cuestión de las transformaciones en la identidad y la subjetividad dentro del espacio de trabajo. Sostenemos en este trabajo que el espacio laboral ocupa un rol fundamental en la conformación de la identidad. Este supuesto se opone a los pronósticos más optimistas del llamado posfordismo que consideran que la esfera extralaboral es la que imprime su sello sobre el mundo del trabajo. La intención de este artículo es indagar, por un lado, cómo abordan las Ciencias Sociales en general y los debates sobre las Clases Medias, la Sociología del Trabajo y la Sociología de las Organizaciones en particular, la cuestión del trabajo gerencial y por otro, qué aportes realiza la bibliografía en este campo para intentar esclarecer qué tipo de subjetividad propician las empresas para con sus mandos gerenciales y qué implicancias conlleva en la práctica laboral concreta de éstos. Es así como se presentarán 3 debates fundamentales que han surcado el camino para acercarnos a dilucidar esta cuestión: la discusión sobre calificación y competencias, la perspectiva de la cultura laboral y, por último, la teoría del capital humano.Second World War caused the disappearing of older life styles in western world. One of the reasons of this phenomen relies on drastic changes in the occupational structure in western world, especially in the US, which result in a new middle class of managers that emerged from colleges who became big bosses in corporate America. Those salaried managers questioned the idea of a homogeneous salaried class in the Marxist way due to the expansion of players such as bureaucrats, professionals, who doesn´t deplete in a dualist or dichotomist explanation of society. Labor studies about managers are framed into the debates around the transition from fordism to posfordism or from mass production to lean production. These discussions used to relegate to a secondary roll the issue of the transformations in the identity and subjectivity at work. We stress in this article that work engage a fundamental roll in the configuration of identity. This postulation opposes to most optimistic forecasts of the so called posfordism, which regard the world outside work as one that outweighs world of labor. The intention of this article is to inquire, on one side, the way Social Sciences in general and the debates around Middle Classes, Sociology of Work and Organizational Sociology in particular, the issue of managerial work and on the other side, which contributions make bibliography in this field in order to clear up what kind of subjectivity corporations promote to their middle management and what implications carry on their everyday work. Therefore, we introduce 3 fundamental debates who have plowed the road to try to elucidate this issue: the debate about qualification and competences, the labor culture perspective and human capital theory.

  17. Pobre de mí en esos años oscuros / Tengo el alma amordazada detrás de los ojos / Cadáveres que son tus manos

    OpenAIRE

    Cadena Pardo, Paola

    2016-01-01

    cuando la palabra amor era pronunciable El silencio se hizo nido en el borde de mis labios y los pájaros llegaron todos a morir allí Las uñas carcomidas como una espera impasible que siempre terminó en desdicha en angustia de tiempos huérfanos en hambre que viene como el abandono sigilosa a hurtadillas danza inservible de llantos estirados hasta la punta más lejana del vacío humano hasta la soledad más sola que ni siquiera se tiene a sí misma.

  18. Soul, mind and brain in pre-history and early human civilizations / Alma, mente e cérebro na pré-história e nas primeiras civilizações humanas

    Directory of Open Access Journals (Sweden)

    Fabiano dos Santos Castro

    2010-01-01

    Full Text Available Currently, the debate about the nature of the human mind is taking new directions through the development of several studies in the field of neuroscience which investigates the location of brain functions. These studies have contributed to a better understanding of the neural substrates of mental functions and the etiology of various mental disorders. However, the knowledge developed by neuroscience did not occur abruptly. Indeed, the study of mind-brain relationship is not new. From pre-history to the present days, various different types of inquiries have been made about the possible materiality and location of human mental functions. This paper presents, in a historic manner, how prehistoric populations as well as early civilizations located in Egypt, Mesopotamia, India, and China developed and employed concepts related to the soul, the mind and the human brain.

  19. Torque de inserção e resistência ao arrancamento dos parafusos vertebrais com alma cilíndrica e cônica Insertion torque and pullout strength of vertebral screws with cylindrical and conic core

    Directory of Open Access Journals (Sweden)

    Ariane Zamarioli

    2008-10-01

    Full Text Available OBJETIVO: Avaliar o torque de inserção e a força de arrancamento de três diferentes parafusos utilizados para a fixação anterior da coluna vertebral, considerando a influência do diâmetro do orifício-piloto (DOP, a densidade dos corpos de prova (CDP e o desenho da rosca dos parafusos. MÉTODOS: Foram utilizados CDP de poliuretana com duas densidades: 0,16 e 0,32g/cm³, e três tipos de parafusos (USS I, USS II posterior e USS II anterior. Na primeira etapa o orifício-piloto foi feito com sonda de 3,8mm para todos os parafusos; na segunda etapa, com sonda menor do que o diâmetro interno dos parafusos (3,5mm para os parafusos USS I; 3,4mm para os parafusos USS II posterior e 3,0mm para os parafusos USS II anterior. Foram formados 12 grupos experimentais com dez corpos de prova em cada grupo, de acordo com a densidade da poliuretana, DOP e tipo de parafuso utilizado. O torque foi mensurado durante a inserção dos parafusos e a força de arrancamento por meio de ensaio mecânico em máquina universal de teste. RESULTADOS: O torque máximo de inserção apresentou valores decrescentes nos corpos de prova de 0,16g/cm³ e 0,32g/cm³ e em todos os diâmetros do orifício-piloto. A força máxima de arrancamento, nos corpos de prova de 0,16g/cm³ e diâmetro da perfuração de 3,8mm, foi maior nos parafusos USS II posterior que nos parafusos USS I. Com o diâmetro da perfuração menor do que o diâmetro interno do parafuso, os parafusos USS II posterior e anterior apresentaram valores maiores que o parafuso USS I. Nos corpos de prova com 0,32g/cm³ de densidade e diâmetro de perfuração de 3,8mm, a força de arrancamento do parafuso USS II posterior e a do USS I foram maiores que a do parafuso USS II anterior. Com o diâmetro da perfuração menor que o diâmetro interno, os valores foram decrescentes entre o USS II posterior, USS II anterior e USS I. CONCLUSÕES: O torque de inserção e a força de arrancamento dos parafusos utilizados para fixação anterior da coluna vertebral são influenciados pela densidade do corpo de prova, desenho da rosca do parafuso e diâmetro do orifício-piloto.OBJECTIVE: To evaluate insertion torque and pullout strength of three different screws used in the anterior fixation of the spine, considering the influence of the diameter of the pilot hole (DOP, the test specimen density (CDP, and the screw thread design. METHODS: The authors used polyurethane test specimens with two densities: 0.16 and 0.32 g/cm³, and three types of screws (USS I, USS II posterior, and USS II anterior. In the first stage, the pilot hole was made with a 3.8 mm probe for all screws; in the second stage, with a probe smaller than the inner diameter of the screws (3.5 mm for screws USS I; 3.4 mm for USS II posterior screws, and 3.0 mm for USS II anterior screws. 12 experimental groups were formed with ten specimen tests in each group, according to the polyurethane density, DOP, and the type of screw used. Torque was measured during insertion of the screws and the pullout strength by a mechanical assay in a universal test machine. RESULTS: The maximum insertion torque presented a decreasing value in test specimens of 0.16 g/cm³ and 0.32 g/cm³ and in all pilot hole diameters. Maximum pullout strength in test specimens of 0.16 g/cm³ and 3.8 mm of perforation diameter was greater in USS II posterior screws than in USS I screws. With the perforation diameter smaller than the inner screw diameter, USS II posterior and anterior screws presented higher values than the USS I screw. In test specimens with 0.32 g/cm³ of density and perforation diameter of 3.8 mm, the pullout strength of USS II posterior and USS I screws was greater than that of USS II anterior screws. With the smaller perforation diameter than the inner diameter, the values were decreasing between the USS II posterior screw, then the USS II anterior screw, and then the USS I screw. CONCLUSION: Insertion torque and pullout strength of the screws used in the anterior fixation of the vertebral spine are influenced by the test specimen density, by the screw thread design, and by the diameter of the pilot hole.

  20. “Adiós, adiós, Europa, te me vas de mi alma, de mi cuerpo cansado, de mi chaqueta vieja”: el exilio del “miserable náufrago” Jorge Guillén

    Directory of Open Access Journals (Sweden)

    Cristiana Fimiani

    2014-06-01

    Full Text Available El interrogante antropológico del exiliado Jorge Guillén – “¿Ser hombre es estar de viaje?” – plantea el dilema existencial de ese sujeto escindido que es el ser humano, en busca constante de la propia identidad. El poeta vallisoletano, uno de los representantes más ilustres de la Generación del 27, cuenta la trágica experiencia de la dictadura franquista y del consiguiente destierro; sus poemas describen un sentimiento de desamparo y de exclusión, que se destaca en la mayoría de los versos de Clamor. El hondo sentido que se esconde detrás de la pregunta ontológica guilleniana, en la que se destaca la oposición semántica de los dos verbos elegidos, se puede buscar en la íntima esencia del ser humano, constantemente dividido entre el “ser”, estable e inmudable, y el “estar” de su condición de eterno viajero, vinculado a una existencia precaria y mudable, sujeta a las reglas-no-reglas del azar.

  1. Sai desse corpo que esse caminho não te pertence! Pessoas trans* e ex-trans* em (re/descaminhos de gênero, corpo e alma

    Directory of Open Access Journals (Sweden)

    Eduardo Meinberg de Albuquerque Maranhão Fo.

    2016-01-01

    Full Text Available Apresento, neste artigo, algumas indicações inconclusivas sobre os múltiplos (re/descaminhos religiosos e generificados de pessoas transgêneras e (ex-ex-transgêneras, conectados a discursos religiosos/generificados. Esse trabalho, de história das religiões e religiosidades no tempo imediato, se fundamentou no que chamei, provisoriamente, de etnografia ciborgue, processo que envolve, dentre outras coisas, a conexão entre história oral e trabalho de campo on e off-line. O campo principal de pesquisa se deu em ministérios de “cura e libertação” de travestis, e os resultados provisórios do trabalho, que também utilizou bibliografia referente à questão do corpo como caminho de e para Deus, permitiram perceber algumas das conexões entre agência subjetiva de pessoas trans*, ex-trans*, ex-ex-trans*, e discurso religioso/generificado, ou melhor explicando, como, de formas diversas, discursos religiosos/generificados atuaram nas (re/descarpintarias identitárias de pessoas transgêneras e (ex-ex-transgêneras.

  2. Brancas de almas negras? : beleza, racialização e cosmética na imprensa negra pós-emancipação (EUA, 1890-1930)

    OpenAIRE

    Giovana Xavier da Conceição Côrtes

    2012-01-01

    Resumo: Esta tese investiga as representações femininas presentes em propagandas de produtos de clareamento de pele (bleachings) e crescedores capilares (hair growers) da indústria cosmética, veiculadas pela imprensa afro-americana em Boston, Chicago e Nova York, cidades que, entre os anos 1890 e 1930, passaram por uma série de transformações sociais por conta do fenômeno historicamente conhecido como Grande Migração Negra. Ao considerar o processo de urbanização vivenciado pela população de ...

  3. Fast Food Restoranlarda Fiziksel Çevre, Fiyat Algısı ve Tekrar Satın Alma Eğilimi Arasındaki İlişki

    OpenAIRE

    KÜÇÜKERGİN, Kemal Gürkan; DEDEOĞLU, Bekir Bora

    2014-01-01

    The Servicescape is a determining factor for customers when they need to make a decision on selecting a restaurant. Therefore, in this study, the effect of the Servicescape factor on price perception and then the effect of the price perception on repurchase intention were tested in the scope of the fast food restaurants. The domain of the research is limited to the province of Izmir. For this research, total of 468 usable surveys returned from the people living in the province of Izmir. The d...

  4. Ortopedia del alma. Degeneracionismo e higiene mental en la Casa de Corrección de Menores y Escuela de Trabajo San José, Colombia 1914-1947

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    Jairo Gutiérrez Avendaño

    2016-03-01

    Full Text Available Objetivo Comprender las prácticas y la formación experimental de la psicopedagogía de la infancia anormal en Colombia, llevadas a cabo en la “Casa de Corrección de Menores y Escuela de Trabajo San José”, entre 1914 y 1947. Métodos y materiales: estudio cualitativo, de enfoque histórico-hermenéutico, mediante investigación documental, heurística de archivos de patrimonio documental e historiografía institucional del periodo de estudio. Conclusiones el surgimiento de un nuevo régimen de educación especial (médico-psico-pedagógico estableció un cambio relevante del modelo reformatorio de castigo al de intervención pedagógica, influida por el cruce de doctrinas científicas de finales del siglo XIX y principios del XX, como la regla de lo normal y lo patológico, la teoría de la degeneración y la eugenesia, para el perfeccionamiento de un sujeto moderno capaz de ser útil por sí mismo y para la sociedad.

  5. De corpo, alma e espírito: apontamentos históricos e teológicos acerca do tema santificação na obra holística de Ellen White

    OpenAIRE

    Fábio Augusto Darius

    2014-01-01

    A presente pesquisa aborda historicamente a construção e o desenvolvimento prático e teórico da teologia holística de Ellen White legada à Igreja Adventista do Sétimo Dia. Ellen White, viveu no momento em que seu país, os Estados Unidos da América, estavam se firmando enquanto nação e morreu precisamente quando ele buscava a hegemonia mundial. Assim, passando pelos turbulentos anos da Secessão e incorporando o espírito pragmático estadunidense cresceu e se firmou com sua pát...

  6. WITNESSING THE BIRTH OF THE RED SEQUENCE: ALMA HIGH-RESOLUTION IMAGING OF [C II] AND DUST IN TWO INTERACTING ULTRA-RED STARBURSTS AT z = 4.425

    International Nuclear Information System (INIS)

    Oteo, I.; Ivison, R. J.; Dunne, L.; Zhang, Z-Y.; Lewis, A.; Maddox, S.; Smail, I.; Swinbank, A. M.; Riechers, D.; Serjeant, S.; Werf, P. Van der; Biggs, A. D.; Bremer, M.; Cigan, P.; Eales, S.; Clements, D. L.; Cooray, A.; Dannerbauer, H.; Ibar, E.; Messias, H.

    2016-01-01

    Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Array, we have studied the morphology and the physical scale of the interstellar medium—both gas and dust—in SGP 38326, an unlensed pair of interacting starbursts at z = 4.425. SGP 38326 is the most luminous star bursting system known at z > 4, with a total IR luminosity of L IR ∼ 2.5 × 10 13 L ⊙ and a star formation rate of ∼ 4500 M ⊙ yr −1 . SGP 38326 also contains a molecular gas reservoir among the most massive yet found in the early universe, and it is the likely progenitor of a massive, red-and-dead elliptical galaxy at z ∼ 3. Probing scales of ∼0.″1 or ∼800 pc we find that the smooth distribution of the continuum emission from cool dust grains contrasts with the more irregular morphology of the gas, as traced by the [C ii] fine structure emission. The gas is also extended over larger physical scales than the dust. The velocity information provided by the resolved [C ii] emission reveals that the dynamics of the two interacting components of SGP 38326 are each compatible with disk-like, ordered rotation, but also reveals an ISM which is turbulent and unstable. Our observations support a scenario where at least a subset of the most distant extreme starbursts are highly dissipative mergers of gas-rich galaxies.

  7. Filosofía y exégesis en las Enéadas. Las alas del alma plotiniana en su lectura del Fedro platónico

    OpenAIRE

    Gabriel Martino

    2014-01-01

    “Philosophy and Exegesis in the Enneads. The Wings of the Plotinean Soul in his reading of Plato’s Phaedrus”. In the present paper, we examine the role exegesis plays in the philosophy of the Enneads and, in particular, the way in which Plotinus interprets Plato. With this purpose we analyze, in the first place, some revealing passages of Porphyrius’ Life of Plotinus in order to understand, on the one hand, how late Greek thinkers conceived the exegetic endeavour and, on the other hand, the w...

  8. Alma, corpo e a antiga civilização grega: as primeiras observações do funcionamento cerebral e das atividades mentais Soul, body and the ancient greek civilization: the first observations of brain functioning and mental activities

    Directory of Open Access Journals (Sweden)

    Fabiano S. Castro

    2011-01-01

    Full Text Available Muitos dos conceitos existentes na neurociência moderna possuem suas origens nas especulações elaboradas pelos antigos filósofos e médicos gregos. Questões centrais sobre a fonte dos pensamentos humanos, o mecanismo da atividade cognitiva, e a natureza das emoções, percepção e movimento voluntário, por exemplo, foram levantadas pelos pensadores gregos. É a partir desta civilização que surgem as observações mais sistemáticas sobre a estrutura e o funcionamento do corpo, da mente e a relação entre estas duas entidades. Assim, o presente trabalho pretende observar as principais tentativas iniciais gregas em vincular estruturas do corpo (tais como o cérebro ou o coração e atividades mentais, ao longo das diversas especulações gregas sobre a natureza, a filosofia, a psicologia e a medicina.Many of the existing concepts in modern neuroscience have their origins in the speculations made by ancient Greek philosophers and physicians. Core questions about the source of human thought, the mechanism of cognitive activity as well as the nature of emotions, perceptions and voluntary movements, for example, were raised by Greek thinkers. It is from this civilization that arise more systematic observations on the structure and functioning of body, mind and relationship between these two entities. The present paper intends to adhere to the first Greek attempts to link structures of the body (such as the brain or the heart and mental activities regarding various Greek speculations about the nature, philosophy, psychology and medicine.

  9. «Con llanto en los ojos, / con luto y duelo en el alma»: el moro como forjador identitario en la tradición dramática del levante peninsular

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    Sáez Raposo, Francisco

    2013-06-01

    Full Text Available The festival of Moors and Christians in the town of Caudete (Albacete, one of the oldest known, came into being within a dramatic tradition that goes back to the late Sixteenth Century. As a paradigmatic example of the dramatic creation process based on rewriting, the original play has been adapted to the audience’s ever changing horizons of expectations to constitute Episodios caudetanos, the core of nowadays celebration. History, religion, legend and literature complement each other in order to form a cultural phenomenon that transcends its mere playful essence as a popular festival. Through the archetypical figure of the moor, the identity of a community has been shaped (and, by extension, that of a whole nation from the concept of a polarized universe that historical documentation insists on denying.La fiesta de moros y cristianos de la villa albaceteña de Caudete, una de las más antiguas que se conocen, tiene su origen en una tradición dramática que se remonta a finales del siglo XVI. Ejemplo paradigmático del proceso de creación teatral basado en la reescritura, la obra primigenia se ha ido adaptando a los cambiantes horizontes de expectativas del público hasta conformar los Episodios caudetanos, médula de la actual celebración. Historia, religión, leyenda y literatura se complementan para configurar un fenómeno cultural que trasciende la mera esencia lúdica de un festejo popular. Mediante la figura prototípica del moro se ha moldeado la identidad de una comunidad (y, por extensión, de toda una nación a partir del concepto de un universo polarizado que la documentación histórica se empeña en refutar.

  10. TÜKETİCİDE SAĞLIĞINI KORUMA BİLİNCİ VE SATIN ALMA NOKTASINDA TÜKETİCİ TUTUMLARI:AMBALAJLI GIDA ÜRÜNLERİ ÜZERİNE BİR ARAŞTIRMA

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    İKBAL AKSULU

    2013-05-01

    Full Text Available Food products takes the priority in the consumer’s basic needs and their importance in the family purchasing budget varies according to their income level. It’s proportion to total expenditure goes up when it’s gone down to the lower income levels. On the other hands the consumption conscious of these products is increasingly rising as the education and income level increases. These trends closely affect the companies decisions on the products. In this study, it is tried to understand whether the consumer takes the decision on the consumption of food product, he or she is interested in nutrition value of the product, and how he she perceives the main product characteristics.

  11. «Cantaron desta suerte...». Functions of Music in the Mistery Play «Bodas entre el alma y el amor divino», by Lope de Vega, Religious Transposition of the Royal Weddings of 1599

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    María Asunción Flórez Asensio

    2013-05-01

    Full Text Available In 1599 Lope de Vega atended the festivities organised in Valencia to celebrate the double royal wedding between Felipe III and his sister Isabel Clara Eugenia with the Archdukes Margaret and Albert of Austria. This historical event was transformed into a religious occasion. This auto reflects a «divine» version of the facts. Included at the end of Book II of El peregrino en su patria, published five years later, this  auto (as well as the others included in the collection allow us to confirm not only that Lope uses music more in his mystery plays than in his comedies, but also that at this early time he had already started to experiment with a series of musical elements that, after being developed by Calderón, came to be characteristic of Spanish Golden Age theatre.

  12. Iraqi Perspectives Project Phase II. Um Al-Ma’arik (The Mother of All Battles): Operational and Strategic Insights from an Iraqi Perspective, Volume 1 (Revised May 2008)

    Science.gov (United States)

    2008-05-01

    against Israel. The Iraqis treated success, real or perceived, with a quixotic awe that placed lessons on this topic in a category all by themselves.949...Lon- don : Harper Collins, 1993 paperback edition. Defense Science Board Task Force. “The Role and Status of DoD Red Teaming Activities.” September...Khazraji, al-Hayah, (Ara- bic) London, 16 April 1996. (Open Source Center, FTS19960416000591) Oberdorfer, Don . “Glaspie Says Saddam is Guilty of

  13. De la sanidad del cuerpo a la sanidad del alma: estudio sobre la lógica de construcción de las identidades colectivas en el neo-pentecostalismo argentino

    Directory of Open Access Journals (Sweden)

    Joaquín Algranti

    2008-01-01

    Full Text Available No presente artigo, o autor se propõe a estudar em grandes traços a lógica de construção das identidades coletivas que se desenvolvem dentro dos grupos evangélicos neo- pentecostais. Para isso analisa a síntese entre religião, psicanálise e auto-ajuda que expressa o discurso de "sanidade interior", desenvolvido no marco de uma igreja evangélica, localizada em um setor de altos ingressos na Cidade de Buenos Aires, Argentina. A teoria da hegemonia de Ernesto Laclau lhe permite analisar o lugar que os significantes flutuantes ocupam no trabalho religioso de construir uma identidade ampla que se nutre de diferentes universos simbólicos no momento de interpelar os sujeitos a partir da teologia da sanidade.The aim of this paper is to study the construction's logic of collective identities within neo-pentecostals evangelic groups. In order to do this the author analyze the synthesis between religion, psychoanalysis and self-help therapy expressed in the discourse of "Inner Health" developed by an evangelic Church located in the center of a high income neighborhood in Buenos Aires city, Argentina. The Ernesto Laclau´s theory of hegemony allows him to analyze the function of floating signifiers in the religious task of creating a wide identity that assimilates elements of different symbolic universes when interpelling the subject through the theology of health.

  14. Joan Costa y Daniel Raposo. La rebelión de los signos. El alma de las letras : Editorial La Crujía, 2008, 159 páginas

    OpenAIRE

    Tram[p]as de la Comunicación y la Cultura

    2009-01-01

    Los signos son signos de cultura. Existen para cumplir una función propia y exclusiva: signifi car. Todo lo que signifi ca es signo. Este libro recoge las evoluciones de la letra desde el cuneiforme y el jeroglífi co hasta el alfabeto moderno, la imprenta y la tecnología digital. La rebelión de los signos revela su rica y apasionante vida y su infl uencia decisiva en el arte, el diseño, la comunicación y la cultura. (Párrafo extraído del texto a modo de resumen)

  15. The ALMA Frontier Fields Survey. III. 1.1 mm emission line identifications in Abell 2744, MACSJ 0416.1-2403, MACSJ 1149.5+2223, Abell 370, and Abell S1063

    Science.gov (United States)

    González-López, J.; Bauer, F. E.; Aravena, M.; Laporte, N.; Bradley, L.; Carrasco, M.; Carvajal, R.; Demarco, R.; Infante, L.; Kneissl, R.; Koekemoer, A. M.; Muñoz Arancibia, A. M.; Troncoso, P.; Villard, E.; Zitrin, A.

    2017-12-01

    Context. Most sub-mm emission line studies of galaxies to date have targeted sources with known redshifts where the frequencies of the lines are well constrained. Recent blind line scans circumvent the spectroscopic redshift requirement, which could represent a selection bias. Aims: Our aim is to detect emission lines present in continuum oriented observations. The detection of these lines provides spectroscopic redshift information and yields important properties of the galaxies. Methods: We perform a search for emission lines in the Atacama Large Millimeter/submillimeter Array observations of five clusters which are part of the Frontier Fields and assess the reliability of our detection. We additionally investigate plausibility by associating line candidates with detected galaxies in deep near-infrared imaging. Results: We find 26 significant emission lines candidates, with observed line fluxes between 0.2-4.6 Jy kms-1and velocity dispersions (FWHM) of 25-600kms-1. Nine of these candidates lie in close proximity to near-infrared sources, boosting their reliability; in six cases the observed line frequency and strength are consistent with expectations given the photometric redshift and properties of the galaxy counterparts. We present redshift identifications, magnifications, and molecular gas estimates for the galaxies with identified lines. We show that two of these candidates likely originate from starburst galaxies, one of which is a so-called jellyfish galaxy that is strongly affected by ram pressure stripping, while another two are consistent with being main sequence galaxies based in their depletion times. Conclusions: This work highlights the degree to which serendipitous emission lines can be discovered in large mosaic continuum observations when deep ancillary data are available. The low number of high-significance line detections, however, confirms that such surveys are not as optimal as blind line scans. We stress that Monte Carlo simulations should be used to assess the line detection significances since using the negative noise suffers from stochasticity and incurs significantly larger uncertainties.

  16. La puerta del alma: el color de ojos y de cabello como forma discursiva de dominación (The doors of soul: the color hairs and eyes as a discursive instrument of domination

    Directory of Open Access Journals (Sweden)

    Korstanje, Maximiliano

    2010-06-01

    Full Text Available Resumen: El nacimiento de un hijo es un evento único e irremplazable para todos aquellos que han tenido la experiencia. Para otros, es una oportunidad de asenso social sobre todo sí por ese juego de los genes la criatura se asemeja al estereotipo indoeuropeo nórdico. Por ese motivo, los padres parecen interesados en que sus hijos tengan ojos claros y cabellos rubios tomando esa característica como cualitativamente positiva. Por ese motivo, no resulta extraño que las diferentes imágenes en publicidades de artículos para bebes enfatice en los “ojos azules y los cabellos rubios” como tipos ideales a seguir. La presente investigación ha demostrado que no sólo que los estereotipos dominantes se multiplican sino también se interiorizan generando un diálogo que tiende a reforzar la hegemonía. Por lo demás, se ha observado que discursivamente la claridad es simbolizada como sinónimo de felicidad, armonía, afecto, bondad y seguridad entre otros mientras la oscuridad adquiere categorías semánticas opuestas. Para los padres, que sus hijos tengan ojos “claros” o cabellos “rubios” significa un verdadero asenso social abstracto. Por lo pronto, no cobrarán un canon adicional por traer a la vida a un hijo rubio, pero los acerca notablemente más a las características de los grupos dominantes reforzando así el auto-desprecio por sí mismos.Abstract: Even a memorable moment as the birth of a son can be subject to a much broader pervasive experience. For some people, this event become in an opportunity to social upward wherein convergence genetic and eugenicist thoughts with concentration in Norse phenotype. For that reason, parents are concerned in their sons have bight eyes and blondes hairs. This is based on the postmodern advertising and marketing efforts to emphasize on these features. Under this context, this present research showed not only that dominant phenotypes are divulged thanks to the advertising but also create a bridge between the hegemony and sentiment of inferiority. Discursively, parents who had children with bright eyes will be paid of an additional Fee, this represents a sociological and psychological need for social upward. This issue reflects that they are hermeneutically close-up to dominant elites.

  17. Deducción de una ecuación simple para el voltaje rectifcado faradaico

    Directory of Open Access Journals (Sweden)

    M. Grajales T.

    2010-06-01

    Full Text Available Usando la ecuación general de Butler-Vohner se dedujo una ecuación simple para el voltaje rectificado con control de corriente senoidal en el potencial de equilibrio. La ecuación fue derivada en términos de los coeficientes de transferencia anódico y catódico y es aplicable en condiciones de total control por transferencia de carga. Se probó que la ecuación deducida por Doss y Agarwal a bajas frecuencias es un caso particular de nuestra ecuación, cuando se aplica a reacciones electroquímicas de un solo paso. Se examinaron también sus implicaciones.

  18. Sistema de modulación de ancho de impulso para el control de potencia alterna monofásica

    OpenAIRE

    Valla, María Inés; Rivetta, Claudio H.

    1987-01-01

    La modulación de ancho de impulsos (PWM) es ampliamente utilizada en el control de inversores. El principal objetivo es lograr una tensión senoidal da salida con mínima distorsión armónica. En el presente trabajo se describe un inversor monofásico de simple implementación, cuyo control presenta la característica inherente de mantener la relación de tensión a frecuencia fundamental de salida (V/f) constante y un mínimo contenido armónico espúreo en un amplio rango de frecuencia de referencia. ...

  19. Determinação de sulfonamidas no mel por um método de HPLC-fluorescência

    OpenAIRE

    Correia, Daniela M.; Vilas-Boas, Miguel; Peres, António M.; Dias, L.G.

    2007-01-01

    O mel e um produto natural pelo que a sua comercialização está sujeita a Legislação Europeia, que proíbe s sua comercialização na presença de quaisquer resíduos de antibióticos. O mel é um produto natural e a sua comercialização está sujeita à Legislação Europeia, que proíbe a sua comercialização na presença de quaisquer resíduos de antibióticos. Os antibióticos são usados no tratamento de abelhas com o intuito de combater infecções associadas às doenças da Loque Americana e Loque...

  20. Descrição de uma nova espécie de Thamnodynastes Wagler, 1830 (Serpentes, Colubridae do nordeste brasileiro, com comentários sobre o gênero.

    Directory of Open Access Journals (Sweden)

    Francisco L. Franco

    2002-12-01

    Full Text Available Thamnodynastes almae sp. nov. is described based on three specimens from Rodelas municipality, state of Bahia, Northeastern Brazil. The new species can be diagnosed by its pale coloration and keeled dorsal scales arranged in 19 rows at midbody and 15 rows posteriorly. Characters for distinguishing T. almae from other brazilian species of Thamnodynastes are provided.

  1. El pensar en la filosofía de la mente de L. Wittgenstein

    OpenAIRE

    Gil-de-Pareja, J.L. (José Luis)

    1988-01-01

    Wittgenstein; filosofía contemporánea; filosofía de la mente; cartesianismo; dualismo; cercanía de la concepción del alma de Wittegenstein con la concepción del alma de Platón como "afinidad con las Formas".

  2. À Sua imagem e semelhança : o misticismo judaico na Antiguidade tardia e a percepção do corpo nas literaturas apocalíptica e hekhalot

    OpenAIRE

    Ramos, Marcus Vinicius

    2011-01-01

    Corpo e alma constituíam, nas Escrituras, uma unidade de personalidade e um único conceito, contrariando a percepção largamente aceita no mundo grego que distinguia o corpo, mortal, de sua alma imortal. Essa dissertação avalia a percepção da unidade entre corpo e alma no período intertestamental, quando a Palestina esteve sob forte influência helenística. São utilizados como fontes os textos apocalípticos de Enoch e a literatura hekhalot. As associações entre as funções fisiológicas e psicoló...

  3. THE HORTON-STRAHLER RIVER ORDER IMPLEMENTATION RELEVANCE WITHIN THE ANALYSIS OF THE ALMAŞ BASIN RELIEF

    OpenAIRE

    MĂDĂLINA-IOANA RUS; I. A. IRIMUŞ

    2014-01-01

    The Horton-Strahler River Order Implementation Relevance within the Analysis of the Almaș Basin. The purpose of the present study/research aims at underlining the importance of the enforcement of the river order within the analysis of the Almaș basin relief. The topic was chosen based on the fact that the hydrographic networks hierarchy offers at the same time quality and quantity information, on the relief evolution tendency and also the chance to compare the Almaș tributary sub-basins ones ...

  4. Close to the Sky

    Science.gov (United States)

    2007-11-01

    Today, a new ALMA outreach and educational book was publicly presented to city officials of San Pedro de Atacama in Chile, as part of the celebrations of the anniversary of the Andean village. ESO PR Photo 50a/07 ESO PR Photo 50a/07 A Useful Tool for Schools Entitled "Close to the sky: Biological heritage in the ALMA area", and edited in English and Spanish by ESO in Chile, the book collects unique on-site observations of the flora and fauna of the ALMA region performed by experts commissioned to investigate it and to provide key initiatives to protect it. "I thank the ALMA project for providing us a book that will surely be a good support for the education of children and youngsters of San Pedro de Atacama. Thanks to this publication, we expect our rich flora and fauna to be better known. I invite teachers and students to take advantage of this educational resource, which will be available in our schools", commented Ms. Sandra Berna, the Mayor of San Pedro de Atacama, who was given the book by representatives of the ALMA global collaboration project. Copies of the book 'Close to the sky' will be donated to all schools in the area, as a contribution to the education of students and young people in northern Chile. "From the very beginning of the project, ALMA construction has had a firm commitment to environment and local culture, protecting unique flora and fauna species and preserving old estancias belonging to the Likan Antai culture," said Jacques Lassalle, who represented ALMA at the hand-over. "Animals like the llama, the fox or the condor do not only live in the region where ALMA is now being built, but they are also key elements of the ancient Andean constellations. In this sense they are part of the same sky that will be explored by ALMA in the near future." ESO PR Photo 50c/07 ESO PR Photo 50c/07 Presentation of the ALMA book The ALMA Project is a giant, international observatory currently under construction on the high-altitude Chajnantor site in Chile

  5. Desenvolvimento e avaliação de um protótipo de cortador de base para colhedoras de cana-de-açúcar Development and evaluation of a prototype of base cutter for sugar-cane harvesters

    Directory of Open Access Journals (Sweden)

    Carlos E. S. Volpato

    2002-01-01

    Full Text Available Um protótipo de cortador de base para o seguimento pantográfico do perfil em colhedoras de cana-de-açúcar, foi projetado e construído e seu desempenho de flutuação foi avaliado em função da força normal de reação do perfil (F N. O trabalho foi conduzido em uma caixa de solo, o protótipo montado sobre um carro porta-ferramentas e submetido a ensaios nos quais variaram três tipos de perfil: senoidal, rampa ascendente e rampa descendente, duas amplitudes do perfil, 0,025 e 0,05 m e cinco velocidades de deslocamento: 0,69, 1,12, 1,48, 1,82 e 2,12 m s-1. Os melhores resultados foram verificados para os perfis em rampa, tanto ascendente quanto descendente, independentemente da amplitude do perfil e da velocidade de deslocamento e, também, para perfil senoidal de ambas as amplitudes, com velocidade de deslocamento inferior a 1,48 m s-1. Os resultados demonstraram que o protótipo ainda é passível de ajustes, uma vez que o desempenho de flutuação sobre o perfil pode ser melhorado através da utilização de técnicas de otimização.A prototype of base cutter for sugar-cane harvester was designed and built. The floating performance was evaluated as a function of the profile reaction force (F N. The prototype was tested in a soil box using a carrier car running on sinusoidal and ramp type profiles with amplitudes of 0.025 and 0.05 m. The travel speeds used were of five different levels: 0.69, 1.12, 1.48, 1.82 and 2.12 m s-1. The best results were obtained while running on ramp profiles, both ascending or descending, independent of the profile amplitude or the travel speed. The sinusoidal profile showed good results for the travel speed of 1.48 m s-1, for both the amplitudes tested. The results demonstrated that the prototype may still be adjusted, as the floating action on the profile can be improved through the use of optimization techniques.

  6. Marka Güveni ve Marka Bağlılığının Satın Alma Niyeti Üzerine Etkisi: Akıllı Telefon Pazarında Bir Araştırma

    Directory of Open Access Journals (Sweden)

    Mehmet Sağlam

    2016-10-01

    Full Text Available This research aims to analyze the effect of brand trust and brand loyalty to consumer purchase intentions in the Smartphone market. All the residents of İstanbul who use mobile phones are the population of the research. Due to the fact that it is very hard to reach all the population, simple sampling method has been used for data collection and 185 participants have been reached. Structural Equation Model has been used to explain the relationship among brand trust, brand loyalty and purchase intentions. SPSS for Windows 17.0 program and AMOS 20 program are used to analyze the data. Results show that both brand trust and brand loyalty have a positive effect on consumer’s purchase intentions. Also it had been determined that brand trust has a positive effect on brand loyalty. Moreover, brand trust has been found as the most effective factor for smartphones brands in the purchase intensions.

  7. Alimentos, palavras e saúde (da alma e do corpo, em sermões de pregadores brasileiros do século XVII Food, words, and health (of soul and body in sermons by seventeenth-century preachers in Brazil

    Directory of Open Access Journals (Sweden)

    Marina Massimi

    2006-06-01

    Full Text Available Este artigo analisa alguns sermões pregados entre os séculos XVII e XVIII no Brasil, baseados em metáforas alimentares. O uso das metáforas, recorrente nos sermões do período colonial, fundamenta-se em dois alicerces: 1 na teoria aristotélica do conhecimento, em que o sensorial ocupa um papel prioritário, como porta de acesso para a compreensão das idéias mais abstratas e para a mobilização dos afetos e da vontade visando à modificação do comportamento dos ouvintes; 2 na doutrina platônica sobre a importância das imagens para conservar a memória das idéias. A oratória sagrada do período desperta interesse para a história cultural, uma vez que os sermões constituíram-se numa importantíssima fonte de transmissão de doutrinas e de modelagem dos comportamentos numa sociedade em que a oralidade era a principal forma de difusão dos conhecimentos.The article analyzes a number of sermons employing food metaphors, preached in Brazil during the seventeenth and eighteenth centuries. The use of metaphors drawn from listeners' daily lives was common in sermons during the colonial period, underpinned by two theoretical considerations: 1 the Aristotelian theory of knowledge, where the senses play a primary role as an access way to comprehension of more abstract ideas and as a means for urging listeners to change their behavior patterns by affecting their emotions and their wills; 2 the Platonic doctrine, where images are important in preserving our memory of ideas. The sacred oratory of the colonial period is of major interest to cultural history, since these sermons served as an invaluable way of transmitting doctrine and of shaping behavior in a society where orality was the chief method for spreading knowledge.

  8. Nesnel ve Öznel Bilginin Tüketicilerin Satın Alma Davranışlarına Etkisine Yönelik Bir Araştırma(An Investigation of The Effect of Objective and Subjective Knowledge on Consumers’ Buying Behaviour

    Directory of Open Access Journals (Sweden)

    Kalender Özcan ATILGAN

    2014-12-01

    Full Text Available In the growing body of marketing literature on the impact of consumer knowledge on intention to buy, distinction between subjective and objective knowledge has clearly been made. The difference between subjective and objective knowledge may be due to both the definition and measurement process. The goal of this research is to examine the impact of both subjective and objective knowledge related to attitude to and intention to buy light milk and dairy products. Data were gathered via face-to-face survey from 330 consumers living in Erdemli district of Mersin, Turkey. A Hybrid Path Analysis was performed to test the hypothesis. The results of Structural Equations Modelling clearly indicate that subjective knowledge and health consciousness are positively associated with attitude towards light milk and dairy products and objective knowledge is negatively associated with attitude towards light milk and dairy products. Also, attitude towards light milk and dairy products is positively associated with intention to buy these products. Implications and suggestions are developed based on the structural model for future researches.

  9. Aile Değerleri ve Dindarlığın Plansız Satın Alma Eğilimi Üzerine Etkilerine Yönelik Bir Yapısal Eşitlik Modeli (A Structural Equation Model on the Effects of Family Values and Religiosity toward Impulse Buying Tendency

    Directory of Open Access Journals (Sweden)

    Aybegüm GÜNGÖRDÜ

    2016-03-01

    Full Text Available The purpose of this study is to measure the effects of family values and religiosity on impulse buying tendency. Our sample consists of 250 consumers. According to the frequency analysis, the sample represents the new middle class consumers who are mostly young, well educated urbanites and white collar professionals. We used reliability and validity analyses, exploratory and confirmatory factor analyses, descriptive statistics, Pearson correlation analysis and structrual equation modelling. Finally, there is a negative and significant relationship between consumers’ religiosity and their impulse buying tendency. Furthermore, there is a positive and significant relationship between consumers’ religiosity and their family values.

  10. Reklamların ve Cinsiyet Kimliği Rolünün Tüketicilerin Satın Alma Davranışları Üzerindeki Etkisi = The Effect of Advertisements and Gender Identity Role on Consumer Buying Behavior

    Directory of Open Access Journals (Sweden)

    Mehmet İsmail YAĞCI

    2010-01-01

    Full Text Available Gender is a segmentation criterion which has been used for a long time especially for the analyses of consumer behavior in traditional marketing. However an obligation has aroused to digress the traditional patterns in order to understand consumer behavior in our rapidly changing world. At this point, “gender identity role” concept which is frequently encountered in the literature reminded may help researchers in understanding complex consumer buying behavior. In this study, consumer’s gender identity’s impact on their response to advertisements and whether their socio-economic status levels’ effect their gender identities or not have been analyzed and some significant relations have been found.

  11. COMENTARIO DEL LIBRO Ronny J. Viales y Andrea M. Montero, La construcción sociohistórica de la calidad del café y del banano de Costa Rica. Un análisis comparado 1890-1950: San José: Alma Máter, 2010.

    Directory of Open Access Journals (Sweden)

    Carlos Izquierdo Vázquez

    2014-12-01

    Full Text Available El artículo comenta el libro acerca de la construcción sociohistórica de la calidad del café y el banano en Costa Rica durante el periodo 1890-1950, considerando que la calidad de un producto es relativa en el tiempo y que esta va más allá de los procesos técnicos, tecnológicos y agroecológicos. Esto significa que hay una dimensión cultural en cuanto a cómo se construye históricamente la calidad. Así, comparativamente se estudiaron diversas variables y actores que incidían en el proceso. Mediante un novedoso análisis, a través de una amplia diversidad de fuentes, el libro constituye un aporte fundamental para la historia económica, pero también para la historia ambiental, en el contexto de nuevas líneas de investigación, al trascender el análisis centrado en los procesos productivos y tomar en cuenta las prácticas culturales.

  12. Kamusal Karar Alma Süreçlerinde Sosyal Tercih Duyarlılığı ve Sürece İlişkin Yapısal Çözümlemeler(The Sensitivity of Social Preferences in Public Decisions Making Process and The Structural Analyses Connected with The Process

    Directory of Open Access Journals (Sweden)

    A. Niyazi ÖZKER

    2014-06-01

    Full Text Available In the study, we aim to bring up the social preferences location that have an important influence on the components of process consisting of social-economics together with the dynamics which should be considered by decision makers as the balanced component between the central government characteristics and the social preferences in public decision making process. Also, the dynamics’ negative effects as under approaches management of central governments’ politic strategies on the socially choices by taking shape publically point of view have been aimed to analyze connected with participation process. Hence, it is appear that the decisions’phenomenon directed towards to analyzes appear in very important the structural models in order to ensure the desired reality participation in decision making and also, the provided participation sensitive that lay the gramework for overtaking some paradox related to decision making process must be required to take into consideration and and check over as the primary point especially in the countries that have the structural politics matters.

  13. Nesnel ve Öznel Bilginin Tüketicilerin Satın Alma Davranışlarına Etkisine Yönelik Bir Araştırma(An Investigation of The Effect of Objective and Subjective Knowledge on Consumers’ Buying Behaviour)

    OpenAIRE

    Kalender Özcan ATILGAN

    2014-01-01

    In the growing body of marketing literature on the impact of consumer knowledge on intention to buy, distinction between subjective and objective knowledge has clearly been made. The difference between subjective and objective knowledge may be due to both the definition and measurement process. The goal of this research is to examine the impact of both subjective and objective knowledge related to attitude to and intention to buy light milk and dairy products. Data were gathered via face-to-f...

  14. TÜKETİCİLERİN SATIN ALMA DAVRANIŞLARI ÜZERİNDE SOSYOLOJİK FAKTÖRLERİN ETKİSİNİN İNCELENMESİNE YÖNELİK AMPİRİK BİR ÇALIŞMA

    OpenAIRE

    DURMAZ, Yakup; BAHAR(ORUÇ), Reyhan

    2014-01-01

    Abstract In the modern world where the concept of communication, changes and innovation have become more and more important many companies have begun to focus on consumers. Business strategies and activities are planned according to consumer behavior. Marketing science communicates face to face with people. From this point of view, marketers has to know the consumers better in order to make different more than their competitors and be successful in the market. It is known that the family ...

  15. El alma de las muñecas. Sobre la construcción de un cuerpo simbólico a través de una dialéctica del simulacro en la novela Érase una vez el amor, pero tuve que matarlo de Efraím Medina

    OpenAIRE

    Camargo, María José

    2013-01-01

    En este ensayo se propone trabajar la muñeca como tópico para entender los diferentes desplazamientos, a través de los cuales el personaje de Rep en la novela Érase una vez el amor, pero tuve que matarlo de Efraím Medina, construye el elemento cierta chica como disposotivo de construcción estética, que posibilita la economía de un cuerpo deseante como socialización artística.

  16. Cumhuriyet İdaresi'nin Nüfusu Kayıt Altına Alma Girişimlerine Bir Örnek: 1934 Yılı Nüfus Taraması
    An Illustration For The Civil Registry Processes During The Republican Era: The Census Of 1934

    OpenAIRE

    Fevzi ÇAKMAK

    2013-01-01

    It’s widely known about the Ottoman State that, rather thanapplying a well-organized population policy; until the final periods of thestate, it was preferred to collect statistical data of population andproperties particularly to provide military needs and tax for the state.The organization, responsible to coordinate the population affairs, wasfirstly established during the modernization phase of the OttomanState, which began with Tanzimat Reform. The causes drifting the stateinto the collaps...

  17. Cumhuriyet İdaresi'nin Nüfusu Kayıt Altına Alma Girişimlerine Bir Örnek: 1934 Yılı Nüfus Taraması An Illustration For The Civil Registry Processes During The Republican Era: The Census Of 1934

    Directory of Open Access Journals (Sweden)

    Fevzi ÇAKMAK

    2013-09-01

    Full Text Available It’s widely known about the Ottoman State that, rather thanapplying a well-organized population policy; until the final periods of thestate, it was preferred to collect statistical data of population andproperties particularly to provide military needs and tax for the state.The organization, responsible to coordinate the population affairs, wasfirstly established during the modernization phase of the OttomanState, which began with Tanzimat Reform. The causes drifting the stateinto the collapse in the following era proved to be more crucial than theapplication of a sound population policy.The new Republican state, established after the War ofIndependence, inherited absolutely unfavorable conditions of populationaffairs from the prior civil organization. The long warfare, theimpossibilities emerging as a result of wars, the internal and externalpopulation movements, the deaths, the births and the negativereactions of the people on population affairs had posed an obstacle forcollecting reliable data for the civil registries in a long course of time.The situation was that thousands of new-born babies weren’t registered;other thousands of dead people were indicated as alive on civilregistries. Furthermore, whereas many thousands of married peopleseemed still single, other some thousands were married according to theregistry. Under those circumstances, the principal matter on whichTurkish Republic emphasized on was the population policy. There weretwo essential pillars of the population policy, attempted to be applied bythe state. One of them was in general to prevent the decrease in thepopulation and to take the steps to increase the population; anotherwas to register the population in terms of quality and quantity.Within the scope of this study, the efforts of the Republicangovernment to register the concealed population as an essential part ofthe policy of population registration will be pointed out. Especially,having encountered the fact that great portion of the populationremained concealed following the census of 1927, the governmentsought to make various amnesty regulations related to the civil registry.After the law was enacted, the people rushed to civil register offices andwith the great demand of the public, the government sought for asolution. The final solution was to assign all public officers that were infield service and available to take in charge, to civil registrationprocedures. Through the ordinance, made for this aim in March 1934, arapid success was attained and then through the Law related toRegistration of Concealed Population, which was made in July 1934,the legal basis of the mechanism was founded. Within the scope of thisstudy, the mechanism mentioned will be sought to be analyzed. Thefundamental reference for our study will be the civil registry books. Osmanlı Devleti’nin son dönemlerine kadar düzenli bir nüfus siyaseti yerine, daha çok vergi ve askeri ihtiyaçlarını karşılamaya yönelik nüfus ve arazi istatistikleri tuttuğu bilinmektedir. Nüfus işlerini düzenlemekle görevli teşkilat Osmanlı devletinin Tanzimat’la başlayan modernleşme döneminde oluşturulmaya başlanmıştır. Sonraki dönemde devleti çöküşe götüren nedenler, sağlıklı bir nüfus siyaseti yürütülmesinin önüne geçmişti.Bağımsızlık Savaşı vererek kurulan yeni Cumhuriyet idaresi, nüfus işleri bakımından eski idareden son derece kötü bir miras devralmıştı. Uzun süren savaşlar, savaşlarla birlikte ortaya çıkan imkânsızlıklar, ülke içine ve dışına yönelik nüfus hareketleri, ölümler, doğumlar ve halkın nüfus işlerine yönelik olumsuz tavrı, nüfus kütüklerinin uzun yıllar doğru bir şekilde tutulması önünden engel teşkil etmişti. Binlerce doğum kayıt altına alınmamışken, binlerce ölü sicillerde sağ görünmekte; binlerce evliler defterlerde bekâr, binlerce boşanmış kütüklerde evli görünüyordu. Bu şartlar altında Türkiye Cumhuriyeti’nin önemle üzerinde durduğu konuların başında, Nüfus siyaseti geliyordu. Devletin uygulamaya çalıştığı nüfus siyasetinin iki önemli ayağı bulunuyordu. Bunlardan biri genel olarak nüfusun azalmasını önlemek ve artmasına yönelik tedbirler almak, diğer ayağı ise nüfusun nitelik ve nicelik olarak kayıt altına alınmasıydı.Bu çalışmada Cumhuriyet idaresinin nüfusu kayıt altına almaya yönelik siyasetin önemli bir parçası olan gizli nüfusların yazımına yönelik çabalarına değineceğiz. Özellikle 1927 nüfus sayımı sonrası pek çok nüfusun saklı kaldığı gerçeği karşısında devlet, nüfus kayıtlarına yönelik çeşitli af düzenlemelerine gidecekti. 1933 yılında çıkarılan Af Kanunu içinde, nüfus kayıtlarının affına dair hükümler bulunuyordu. Kanun sonrası halk, nüfus dairelerine koşarken, devlet karşı karşıya kaldığı yoğun talep karşısında çıkış çareleri arayacaktı. Bulunan çıkış yolu, nüfus kayıt işlemlerinde, taşrada görev yapan, durumu görev almaya müsait olan tüm devlet memurlarının kullanılmasıydı.1934 yılının Mart ayında bu yönde çıkarılan talimatname ile kısa sürede başarı yakalanmış ve ardından 1934 yılının Temmuz ayında çıkarılan Gizli Nüfusların Yazımına ilişkin kanunla, işleyişin yasal dayanakları oluşturulmuştu. Buradaki çalışmamızda, sözü edilen işleyişi tahlil etmeye çalışacağız. Çalışmamıza nüfus kayıt defterleri temel kaynak teşkil edecektir.

  18. Plaadid / Valner Valme

    Index Scriptorium Estoniae

    Valme, Valner, 1970-

    2003-01-01

    Uutest plaatidest Stereolab "Instant O In The Universe", Masters Of Gregorian Chant "Chapter IV", R.E.M. "In Time. The Best Of R.E.M.", Celia Cruz "Regalo de alma", John Mayer "Heavier Things", Dayampert "Shapes & Colors"

  19. Science with the Atacama Large Millimeter Array A New Era for Astrophysics

    CERN Document Server

    Bachiller, Rafael

    2008-01-01

    Currently under construction in the Andean Altiplano, Northern Chile, the Atacama Large Millimeter Array (ALMA) is the most ambitious astronomy facility under construction. ALMA is a radio interferometer composed of 54 antennas of 12 m diameter, and twelve 7 m antennas with about 6600 square meters of total collecting area. Initially covering the most interesting spectral wavelength ranges from 3 to 0.3 mm, ALMA will be a revolutionary telescope aimed to unveil the details of star and planet formation and to provide astronomy with the first exhaustive view of the dark and youngest objects of the Universe. This book describes the enormous capabilities of ALMA, the state of the project, and most notably the scientific prospects with such a unique facility. The book includes comprehensive reviews and recent results on most hot topics of modern Astronomy (the formation and evolution of galaxies, the physics and chemistry of the interstellar medium, and the processes of star and planet formation) with prospects to...

  20. A drone flight over ESO’s experimental sites in Chile

    CERN Multimedia

    CERN Bulletin

    2015-01-01

    Paola Catapano, a member of CERN’s Communication Group, and Mike Struik, a member of the TE Department, were invited to visit ESO’s experimental sites – the ALMA observatory and the Very Large Telescope in Paranal, Chile. Enjoy some of the beautiful images they sent to the Bulletin.   Image courtesy Paola Catapano and Mike Struik. The 66 radio astronomy antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) observatory at 5,000 m altitude on the Chajnantor highland in Chile. The ALMA array specialises in the cold, invisible Universe, catching radiation from millimetre and submillimetre radiowaves night and day. ALMA is an international partnership between the European Southern Observatory (ESO), the US National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan, together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile.   Image cour...

  1. Üks päev Kolumbia lastekodus / Siiri Liiva

    Index Scriptorium Estoniae

    Liiva, Siiri

    2009-01-01

    Puka Avatud Noortekeskuse noorsootöötaja Siiri Liiva kirjutab šokeerivatest ja rõõmsatest kogemustest, mida on pakkunud töö vabatahtlikuna Kolumbia organisatsiooni Proyecto Alma de Nino lastekodus

  2. Postal enviada desde Paris, de Fernando Arrabal a Jesús Arcensio

    OpenAIRE

    Arcensio, Jesús, 1911-1992

    2012-01-01

    Texto de la postal: Querido poeta. Solo dos letras para decirte que tus versos me han llegado al alma. Me encantaría poder tener el honor de presentarlos. Espero tus noticias. Un abrazo muy cordial. F. Arrabal

  3. 100 History-Making Ethnic Women

    Science.gov (United States)

    York, Sherry

    2004-01-01

    A list of hundred history-making ethnic women who have created history in their respective fields and become successful writers is presented. The list includes Alma Flor Ada, Julia Alvarez and Oprah Winfrey.

  4. Know Stroke: Know the Signs, Act in Time Video

    Medline Plus

    Full Text Available ... you need to do is get to a hospital as quickly as possible. Every minute counts. When ... strokes. Alma Shanley: "He made it to the hospital, I would say, in probably 25 minutes from ...

  5. Chrysler's Iacocca, Class of '45, Brings Verve to Lehigh U. Fund-Raising Drive.

    Science.gov (United States)

    Bailey, Anne Lowrey

    1987-01-01

    Lee Iacocca is steering his alma mater's drive to raise money to develop a facility for linking the university's two campuses, housing programs on regional and national economic development, and establishing an institute for research on economic competitiveness. (MSE)

  6. Introduction

    Science.gov (United States)

    de Graauw, T.

    2010-09-01

    As this editorial is written, we have seven antennas at the Chajnantor plateau, the "High Site". Seven antennas means twenty-one baselines, i.e. more than twice as many as we had only two months ago. As you know, the bonus we have in interferometry is that the the number of baselines increases roughly with the square of the available antennas. The image quality can be further enhanced, because the projection of a celestial source onto the existing baselines changes due to the rotation of the Earth. A large number of baselines is important but not sufficient to fulfill one important promise of ALMA, namely to provide crisp images. Unlike the sharp images from the Hubble Space Telescope, images from ground based optical or radio telescopes are blurred by the Earth's atmosphere. It is the Holy Grail of observing astronomy to overcome such atmospheric effects. Recently, ALMA has made a big step toward this goal by using Water Vapor Radiometers operating at 183 GHz to measure the amount of atmospheric water vapor at any instant in the line of sight of each antenna, and applying a corresponding correction to the astronomical data received. This not only improves the image quality, it is essential for using ALMA at its lowest wavelengths of around 0.3mm and at baselines exceeding several kilometers. Achieving this has a been a collaborative effort involving many parts of the project and there are all to be congratulated. JAO has now moved into our new Santiago Central Office in Vitacura next to the ESO premises, ending a phase of two years were Santiago based staff was distributed in two different buildings. This new ALMA office will also host the ALMA archive. Although ALMA users are normally not expected to come to Chile to observe, there will be office space for visitors, since ALMA has been and will always be a cooperation of people from many countries and many fields of science and engineering. This newsletter contains a list of workshops, schools and conferences

  7. O estresse salino afeta o crescimento e o equilíbrio entre compostos ...

    African Journals Online (AJOL)

    Alide Mitsue Watanabe Cova

    2016-10-26

    Oct 26, 2016 ... 1Centro de Ciências Agrárias, Ambientais e Biológicas, Universidade Federal do Recôncavo da Bahia, Cruz das Almas,. 44380, BA, Brasil. 2Centro de Ciências Exatas e Tecnológicas, Universidade Federal do Recôncavo da Bahia, Cruz das Almas, 44380,. BA, Brasil. Received 1 August 2016, Accepted ...

  8. The VLA view of the HL Tau Disk - Disk Mass, Grain Evolution, and Early Planet Formation

    OpenAIRE

    Carrasco-Gonzalez, Carlos; Henning, Thomas; Chandler, Claire J.; Linz, Hendrik; Perez, Laura; Rodriguez, Luis F.; Galvan-Madrid, Roberto; Anglada, Guillem; Birnstiel, Til; van Boekel, Roy; Flock, Mario; Klahr, Hubert; Macias, Enrique; Menten, Karl; Osorio, Mayra

    2016-01-01

    The first long-baseline ALMA campaign resolved the disk around the young star HL Tau into a number of axisymmetric bright and dark rings. Despite the very young age of HL Tau these structures have been interpreted as signatures for the presence of (proto)planets. The ALMA images triggered numerous theoretical studies based on disk-planet interactions, magnetically driven disk structures, and grain evolution. Of special interest are the inner parts of disks, where terrestrial planets are expec...

  9. Military Standard Transportation and Movement Procedures. Volume 1. Change 5

    Science.gov (United States)

    1994-08-12

    DCMINGO SDQ AWAN ADH ALMA ATA ALA EASTER ISLAND ANDER4A AW EASTER IS, MATAVERI INTL AP IPC ANAPA AAQ ARFBANGELSK ARM ECUADOR ASHKHABAD ASB AMBATO, CRACHOAN...ESK MONTEVIDEO, CARRASCO AIRPORT MVD ISTANBUL, ATATURK AIRPORT IST ZBR - ADNAN M ADB VANLTATA IZMIR, CIGLI MILITARY AIRPORT IGL AWIzTY AUY KAYSER ASR...MYANMAR AMZ ARDMORE, NEW ZEALAND ALA ALMA ATA, CIS ANA ANAHEIM, CA ALB ALBANY, NEW YORK, USA ANB ANNISTON, ALABAMA, USA ALC ALICANTE, SPAIN ANC

  10. Wood liquefaction and its application to Novolac resin

    Science.gov (United States)

    Hui Pan; Chung-Yun Hse; Todd F. Shupe

    2009-01-01

    Wood liquefaction was conducted using phenol as a reagent solvent with a weak acid catalyst in two different reactors: (Alma et al., 1995a.) an atmospheric glass reactor and (Alma et al., 1995b.) a sealed Parr® reactor. Residues were characterized by wet chemical analyses, Fourier transform infrared (FT-IR) spectroscopy, and X-ray diffraction (XRD). The FT-IR...

  11. The CASA Software Package

    Science.gov (United States)

    Petry, Dirk

    2018-03-01

    CASA is the standard science data analysis package for ALMA and VLA but it can also be used for the analysis of data from other observatories. In this talk, I will give an overview of the structure and features of CASA, who develops it, and the present status and plans, and then show typical analysis workflows for ALMA data with special emphasis on the handling of single dish data and its combination with interferometric data.

  12. The Antenna Bride and Bridegroom

    Science.gov (United States)

    2007-03-01

    ALMA Achieves Major Milestone With Antenna-Link Success The Atacama Large Millimeter/submillimeter Array (ALMA), an international telescope project, reached a major milestone on 2 March, when two 12-m ALMA prototype antennas were first linked together as an integrated system to observe an astronomical object. "This achievement results from the integration of many state-of-the-art components from Europe and North America and bodes well for the success of ALMA in Chile", said Catherine Cesarsky, ESO's Director General. ESO PR Photo 10/07 ESO PR Photo 10/07 The Prototype Antennas The milestone achievement, technically termed 'First Fringes', came at the ALMA Test Facility (ATF), located near Socorro in New Mexico. Faint radio waves emitted by the planet Saturn were collected by two ALMA prototype antennas, then processed by new, high-tech electronics to turn the two antennas into a single, high-resolution telescope system, called an interferometer. The planet's radio emissions at a frequency of 104 gigahertz were tracked by the ALMA system for more than an hour. Such pairs of antennas are the basic building blocks of the multi-antenna imaging system ALMA. In such a system, the signals recorded by each antenna are electronically combined with the signals of every other antenna to form a multitude of pairs. Each pair contributes unique information that is used to build a highly detailed image of the astronomical object under observation. When completed in the year 2012, ALMA will have 66 antennas. "Our congratulations go to the dedicated team of scientists, engineers and technicians who produced this groundbreaking achievement for ALMA. Much hard work and many long hours went into this effort, and we appreciate it all. This team should be very proud today," said NRAO Director Fred K.Y. Lo. "With this milestone behind us, we now can proceed with increased confidence toward completing ALMA," he added. ALMA, located at an elevation of 5,000m in the Atacama Desert of

  13. Calculation of the electromagnetic fields in electric machines through the use of the finite element. Algorithms for the solution of induction problems. Pt. 3; Calculo de campos electromagneticos en maquinas electricas mediante elemento finito. Algoritmos para la solucion de problemas de induccion. Pt. 3

    Energy Technology Data Exchange (ETDEWEB)

    Rosales, Mario F. [Instituto de Investigaciones Electricas, Cuernavaca (Mexico)

    1988-12-31

    This article is based in the electromagnetic modeling presented in the first part of the series for the indirect solution of partial differential equations. Magnetic systems in closed regions with moving or axial symmetry, whose total current density is partially known (induction problems) are considered. Includes the ability to deal with means in movement and a sinusoidal behavior for the source density current is assumed. Some algorithms are developed that are implanted in the software CALIIE-2D of the Instituto de Investigaciones Electricas (IIE) to obtain the numerical solutions of these problems. The basic systems of algebraic equations are obtained through the application of the Galerkin method in the discreteness of the finite element with first order triangular elements. [Espanol] Este articulo se basa en la modelacion electromagnetica presentada en la primera parte de la serie y en el planteamiento proporcionado en la segunda parte para la solucion indirecta de ecuaciones diferenciales parciales. Se consideran sistemas magneticos en regiones cerradas con simetria traslacional o axial, cuya densidad de corriente total es parcialmente conocida (problemas de induccion). Incluye la capacidad para tratar medios con movimiento y se supone un comportamiento senoidal para la densidad de corriente fuente. Se desarrollan los algoritmos que se implantan en el programa de computo CALIIE-2D del Instituto de Investiga