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Sample records for ottavio leoni 1578-1630

  1. Ocean to Outback: Leonie Rennie's Contribution to Science Education in Australia

    Science.gov (United States)

    Venville, Grady

    2009-01-01

    In this article I initially borrow a metaphor from an art exhibition, "Ocean to Outback," as a way to express my perspective on the contribution that Leonie Rennie has made to science education in Australia. I then consider Leonie's contributions as overlapping themes. In particular, Leonie's well-known research on gender and issues of…

  2. Exocomet Signatures Around the A-shell Star Phi Leonis

    Science.gov (United States)

    Eiroa, C.; Rebollido, I.; Montesinos, B.; Villaver, E.; Absil, O.; Henning, Th.; Bayo, A.; Canovas, H.; Carmona, A.; Chen, Ch.; hide

    2016-01-01

    We present an intensive monitoring of high-resolution spectra of the Ca II K line in the A7IV shell star Phi Leonis at very short (minutes, hours), short (night to night), and medium (weeks, months) timescales. The spectra show remarkable variable absorptions on timescales of hours, days, and months. The characteristics of these sporadic events are very similar to most that are observed toward the debris disk host star Beta Pictoris, which are commonly interpreted as signs of the evaporation of solid, comet-like bodies grazing or falling onto the star. Therefore, our results suggest the presence of solid bodies around Phi Leonis. To our knowledge, with the exception of Beta Pictoris, our monitoring has the best time resolution at the mentioned timescales for a star with events attributed to exocomets. Assuming the cometary scenario and considering the timescales of our monitoring, our results indicate that Phi Leonis presents the richest environment with comet-like events known to date, second only to Beta Pictoris.

  3. Spatial heterodyne interferometry of VY Canis Majoris, alpha Orionis, alpha Scorpii, and R Leonis at 11 microns

    International Nuclear Information System (INIS)

    Sutton, E.C.; Storey, J.W.V.; Betz, A.L.; Townes, C.H.; Spears, D.L.

    1977-01-01

    Using the technique of heterodyne interferometry, measurements were made of the spatial distribution of 11 micron radiation from four late type stars. The circumstellar shells surrounding VY Canis Majoris, alpha Orionis, and alpha Scorpii were resolved, whereas that of R Leonis was only partially resolved at a fringe spacing of 0.4 sec

  4. Spatial heterodyne interferometry of VY Canis Major's, alpha Orionis, alpha Scorpii, and R leonis at 11 microns

    Science.gov (United States)

    Sutton, E. C.; Storey, J. W. V.; Betz, A. L.; Townes, C. H.; Spears, D. L.

    1977-01-01

    Using the technique of heterodyne interferometry, measurements were made of the spatial distribution of 11 micron radiation from four late type stars. The circumstellar shells surrounding VY Canis Majoris, alpha Orionis, and alpha Scorpii were resolved, whereas that of R Leonis was only partially resolved at a fringe spacing of 0.4 sec.

  5. Masses and K-line absolute magnitudes of γ Leonis and 35 Comae

    International Nuclear Information System (INIS)

    Deming, D.; Dykton, M.

    1979-01-01

    The visual binary system γ Leonis consists of two K giants whose total mass was found by Wilson to be less than 0.6M/sub sun/ when a distance was obtained from K-line absolute magnitudes of both components. Since the orbital period of the system is of order 600 years, the orbital solution has usually been regarded as the most likely explanation of the anomalous mass. We have investigated the uniqueness of the orbital solution. We find that the individual orbital elements are only poorly determined, but that a 3 /P 2 is known to within +- 10%. The anomalous mass of this binary system implies either extensive mass-loss or the need for revisions in the K-line absolute magnitudes. We also investigate the binary system 35 Comae. Wilson has noted that in this system the K-line absolute magnitude of the G8 III primary component implies a total mass of 8 M/sub sun/. However the A component of 35 Comae is not sufficiently luminous to justify such a large total mass. The system has a period of order 700 years, and the uniqueness of the orbital solution is therefore suspect. However, in this case also we have investigated the uniqueness of the orbital solution and find that individual orbital elements are poorly determined, but that a 3 /P 2 is known to within +- 17%. We point out that 35 Comae is known to be very metal rich, in contrast to γ Leonis which is metal poor. We conclude that a composition-dependent correction to the K-line absolute magnitudes provides the simplest explanation of these mass anomalies. Such a correction would also give better agreement with the trigonometric parallaxes of these binary systems

  6. AD Leonis: Radial Velocity Signal of Stellar Rotation or Spin–Orbit Resonance?

    Science.gov (United States)

    Tuomi, Mikko; Jones, Hugh R. A.; Barnes, John R.; Anglada-Escudé, Guillem; Butler, R. Paul; Kiraga, Marcin; Vogt, Steven S.

    2018-05-01

    AD Leonis is a nearby magnetically active M dwarf. We find Doppler variability with a period of 2.23 days, as well as photometric signals: (1) a short-period signal, which is similar to the radial velocity signal, albeit with considerable variability; and (2) a long-term activity cycle of 4070 ± 120 days. We examine the short-term photometric signal in the available All-Sky Automated Survey and Microvariability and Oscillations of STars (MOST) photometry and find that the signal is not consistently present and varies considerably as a function of time. This signal undergoes a phase change of roughly 0.8 rad when considering the first and second halves of the MOST data set, which are separated in median time by 3.38 days. In contrast, the Doppler signal is stable in the combined High-Accuracy Radial velocity Planet Searcher and High Resolution Echelle Spectrometer radial velocities for over 4700 days and does not appear to vary in time in amplitude, phase, period, or as a function of extracted wavelength. We consider a variety of starspot scenarios and find it challenging to simultaneously explain the rapidly varying photometric signal and the stable radial velocity signal as being caused by starspots corotating on the stellar surface. This suggests that the origin of the Doppler periodicity might be the gravitational tug of a planet orbiting the star in spin–orbit resonance. For such a scenario and no spin–orbit misalignment, the measured v\\sin i indicates an inclination angle of 15.°5 ± 2.°5 and a planetary companion mass of 0.237 ± 0.047 M Jup.

  7. From Point Cloud to Digital Fabrication: a Tangible Reconstruction of Ca' Venier Dei Leoni, the Guggenheim Museum in Venice

    Science.gov (United States)

    Balletti, C.; D'Agnano, F.; Guerra, F.; Vernier, P.

    2016-06-01

    The paper describes how new digital methodologies can be used within the field of Cultural Heritage, not only with the aim of documenting the actual state of an architecture but to review the past transformations it has undergone, conserving and representing these histories as well. The premise to conservation and enhancement of our Heritage is a deep study in terms of position, shape, colour, and also of the historical and artistic features. Survey methods have acquired data acquisition techniques in line with technological progress: today's electronic and IT technologies, that are the tools of modern Geomatics, allow the effective survey and representation of 3D objects, from architectural structures to sculptures or archaeological finds. Over the last few years, the methodologies of acquisition and integrated representation for 3D patrimony documentation have developed and consolidated considerably: the possibilities of the digital realm can augment the understanding and the valorisation of a monument. The specific case offered in the present paper, Ca' Venier dei Leoni, the palace where is the Guggenheim Museum in Venice, is a significant example. It suggests not only the theme of the "no longer existing", or better never built, but also the opportunity to formulate hypotheses regarding its implementation and the impact that the palace would have had in the Venetian contest.

  8. A general solution for optimal egg size during external fertilization, extended scope for intermediate optimal egg size and the introduction of Don Ottavio 'tango'

    NARCIS (Netherlands)

    Luttikhuizen, PC; Honkoop, PJC; Drent, J; van der Meer, J

    2004-01-01

    Egg sizes of marine invertebrates vary greatly, both within and between species. Among the proposed causes of this are a trade-off between egg size, egg number and survival probability of offspring, and a selection pressure exerted by sperm limitation during external fertilization. Although larger

  9. Physical Nature and Orbital Behavior of the Eclipsing System UZ Leonis

    Science.gov (United States)

    Lee, Jae Woo; Park, Jang-Ho

    2018-03-01

    New CCD photometric observations of UZ Leo were obtained between 2012 February and 2013 April, and on 2017 February. Its physical properties were derived from detailed analyses of our light curves and existing radial velocities. The results indicate that this system is a totally eclipsing A-subtype overcontact binary with both a high fill-out factor of 76% and a third light source contributing 12% light in the B bandpass, 10% in V, and 7% in R. The light residuals between observations and theoretical models are satisfactorily fitted by adopting a magnetic cool spot on the more massive primary star. Including our 12 measurements, a total of 172 eclipse times were used for ephemeris computations. We found that the orbital period of UZ Leo has varied due to a periodic oscillation superposed on an upward parabolic variation. The observed period increase at a rate of +3.49× {10}-7 day yr‑1 can be plausibly explained by some combination of non-conservative mass transfer from the secondary to the primary component and angular momentum loss due to magnetic braking. The period and semi-amplitude of the oscillation are about 139 years and 0.0225 days, respectively, which is interpreted as a light-time effect due to a third component with a mass of {M}3\\sin {i}3=0.30 {M}ȯ . Because the third lights of 7%–12% indicate that the circumbinary object is very overluminous for its mass, it would possibly match a white dwarf, rather than an M-type main sequence.

  10. Hubble Space Telescope Ultraviolet Light Curves Reveal Interesting Properties of CC Sculptoris and RZ Leonis

    Energy Technology Data Exchange (ETDEWEB)

    Szkody, Paula; Mukadam, Anjum S. [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States); Toloza, Odette; Gänsicke, Boris T.; Pala, Anna F. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Dai, Zhibin [Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216 (China); Waagen, Elizabeth O. [AAVSO, 48 Bay State Rd, Cambridge, MA 02138 (United States); Godon, Patrick; Sion, Edward M., E-mail: szkody@astro.washington.edu [Department of Astrophysics and Planetary Science, Villanova University, Villanova, PA 19085 (United States)

    2017-03-01

    Time-tag ultraviolet data obtained on the Hubble Space Telescope in 2013 reveal interesting variability related to the white dwarf spin in the two cataclysmic variables RZ Leo and CC Scl. RZ Leo shows a period at 220 s and its harmonic at 110 s, thus identifying it as a likely Intermediate Polar (IP). The spin signal is not visible in a short single night of ground-based data in 2016, but the shorter exposures in that data set indicate a possible partial eclipse. The much larger UV amplitude of the spin signal in the known IP CC Scl allows the spin of 389 s, previously only seen at outburst, to be visible at quiescence. Spectra created from the peaks and troughs of the spin times indicate a hotter temperature of several thousand degrees during the peak phases, with multiple components contributing to the UV light.

  11. PHOTOMETRIC STUDIES OF THREE NEGLECTED SHORT-PERIOD CONTACT BINARIES GN BOOTIS, BL LEONIS, AND V1918 CYGNI

    International Nuclear Information System (INIS)

    Yang, Y.-G.; Dai, H.-F.; Qian, S.-B.

    2013-01-01

    We present new photometry for three short-period contact binaries, GN Boo, BL Leo, and V1918 Cyg, observed from 2008 December to 2012 April using several small telescopes in China. Photometric models were deduced from new observations using the updated Wilson-Devinney Code. The results show that GN Boo and BL Leo are W-type contact binaries, while V1918 Cyg is an A-type one. The mass ratios and fill-out factors are q = 0.320(± 0.002) and f = 5.8(± 0.1)% for GN Boo, q = 0.476(± 0.005) and f = 21.3(± 1.1)% for BL Leo, q = 0.264(± 0.002), and f = 49.7(± 0.7)% for V1918 Cyg, respectively. From the (O – C) curves, it is discovered that the orbital periods of three binaries have varied in a complicated way, i.e., cyclic oscillation for GN Boo, long-term period decrease for BL Leo, and both for V1918 Cyg. The cyclic variations for GN Boo and V1918 Cyg may probably be attributed to the magnetic activity of the primary component or light-time effect due to the third body. Meanwhile, the secular period decreases for BL Leo and V1918 Cyg may result from mass transfer from the primary to the secondary, accompanying the mass and angular momentum loss from the central system. Finally, GN Boo, BL Leo, and V1918 Cyg will evolve into deep contact binaries. Additionally, a statistical study of 37 contact binaries with decreasing periods is given. We obtained the relations of q – f and q – dln P/dt, and preliminarily determined the mass loss rate of dln M/dt from the binary system.

  12. Optical region elemental abundance analyses of B and A stars. V. The normal stars theta Leonis, tau Herculis, 14 Cygni, and 5 Aquarii

    International Nuclear Information System (INIS)

    Adelman, S.J.; NASA Goddard Space Flight Center, Greenbelt, MD

    1986-01-01

    Abundance analyses using optical region data and fully line-blanketed model atmospheres have been performed for four sharp-lined normal B and A type stars. This work extends the results presented in the first and fourth papers of this series. The microturbulent velocities of all the stars studied in this series are found to follow the same relation with temperature. Some of the stars studied in this paper are found to have one or two anomalous abundances, such as the zirconium abundance of theta Leo

  13. Astrometrically registered simultaneous observations of the 22 GHz H{sub 2}O and 43 GHz SiO masers toward R Leonis Minoris using KVN and source/frequency phase referencing

    Energy Technology Data Exchange (ETDEWEB)

    Dodson, Richard; Rioja, María J.; Jung, Tae-Hyun; Sohn, Bong-Won; Byun, Do-Young; Cho, Se-Hyung; Lee, Sang-Sung; Kim, Jongsoo; Kim, Kee-Tae; Oh, Chung-Sik; Han, Seog-Tae; Je, Do-Heung; Chung, Moon-Hee; Wi, Seog-Oh; Kang, Jiman; Lee, Jung-Won; Chung, Hyunsoo; Kim, Hyo-Ryoung; Kim, Hyun-Goo; Lee, Chang-Hoon, E-mail: rdodson@kasi.re.kr [Korea Astronomy and Space Science Institute, Daedeokdae-ro 776, Yuseong-gu, Daejeon 305-348 (Korea, Republic of); and others

    2014-11-01

    Oxygen-rich asymptotic giant branch (AGB) stars can be intense emitters of SiO (v = 1 and 2, J = 1 → 0) and H{sub 2}O maser lines at 43 and 22 GHz, respectively. Very long baseline interferometry (VLBI) observations of the maser emission provide a unique tool to probe the innermost layers of the circumstellar envelopes in AGB stars. Nevertheless, the difficulties in achieving astrometrically aligned H{sub 2}O and v = 1 and v = 2 SiO maser maps have traditionally limited the physical constraints that can be placed on the SiO maser pumping mechanism. We present phase-referenced simultaneous spectral-line VLBI images for the SiO v = 1 and v = 2, J = 1 → 0, and H{sub 2}O maser emission around the AGB star R LMi, obtained from the Korean VLBI Network (KVN). The simultaneous multi-channel receivers of the KVN offer great possibilities for astrometry in the frequency domain. With this facility, we have produced images with bona fide absolute astrometric registration between high-frequency maser transitions of different species to provide the positions of the H{sub 2}O maser emission and the center of the SiO maser emission, hence reducing the uncertainty in the proper motions for R LMi by an order of magnitude over that from Hipparcos. This is the first successful demonstration of source frequency phase referencing for millimeter VLBI spectral-line observations and also where the ratio between the frequencies is not an integer.

  14. Animated Dreamsi peaauhind läks Tšiili

    Index Scriptorium Estoniae

    2009-01-01

    Pimedate Ööde 13. filmifestivali teise alafestivali Animated Dreams auhinnasaajad : võitis Cristobal Leoni, Niles Atallah' ja Joaquin Cocina "Lucia", Anoba nominatsiooni sai Kaspar Jancise "Krokodill"

  15. Animated Dreamsi grand prix läks Tšiilisse / Kristiina Davidjants

    Index Scriptorium Estoniae

    Davidjants, Kristiina, 1974-

    2009-01-01

    Pimedate Ööde 13. filmifestivali teise alafestivali Animated Dreams auhinnasaajad: võitis Cristobal Leoni, Niles Atallah' ja Joaquin Cocina "Lucia", ANOBA nominatsiooni sai Kaspar Jancise "Krokodill". Lisatud nimekiri "Animated Dreamsi võitjad"

  16. On A Recent Theory of 'Legal Obligation'

    Directory of Open Access Journals (Sweden)

    Bruno Leoni

    2009-02-01

    Full Text Available This paper, by the late Bruno Leoni, was originally published in the Italian journal Il Politico in 1966. In the article, Leoni reviews H.L.A. Hart’s The Concept of Law (1961. Hart first analyzes the concept of law by resorting to the classical concept of “obligation.” But he later tries a “fresh start” by resorting to the concept of “secondary rules.” In his review, Leoni argues that the former attempt is confronted with serious difficulties, and that the latter attempt (to which professor Hart possibly resorts in view of overcoming some of said difficulties is ultimately inconsistent with the former

  17. Propos autour d’un inventaire : quelques peintures italiennes à Bastia

    OpenAIRE

    Michel-Edouard Nigaglioni; Pierre Curie

    2005-01-01

    Du Moyen Age à la fin du XVIIIe siècle, Bastia fut une ville italienne dépendant de la république de Gênes. C’est pourquoi les églises de la ville conservent encore nombre de toiles d’artistes génois (Ottavio Cambiaso, Domenico Piola, Giuseppe Badaracco) ou provenant de régions italiennes proches de la Corse (Giovanni Bilivert). En 1844, le legs du cardinal Fesch, oncle de Napoléon, fait entrer dans les collections municipales une centaine de tableaux italiens. Des restaurations récentes (Lav...

  18. Prima Vistale tuleb tuntud kirjanikke mitmest Euroopa riigist / Kaarel Kressa

    Index Scriptorium Estoniae

    Kressa, Kaarel, 1983-

    2010-01-01

    Prima Vista kirjandusfestivali külalisi: Leonie Swann, Attila Bartis, Dmitri Bõkov, Zinaida Lindén, Mihhail Šiškin, Fay Weldon, Jason Goodwin, Rosa Maria Rodríguez Magda, Inga Gaile, Juris Kronbergs, Guntars Godinš, Liana Langa

  19. Leo

    Science.gov (United States)

    Murdin, P.

    2000-11-01

    (the Lion; abbrev. Leo, gen. Leonis; area 947 sq. deg.) A northern zodiacal constellation which lies between Cancer and Virgo, and culminates at midnight in early March. It represents the Nemean lion that, in Greek mythology, Hercules killed as the first of his 12 labors. Its brightest stars were cataloged by Ptolemy (c. AD 100-175) in the Almagest....

  20. The Hungry Season

    African Journals Online (AJOL)

    start to go some way towards addressing this fundamental question. A delightful animation of The Hungry Season, commissioned by Leonie Joubert and funded by the University of Cape Town's Criminology. Department and the Embassy of Finland, is available online at http://www.youtube.com/ watch?v=iX77NZttLKo.

  1. Fiktiivne auhinnagala Lõuna-Prantsusmaal II / Madli Pesti

    Index Scriptorium Estoniae

    Pesti, Madli, 1980-

    2009-01-01

    Muljeid tänavusest 63. Avignoni teatrifestivalist. Pikemalt järgmistest etendustest: Krzysztof Warlikowski "(A)pollonia", Claude Regy "Ode Maritime" (Fernando Pessoa poeemi järgi), Frederico Leoni "Yo en el futuro" ("Mina tulevikus"), Thierry Bedard'i "Geko košmaarid" jt.

  2. Herschel/HIFI Observations of IRC+10216: Water Vapor in the Inner Envelope of a Carbon-rich Asymptotic Giant Branch Star

    NARCIS (Netherlands)

    Neufeld, D. A.; González-Alfonso, E.; Melnick, G.; Szczerba, R.; Schmidt, M.; Decin, L.; de Koter, A.; Schöier, F. L.; Cernicharo, J.

    2011-01-01

    We report the results of observations of 10 rotational transitions of water vapor toward the carbon-rich asymptotic giant branch (AGB) star IRC+10216 (CW Leonis), carried out with Herschel's HIFI instrument. Each transition was securely detected by means of observations using the dual beam switch

  3. Muusikamaailm. Magnus Lindbergi festivali jätk. Jonas Forsell taas ooperijuhiks. Marcello Panni uus ooper. György Kurtagile Sonningi preemia. Peter Gradenwitz lahkunud / Priit Kuusk

    Index Scriptorium Estoniae

    Kuusk, Priit, 1938-

    2002-01-01

    Soome helilooja Magnus Lindbergi mitmeid teoseid esitatakse Inglismaal. Rootsi heliloojast Jonas Forsellist sai jaanuaris Kopenhaageni trupi Den Anden Opera kunstiline juht. Firenzes tuli esiettekandele Marcello Panni uus ooper "The Banquet ئ Talking about Love". Helilooja György Kurtag pälvis Taani 2003.a. Leonie Sonningi muusikapreemia. 91aastasena suri muusikateadlane Peter Gradenwitz

  4. The effects of altered levels of UV-B radiation on an Antarctic grass and lichen

    NARCIS (Netherlands)

    Lud, D.; Huiskes, A.H.L.; Moerdijk-Poortvliet, T.C.W.; Rozema, J.J.

    2001-01-01

    We report a long-term experiment on the photosynthetic response of natural vegetation of Deschampsia antarctica (Poaceae) and Turgidosculum complicatulum (Lichenes) to altered UV-B levels on Leonie Island, Antarctica. UV-B above the vegetation was reduced by filter screens during two seasons. Half

  5. Consequences of depletion of stratospheric ozone for terrestrial Antarctic ecosystems: the response of Deschampsia antarctica to enhanced UV-B radiation in a controlled environment

    NARCIS (Netherlands)

    Rozema, J.J.; Broekman, R.; Lud, D.; Huiskes, A.H.L.; Moerdijk-Poortvliet, T.C.W.; De Bakker, N.; Meijkamp, B.; Van Beem, A.

    2001-01-01

    Mini UV lamps were installed over antarctic plants at Leonie Island, Antarctic peninsula, and shoot length measurements of Deschampsia antarctica were performed during the austral summer January-February 1999. We studied the response of the antarctic hairgrass, Deschampsia antarctica to enhanced

  6. Bagatellid : Maailm / Nele-Eva Steinfeld

    Index Scriptorium Estoniae

    Steinfeld, Nele-Eva

    2009-01-01

    Muusikasõnumeid maailmast: Cecilia Bartoli pälvis Leonie Sonningi auhinna. Lorin Maazel jätab hüvasti New Yorgi Filharmoonikutega. Leitud kaks uut Mozarti klaveriteost. Uudiseid konkursimaailmast. Rootsi Raadio P2 resideerivaks heliloojaks valiti Mirjam Tally

  7. Tommaso Pincio and the paper world

    Directory of Open Access Journals (Sweden)

    Franco Zangrilli

    2016-07-01

    Full Text Available Ottavio Tondi, the main character of Tommaso Pincio’s last novel, Panorama (NN Editore, 2015, works as a literary consultant for influential publishing houses. Described as an isolated person, epitome of the intellectual-writer able to see his own crisis and, so far, the crisis of his historic moment, Ottavio oscillates between the distant relationship with a woman, Ligeia, whom he doesn’t know in person, and his resigned rejection of life in society, trying to remain, as a new Don Quixote, as a “pure reader”. Offering a critical view of trending writers, of those vain and egoistic “divos” always in the heart of mass media, the novel builds up a very large number of topics, such as the reflection about reading considered as a mythic, intimate and sacred ritual, as well as the limits of translation, an incisive satire of the nowadays journalism or the condition of our decadent society, in the hands of an alienating and impersonal technology that have finally changed personal relationships through the use of online social networking services.

  8. FITOCENOSIS EN LOS MOGOTES DE LA GRAN MESETA DE GUANTÁNAMO, CUBA ORIENTAL

    Directory of Open Access Journals (Sweden)

    Reyes Orlando

    2013-07-01

    Full Text Available Los mogotes de la Gran Meseta de Guantánamo están constituidos por calizas durasde la Formación Charco Redondo. La temperatura del aire varía entre 22 y 240C yllueve de 1 200 a 1 400 mm al año. Mediante la metodología de la Escuela Zurich- Montpellier se describe un nuevo orden, Coccothrinaci leonis - Guapiretaliarufescentis, con su alianza Coccothrinaci leonis - Guapirion rufescentis y tresasociaciones. Bactrio cubensis - Podocarpodetum ekmanii y Phyllantho epiphyllanthi- Tabebuietum myrtifoliae que se establecen en la parte superior de los mogotes y laasociación Pileo fruticulosae - Thelypteridetum alatae en fragmentos verticales, lasdos primeras tienen una bien desarrollada estera radical donde se produce el reciclajede nutrientes de este ecosistema

  9. An overview of dinoflagellate cysts in recent sediments along the west coast of India

    Digital Repository Service at National Institute of Oceanography (India)

    DeSilva, M.S.; Anil, A.C.; DeCosta, P.M.

    using SURFER Fig. 1—Location map of sampling stations (26 coastal stations and 3 port areas) along the west coast of India. D’SILVA et al.: AN OVERVIEW OF DINOFLAGELLATE CYSTS IN RECENT SEDIMENTS 699 plots (SURFER 8 program). The relative... Xandarodinium variable Bujak Prot.div Protoperidinium latissimum (Kofoid) Balech – Prot.lat Protoperidinium leonis (Pavillard) Balech Quinquecuspis concreta (Reid) Harland Prot.leo Protoperidinium oblongum (Aurivillius) Balech Votadinium calvum Reid Prot...

  10. Propos autour d’un inventaire : quelques peintures italiennes à Bastia

    Directory of Open Access Journals (Sweden)

    Michel-Edouard Nigaglioni

    2005-09-01

    Full Text Available Du Moyen Age à la fin du XVIIIe siècle, Bastia fut une ville italienne dépendant de la république de Gênes. C’est pourquoi les églises de la ville conservent encore nombre de toiles d’artistes génois (Ottavio Cambiaso, Domenico Piola, Giuseppe Badaracco ou provenant de régions italiennes proches de la Corse (Giovanni Bilivert. En 1844, le legs du cardinal Fesch, oncle de Napoléon, fait entrer dans les collections municipales une centaine de tableaux italiens. Des restaurations récentes (Lavinia Fontana et une reconsidération globale du fonds, rendue possible par l’inventaire du mobilier appartenant à la ville, permettent découvertes et propositions d’attribution (Francesco Brizio, Giuseppe Bonito….From the Middle Ages up to the end of the eighteenth century, Bastia was an Italian city belonging to the Republic of Genoa. This is why the churches of the city conserve several paintings by artists of Genoese origin (Ottavio Cambiaso, Domenico Piola, Giuseppe Badaracco or coming from other regions in Italy close to Corsica (Giovanni Bilivert. In 1844, a bequest by Cardinal Fesch (Napoleon’s uncle also brought about a hundred Italian paintings to the collections of the city. Some recent restoration work (Lavinia Fontana and a new, general view of the corpus of paintings, helped by the inventory of the furniture belonging to the city, has given rise to some discoveries and also allows for the authors of certain paintings to be identified (Francesco Brizio, Guiseppe Bonito….

  11. Radio-wavelength observations of magnetic fields on active dwarf-M, RS CVN and magnetic stars

    Energy Technology Data Exchange (ETDEWEB)

    Lang, K.R.

    1986-01-01

    The dwarf M stars YZ Canis Minoris and AD Leonis exhibit narrow band, slowly varying (hours) microwave emission that cannot be explained by conventional thermal radiation mechanisms. The dwarf M stars AD Leonis and Wolf 424 emit rapid spikes whose high brightness temperatures similarly require a nonthermal radiation process which could result from coherent mechanisms such as an electron-cyclotron maser or coherent-plasma radiation. If the electron-cyclotron maser emits at the second or third harmonic of the gyrofrequency, the coronal magnetic field strength H = 250 or 167 G and constraints on the plasma frequency imply an electron density of 6 x 10/sup 9//cm/sup 3/. Coherent-plasma radiation requires similar values of electron density but much weaker magnetic fields. Radio spikes from AD Leonis and Wolf 424 have rise times tau/sub R/ < 5 ms, indicating a linear size of L < 1.5 x 10/sup 8/ cm, or less than 0.005 of the stellar radius. Although Ap magnetic stars have strong dipole magnetic fields, they exhibit no detectable gyroresonant radiation, suggesting that these stars do not have hot, dense coronae. The binary RS CVn star UX Arietis exhibits variable emission at 6 cm wavelength on time scales ranging from 30 s to more than one hour. The shortest variation implies a linear size much less than that of the halo observed by VLBI techniques, and most probably sizes smaller than those of the component stars. The observed variations might be due to absorption by a thermal plasma located between the stars.

  12. Detroit – En by i forfald

    OpenAIRE

    Schultz, Agnethe; Mia, [No Value; Lise, [No Value; Nanna, [No Value; Borggaard, Mille; Kvorning, [No Value; Jacobsen, [No Value; Bjørnstrup, [No Value

    2014-01-01

    Through this bachelor project we have studied how to create incentive for economic growth in Detroit without losing the authenticity of the city, and how this can be co-creational in an attractive identity for Detroit. The outcome of our study is based on Sharon Zukin’s understanding of authenticity and identity in urban cities, Richard Florida’s theory of the Creative Class, and Leonie Sandercock’s assumptions of storytelling in city development. The conclusion of our study is formed as five...

  13. Broadband spectral observation of a dMe star radio flare

    International Nuclear Information System (INIS)

    Guedel, M.; Benz, A.O.; Fuerst, E.; Simett, G.M.; Davis, R.J.

    1989-01-01

    A flare on the dMe star AD Leonis was simultaneously observed with the radio telescopes in Effelsberg, Jodrell Bank, and Arecibo using spectrometers at 1665, 166 and 1415 MHz with bandwidths of 25, 100 and 40 MHz respectively. The time coincidence confirms the stellar origin of the radiation. The flare emission was resolved into a multitude of broadband pulsations. The e-folding rise and decay times were of the order of the time resolution of the Effelsberg data (125 ms), or less. The circular polarization was ∼ 100%. Similar bursts, but 4 orders of magnitude less powerful, have been observed from the sun at lower frequencies

  14. THEORETICAL CONCEPTIONS OF GEOGRAPHY TEACHERS

    Directory of Open Access Journals (Sweden)

    Eloy Montes Galbán

    2007-11-01

    Full Text Available The main goal of this research was to determine the current theoretical concepts handled by third stage basic education geography teachers. A non experimental descriptive study was made. Data was collected through a semi structured questionnaire. The population was conformed by the teachers who work at the National schools placed in the parishes Raul Leoni and Cacique Mara of Maracaibo city, Zulia State. There is not clarity in regard to the correct handling of the different geographic currents, and the slight notion teachers have leans towards a traditional, descriptive, retrospective memory based conception.

  15. Synthesis and in vitro growth inhibitory activity of novel silyl- and trityl-modified nucleosides

    CSIR Research Space (South Africa)

    Panayides, Jenny-Lee

    2016-06-01

    Full Text Available -Farkas d, Hajierah Davids d,e , Leonie Harmse d , M. E. Christine Rey f , Ivan R. Green g, Stephen C. Pelly g, Robert Kiss c, Alexander Kornienko h, Willem A. L. van Otterlo a,g,⇑ a Molecular Sciences Institute, School of Chemistry, University..., Matieland 7602, South Africa hDepartment of Chemistry and Biochemistry, Texas State University, San Marcos, TX 78666, USA Abstract Seventeen silyl- and trityl-modified (5'-O- and 3',5'-di-O-) nucleosides were synthesized with the aim of investigating...

  16. Lion walking freely in the Louvre

    OpenAIRE

    Dimitrijević, Braco

    2016-01-01

    Nel 1996 Braco Dimitrijević, intervistato da Jean-Hubert Martin per “Flash Art” ha affermato: Se si guarda la terra dalla luna non c’è praticamente alcuna distanza tra il Louvre e lo zoo. Ci sono gabbie allo zoo così come ci sono al Louvre. Il mio ultimo obiettivo è rimuovere le porte e vedere i leoni liberi al Louvre. Questo progetto utopico, donato a MoRE, si inserisce all’interno di quella linea di ricerca basata appunto sull’accostamento tra importanti collezioni espositive ed animali viv...

  17. Genome-scale data suggest reclassifications in the Leisingera-Phaeobacter cluster including proposals for Sedimentitalea gen. nov. and Pseudophaeobacter gen. nov.

    Directory of Open Access Journals (Sweden)

    Sven eBreider

    2014-08-01

    Full Text Available Earlier phylogenetic analyses of the marine Rhodobacteraceae (class Alphaproteobacteria genera Leisingera and Phaeobacter indicated that neither genus might be monophyletic. We here used phylogenetic reconstruction from genome-scale data, MALDI-TOF mass-spectrometry analysis and a re-assessment of the phenotypic data from the literature to settle this matter, aiming at a reclassification of the two genera. Neither Phaeobacter nor Leisingera formed a clade in any of the phylogenetic analyses conducted. Rather, smaller monophyletic assemblages emerged, which were phenotypically more homogeneous, too. We thus propose the reclassification of Leisingera nanhaiensis as the type species of a new genus as Sedimentitalea nanhaiensis gen. nov., comb. nov., the reclassification of Phaeobacter arcticus and Phaeobacter leonis as Pseudophaeobacter arcticus gen. nov., comb. nov. and Pseudophaeobacter leonis comb. nov., and the reclassification of Phaeobacter aquaemixtae, Phaeobacter caeruleus and Phaeobacter daeponensis as Leisingera aquaemixtae comb. nov., Leisingera caerulea comb. nov. and Leisingera daeponensis comb. nov. The genera Phaeobacter and Leisingera are accordingly emended.

  18. Euridice by Giulio Caccini: Two (? Copies of the Original Score Held in the Cathedral of Ljubljana around 1620

    Directory of Open Access Journals (Sweden)

    Metoda Kokole

    2012-07-01

    Full Text Available L’Euridice, composta in musica in stile rappresentativo by Giulio Caccini (1551–1618 is considered the first fully preserved and printed opera in music history. It was composed in 1600 to the libretto by Ottavio Rinuccini, itself commissioned for the wedding celebrations of Maria de Medici and her spouse, the French king Henry IV. The score was printed in 1600 in Florence and dedicated to Count Giovanni Bardi; in 1615 it was reprinted in Venice, but without the dedication. In fact, Caccini had not been commissioned to write the music for that occasion: in 1600 the official composer of the opera Euridice had been Jacopo Peri, whose version, with approximately one sixth of Caccini’s music – the parts sung by Caccini’s family members, including Euridice’s part – was performed in Florence on 6 October 1600. At this hybrid performance, parts of Giulio Caccini’s opera were heard for the first time. The only known full staging of Caccini’s opera took place on 5 December 1602 at Palazzo Pitti in Florence to honour Cardinal Montalto. It entertained the noble public for two hours. Considering the simplicity and shortness of the extant score, the performance cannot have been a simple one: it would have included repetitions, dances, and other unwritten additions. In the tradition of humanist Florentine circles, Ottavio Rinuccini’s libretto follows one of the most famous classical myths – the story of the divine singer Orpheus, which was particularly appropriate for a first attempt to resurrect the classical tragedy, believed to have been entirely sung. Yet Rinuccini was inspired not only by Ovid’s and Virgil’s narratives of the myth but also by Angelo Poliziano’s Favola di Orfeo and some other, earlier Renaissance sources. Thee story itself was partly changed and adapted to the occasion of an important state marriage, a common practice in later operatic texts as well. It tells only the first part of the myth, centred on the

  19. Francisco Giralte y el sepulcro del obispo Gutierre de Carvajal

    Directory of Open Access Journals (Sweden)

    Vasallo Toranzo, Luis

    2013-12-01

    Full Text Available The high valuation placed on the tomb of Bishop Gutierre de Carvajal, sculpted by Francisco de Giralte, resulted in a lawsuit for which the most important artists from Toledo, Alcalá and Madrid were called to testify. Their testimonies, made during the crucial moment when Berruguete died and the court arrived at Madrid are very useful for understanding the artistic appreciation of a work. Thus, relevant artists of the period –Pompeyo Leoni, Nicolás Vergara el Viejo, Jácome Trezo or Juan Bautista de Toledo– attested to the perfect technique, the beauty of the carving, the multiplicity of personages represented next to the dead Bishop, and the wish to achieve their portrait likenesses.La alta tasación alcanzada por el sepulcro del obispo Gutierre de Carvajal, obra de Francisco Giralte, motivó un pleito al que fueron llamados los principales artistas de Toledo, Alcalá y Madrid. Sus testimonios, realizados en el crucial momento en que se produjo la muerte de Berruguete y llegó la corte a Madrid, son muy útiles para conocer la estimación artística de una obra, de la que personajes como Pompeyo Leoni, Nicolás de Vergara el Viejo, Jácome Trezo o Juan Bautista de Toledo ponderaron la perfección técnica, la belleza de su talla, la multiplicación de personajes representados junto al finado y la voluntad retratística presente en todos ellos.

  20. Assessment of volume and leak measurements during CPAP using a neonatal lung model

    International Nuclear Information System (INIS)

    Fischer, H S; Roehr, C C; Proquitté, H; Wauer, R R; Schmalisch, G

    2008-01-01

    Although several commercial devices are available which allow tidal volume and air leak monitoring during continuous positive airway pressure (CPAP) in neonates, little is known about their measurement accuracy and about the influence of air leaks on volume measurement. The aim of this in vitro study was the validation of volume and leak measurement under CPAP using a commercial ventilatory device, taking into consideration the clinical conditions in neonatology. The measurement accuracy of the Leoni ventilator (Heinen and Löwenstein, Germany) was investigated both in a leak-free system and with leaks simulated using calibration syringes (2–10 ml, 20–100 ml) and a mechanical lung model. Open tubes of variable lengths were connected for leak simulation. Leak flow was measured with the flow-through technique. In a leak-free system the mean relative volume error ±SD was 3.5 ± 2.6% (2–10 ml) and 5.9 ± 0.7% (20–60 ml), respectively. The influence of CPAP level, driving flow, respiratory rate and humidification of the breathing gas on the volume error was negligible. However, an increasing F i O 2 caused the measured tidal volume to increase by up to 25% (F i O 2 = 1.0). The relative error ±SD of the leak measurements was −0.2 ± 11.9%. For leaks >19%, measured tidal volume was underestimated by more than 10%. In conclusion, the present in vitro study showed that the Leoni allowed accurate volume monitoring under CPAP conditions similar to neonates. Air leaks of up to 90% of patient flow were reliably detected. For an F i O 2 >0.4 and for leaks >19%, a numerical correction of the displayed volume should be performed

  1. Assessment of volume and leak measurements during CPAP using a neonatal lung model.

    Science.gov (United States)

    Fischer, H S; Roehr, C C; Proquitté, H; Wauer, R R; Schmalisch, G

    2008-01-01

    Although several commercial devices are available which allow tidal volume and air leak monitoring during continuous positive airway pressure (CPAP) in neonates, little is known about their measurement accuracy and about the influence of air leaks on volume measurement. The aim of this in vitro study was the validation of volume and leak measurement under CPAP using a commercial ventilatory device, taking into consideration the clinical conditions in neonatology. The measurement accuracy of the Leoni ventilator (Heinen & Löwenstein, Germany) was investigated both in a leak-free system and with leaks simulated using calibration syringes (2-10 ml, 20-100 ml) and a mechanical lung model. Open tubes of variable lengths were connected for leak simulation. Leak flow was measured with the flow-through technique. In a leak-free system the mean relative volume error +/-SD was 3.5 +/- 2.6% (2-10 ml) and 5.9 +/- 0.7% (20-60 ml), respectively. The influence of CPAP level, driving flow, respiratory rate and humidification of the breathing gas on the volume error was negligible. However, an increasing F(i)O(2) caused the measured tidal volume to increase by up to 25% (F(i)O(2) = 1.0). The relative error +/- SD of the leak measurements was -0.2 +/- 11.9%. For leaks > 19%, measured tidal volume was underestimated by more than 10%. In conclusion, the present in vitro study showed that the Leoni allowed accurate volume monitoring under CPAP conditions similar to neonates. Air leaks of up to 90% of patient flow were reliably detected. For an F(i)O(2) > 0.4 and for leaks > 19%, a numerical correction of the displayed volume should be performed.

  2. Nitrogen Dioxide long term trends at mid and high latitudes by means of ground based observations

    Science.gov (United States)

    Bortoli, D.; Petritoli, A.; Giovanelli, G.; Kostadinov, I.; Ravegnani, F.

    2003-04-01

    The interactions between mid- and high latitudes atmospheric changes are going to be one of the main issue for the future of stratospheric and tropospheric chemistry research. A more detailed study of the ozone trends as well as a wider comprehension of the interactions with lower and higher latitudes are maybe the main arguments to which scientist should address their works in order to build-up a more detailed picture of what scenarios we have to face in the near future. GASCODs type spectrometers (Gas Analyzer Spectrometer Correlating Optical Differences) are installed at the "Ottavio Vittori" research station (44.11N, 10.42E, 2165 m asl) since June 1993, at the Italian Antarctic Station (74.69S, 164.12E) since December 1995 and at the STIL-BAS station (42.42N, 25.63E) since 1999. The instruments measure zenith scattered solar radiation between 407 and 464 nm. Nitrogen dioxide total column is retrieved with DOAS methodology. The seasonal trend of NO2 vc values is reported and it shows the expected behaviour: maximum values during the summer period while the minimum occur in the winter season in both the hemispheres. A typical behaviour of the AMPM ratio at high latitudes is highlight. A Fourier analysis is proposed as a tool to investigate the long-term components of nitrogen dioxide stratospheric amount. Results are presented and the NO2 trend is evidenced and commented. ACKNOWLEDGMENTS: The author Daniele Bortoli was financially supported by the Subprograma Ciência e Tecnologia do 3° Quadro Comunitário de Apoio. The National Antarctic Research Program (PNRA) and the Quantification and Interpretation of Long-Term UV-Vis Observations of the Stratosphere (QUILT) project supported this research.

  3. Some Information Concerning Yom Tob Atias (Jeronimo de Vargas

    Directory of Open Access Journals (Sweden)

    Salomon, Herman P.

    2010-12-01

    Full Text Available The team of Ferrara editors was headed by two former New Christians: an entrepreneur, a native of Spain, and a Latin scholar from Portugal who in the introductions to variant editions of their scriptural production alternately call themselves by their Christian names Jeronimo de Vargas and Duarte Pinel, and by their Jewish names Yom Tob Atias and Abraham Usque. This “editorial schizophrenia” is reflected in the Italian archives. Whereas the historian Renata Segre’s researches have documented that Duarte Pinel and Abraham Usque were one and the same person, she was unable to find archival proof uniting Jeronimo de Vargas and Yom Tob Atias. The researcher Aron Leoni came up with a Latin notarial deed in the Ferrara archives wherein “Joantu Athias” is called “ptrem ac legitimum administratorum Hieronimi Vargas” and also the latter’s “patre et legitimo administrator.” He supposed “ptrem” to be an abbreviation of “procuratorem” and “patre” to mean father. Thus he concluded that Yom Tob Atias was the father of Jeronimo de Vargas. Close examination of the document and comparison with two others which have recently come to light reveal, however, the incontrovertible identity of Yom Tob Atias and Jeronimo de Vargas. We are dealing with a typical case of ex-Marrano heteronomy: a former New Christian maintaining a separate onomastic Christian identity alongside his Jewish one.

    El equipo de editores de Ferrara fue dirigido por dos antiguos cristianos nuevos, uno financiero, originario de España, y el otro, un latinista portugués. En las distintas introducciones a edición bíblica los dos se autodenominan alternativamente por sus nombres cristianos –Jerónimo de Vargas y Duarte Pinel– y por sus nombres judíos, Yom Tob Atías y Abraham Usque. Esta «esquizofrenia editorial» ha dejado huella en los archivos italianos. Mientras que las investigaciones de Renata Segre han documentado que Pinel y Usque eran la misma

  4. Ground-based observation of emission lines from the corona of a red-dwarf star.

    Science.gov (United States)

    Schmitt, J H; Wichmann, R

    2001-08-02

    All 'solar-like' stars are surrounded by coronae, which contain magnetically confined plasma at temperatures above 106 K. (Until now, only the Sun's corona could be observed in the optical-as a shimmering envelope during a total solar eclipse.) As the underlying stellar 'surfaces'-the photospheres-are much cooler, some non-radiative process must be responsible for heating the coronae. The heating mechanism is generally thought to be magnetic in origin, but is not yet understood even for the case of the Sun. Ultraviolet emission lines first led to the discovery of the enormous temperature of the Sun's corona, but thermal emission from the coronae of other stars has hitherto been detectable only from space, at X-ray wavelengths. Here we report the detection of emission from highly ionized iron (Fe XIII at 3,388.1 A) in the corona of the red-dwarf star CN Leonis, using a ground-based telescope. The X-ray flux inferred from our data is consistent with previously measured X-ray fluxes, and the non-thermal line width of 18.4 km s-1 indicates great similarities between solar and stellar coronal heating mechanisms. The accessibility and spectral resolution (45,000) of the ground-based instrument are much better than those of X-ray satellites, so a new window to the study of stellar coronae has been opened.

  5. VLA observations of dwarf M flare stars and magnetic stars

    Science.gov (United States)

    Willson, R. F.; Lang, K. R.; Foster, P.

    1988-01-01

    The VLA has been used to search for 6 cm emission from 16 nearby dwarf M stars, leading to the detection of only one of them - Gliese 735. The dwarf M flare stars AD Leonis and YZ Canis Minoris were also monitored at 6 cm and 20 cm wavelength in order to study variability. Successive oppositely circularly polarized bursts were detected from AD Leo at 6 cm, suggesting the presence of magnetic fields of both magnetic polarities. An impulsive 20-cm burst from YZ CMi preceded slowly varying 6-cm emission. The VLA was also used, unsuccessfully, to search for 6-cm emission from 13 magnetic Ap stars, all of which exhibit kG magnetic fields. Although the Ap magnetic stars have strong dipolar magnetic fields, the failure to detect gyroresonant radiation suggests that these stars do not have hot, dense coronae. The quiescent microwave emission from GL 735 is probably due to nonthermal radiation, since unusually high (H = 50 kG or greater) surface magnetic fields are inferred under the assumption that the 6-cm radiation is the gyroresonant radiation of thermal electrons.

  6. Elemental abundance analyses with coadded Dominion Astrophysical Observatory spectrograms: Pt. 3

    International Nuclear Information System (INIS)

    Adelman, S.J.

    1988-01-01

    Elemental abundance analyses were performed for three superficially normal main-sequence stars θ Leonis (A2V), τ Herculus (B5IV) and ο Pegasi (AlIV). These studies used coadded spectrograms produced from at least 12 2.4 A mm -1 IIaO Dominion Astrophysical Observatory spectrograms and show a greater degree of internal consistency and smaller microturbulent velocities than previous studies of these stars which used lower signal-to-noise data. Many lines not previously seen were identified including some of new atomic species whose analysis provide a more complete picture of the elemental abundances. The identification and analysis of La II lines in ο Peg link this star more closely with the classical metallic-lined (Am) stars, although there are considerable differences in abundances. Some of θ Leo's elemental abundances, particularly those of vanadium, strontium, and zirconium, are significantly different from solar in confirmation of previous analyses. τ Her's elemental abundances are typically a factor of 2 less than solar. (author)

  7. HERSCHEL /HIFI OBSERVATIONS OF IRC+10216: WATER VAPOR IN THE INNER ENVELOPE OF A CARBON-RICH ASYMPTOTIC GIANT BRANCH STAR

    International Nuclear Information System (INIS)

    Neufeld, David A.; Gonzalez-Alfonso, Eduardo; Melnick, Gary J.; Szczerba, Ryszard; Schmidt, Miroslaw; Decin, Leen; De Koter, Alex; Schoeier, Fredrik; Cernicharo, Jose

    2011-01-01

    We report the results of observations of 10 rotational transitions of water vapor toward the carbon-rich asymptotic giant branch (AGB) star IRC+10216 (CW Leonis), carried out with Herschel's HIFI instrument. Each transition was securely detected by means of observations using the dual beam switch mode of HIFI. The measured line ratios imply that water vapor is present in the inner outflow at small distances (≤few x 10 14 cm) from the star, confirming recent results reported by Decin et al. from observations with Herschel's PACS and SPIRE instruments. This finding definitively rules out the hypothesis that the observed water results from the vaporization of small icy objects in circular orbits. The origin of water within the dense C-rich envelope of IRC+10216 remains poorly understood. We derive upper limits on the H 17 2 O/H 16 2 O and H 18 2 O/H 16 2 O isotopic abundance ratios of ∼5 x 10 -3 (3σ), providing additional constraints on models for the origin of the water vapor in IRC+10216.

  8. Foreword

    Directory of Open Access Journals (Sweden)

    Héctor Cancela

    2017-04-01

    Full Text Available The 20th volume of the CLEI electronic journal includes six papers selected from an open call for papers on Natural Language Processing (NLP, processed by invited editors Gerardo Sierra and César Aguilar, and an additional regular paper. The NLP subject was suggested by Gabriela Marín and Antonio Leoni de León, the chairs of NLPCR 2016, the First Costa-Rican Colloquium on Natural Language Processing. The invited editors took care of the review process and the selection of the six papers, as discussed in their Preface which opens this issue. The additional regular paper is a contribution by Jose Aguilar, Guido Riofrío, and Eduardo Encalada, titled "Learning Analytics focused on student behavior. Case study: dropout in distance learning institutions", which focuses on the use of Learning Analytics for undestanding student behavior in the context of distance learning universities, particularly focuses on the students’ behavior, with the goal of identifying factors that influence the decision of a student to abandon their studies, predicting students susceptible to abandon their studies, and defining their motivational patterns. This issue, which opens the 20th volume of the journal, is a mark of the success of the mission of CLEIej as a vehicle for publishing Latin American based original research in subjects of international interest; we are glad to be able to develop this mission with the support of the researchers who kindly contribute their time as invited editors and reviewers of the papers received.

  9. Cine Club

    CERN Document Server

    Ciné Club

    2013-01-01

    Thursday 22 August 2013 at 20:00 CERN Council Chamber The Angels’ Share Directed by Ken Loach (UK, 2012) Original version English; french subtitles; 101 minute This bitter sweet comedy follows protagonist Robbie as he sneaks into the maternity hospital to visit his young girlfriend Leonie and hold his newborn son Luke for the first time. Overwhelmed by the moment, he swears that Luke will not have the same tragic life he has had. Escaping a prison sentence by the skin of his teeth, he's given one last chance...While serving a community service order, he meets Rhino, Albert and Mo who, like him, find it impossible to find work because of their criminal records. Little did Robbie imagine how turning to drink might change their lives - not cheap fortified wine, but the best malt whiskies in the world. Will it be 'slopping out' for the next twenty years, or a new future with 'Uisge Beatha' the 'Water of Life?' Only the angels know.... Th...

  10. Interferometric Studies of Red Giants with MAPPIT

    Science.gov (United States)

    Ireland, Michael J.

    2002-06-01

    Powerful new tools for the analysis of wavelength-dispersed aperture masking data are presented, as applied to the MAPPIT instrument of the 3.9 m Anglo-Australia Telescope. By using both baseline and wavelength bootstrapping simultaneously, solutions were found for the phase of wavefronts degraded by atmospheric and instrumental effects. This allowed coherent processing of many data sets, greatly improving signal-to-noise both at the longest baselines for well resolved objects, and at all baselines in for data in TiO absorption bands. Using this new techniques, as well as power spectrum-based techniques, wavelength-dependent diameters are found in the range 650-950 nm for the following stars: R Carinae, R Leonis, omicron Ceti, R Hydrae, W Hydrae, R Doradus, L2 Puppis, alpha Orionis, gamma Crucis, eta Carinae and VY Canis Majoris. All the Mira-like stars showed greater than 50% variation in diameter over the available wavelength range. L2 Puppis, a semi-regular variable resolved for the first time, showed a variation in diameter consistent with scattering by a recently ejected shell of dust.

  11. Cine-Club

    CERN Multimedia

    Cine-Club

    2012-01-01

    Thursday 31 May 2012 at 20:30 CERN Council Chamber The Kite Runner By Marc Forster (USA, 2007) With: Khalid Abdalla, Ahmad Khan Mahmoodzada, Atossa Leoni Original version English/Pashtu/Urdu; French subtitles; 128 minutes. In the 70's in Afghanistan, the Pushtun boy Amir and the Hazara boy Hassan, who is his loyal friend and son of their servant Ali, are raised together in Amir's father’s house, playing and kitting on the streets of a peaceful Kabul. After Amir wins a competition of kitting, Hassan runs to bring a kite to Amir, but he is beaten and raped in an empty street to protect Amir's kite; the coward Amir witness the assault but does not help the loyal Hassam. On the day after his birthday party, Amir hides his new watch in Hassam's bed to frame the boy as a thief and force his father to fire Ali, releasing his conscience from recalling his cowardice and betrayal. In 1979, the Russians invade Afghanistan and Baba and Amir escape to Pakistan....

  12. Estrategias gerenciales administrativas para Centros Médicos Privados

    Directory of Open Access Journals (Sweden)

    Thaide Torres Guerra

    2013-01-01

    Full Text Available El problema abordado en este artículo plantea la necesidad de nuevas estrategias gerenciales administrativas para los Centros Médicos Privados de la Parroquia Raúl Leoni del Municipio Maracaibo, con el fin de identificar las fallas, para la mejora del desempeño gerencial. La metodología corresponde a un estudio descriptivo, pues contextualiza el desempeño gerencial administrativo actual en cuanto a las funciones en los centros seleccionados, identificando métodos y test que sirvan para su medición en aspectos relevantes de la planificación, organización, dirección y control. Finalmente se concluye que la estructura organizacional y la caracterización del enfoque confirma con los resultados que el liderazgo, la motivación, comunicación y toma de decisiones, son medianamente efectivas, siendo una debilidad para alcanzar la integración y unificación de los equipos de trabajo y de todos sus miembros que hacen vida en la institución.

  13. Scientific aptitude and academic performance in incoming students of medicine Aptitud científica y rendimiento académico en histología y genética en alumnos de medicina

    Directory of Open Access Journals (Sweden)

    Miguel Angel Vinuesa

    2005-04-01

    Full Text Available Acting scientifically is a competence to be developed by medical students and expressed by them when physicians. The aim of this study was to establish the relationship between scientific aptitude in medical applicants incoming to Rosario Interamerican Open University (UAI and their academic performance in Human Genetics and Histology. Seventy four out of 102 students (29 male and 45 female filled in the aptitude scientific model (ASM designed by D’Ottavio & Bassan (1989. For both, Human Genetics and Histology, performance of the students was considered as satisfactory when they reached a minimum of 85% correct answers in their objective periodic and final examinations. Conversely, lower performance was considered as less than satisfactory. The aforementioned 74 students correctly answered 3.89 ± 1.96 of the 12 ASM problems; average for males was 4.50 ± 1.99 and that for females, 3.48 ± 1.83, (p < 0.025. Students with a satisfactory performance in Histology (n = 34 showed higher scientific aptitude 4.67 ± 2.04 compared with those (n = 40 that had a less than satisfactory one 3.02 ± 1.36 (p <0.001. Significant gender differences were registered: males (n = 14 5.42 ± 2.37 vs. (n = 15 3.20 ± 1.14, p < 0.01, and females (n = 22 4.18 ± 1.56 vs. (n = 23 2.78 ± 1.47, p < 0.01. Concerning Human Genetics, those students with a satisfactory performance (n = 46 revealed higher scientific aptitude: 4.00 ± 2.00 than those with a less than satisfactory one (n = 28: 2.71 ± 1.04, p < 0.01. As in Histology, significant gender differences appeared: males (n = 18 5.22 ± 2.12 vs. (n = 11 3.54 ± 1.21, p < 0.05, and females, (n = 30 3.90 1.70 vs.(n = 15 2.33 ± 1.70, p<0.01. Summing up, in both subject matters students with a satisfactory performance evidenced a higher average of scientific aptitude than that of the studied population. Consequently, we interpret that the degree of scientific aptitude could be a predictive variable of future academic

  14. Two Views of Liberty, Occidental and Oriental(?

    Directory of Open Access Journals (Sweden)

    Bruno Leoni

    2009-02-01

    Full Text Available This paper, by the late Bruno Leoni, was originally presented at a special meeting of the Mont Pèlerin Society (Tokyo, Sept. 5–10, 1966, and was originally published in the Italian journal Il Politico in 1966. The paper displays Leoni’s fondness for Chinese culture, and is essentially a defense of the unity of mankind. Westerners are often of the belief that the Occidental, or Western, individual freedom-based view of liberty is distinct from the Oriental (Eastern view of liberty. Leoni challenges this perspective. Mill believed that disregard for custom was what made the West both free and different from the rest of the world, while the Oriental approach is more backward and based on blind respect for customs. However, custom has often been invoked both in the East and in the West to oppose and limit the power of tyrants, and to defend or to secure civil or political liberty. Mill argued that disregard of custom accounts for novelty, novelty for diversity of character and culture, and the latter for freedom and progress, but there was an unsurpassed diversity of character and culture when Oriental and Occidental people were put together under the rule of the Roman emperors. Furthermore, the “Orient” was not monotonous, dull, and homogeneous, as Mill presumed; to the contrary, Europe cannot show in any period of its history a variety of races, languages, cultures, philosophies and religions even slightly comparable to those of India or China. In fact, Buddha and Confucius were both concerned mainly with individual freedom. Confucius’s theory of society, in particular, was very individualistic; he clearly formulated for the first time in recorded history that principle of “reciprocity,” the “golden rule” for any liberal society. He maintained that the very fundamental principle for a happy society is “Not doing to others what one does not wish them do to one’s self.” Confucius shared, along with the greatest masters of

  15. The effect of a strong stellar flare on the atmospheric chemistry of an earth-like planet orbiting an M dwarf.

    Science.gov (United States)

    Segura, Antígona; Walkowicz, Lucianne M; Meadows, Victoria; Kasting, James; Hawley, Suzanne

    2010-09-01

    Main sequence M stars pose an interesting problem for astrobiology: their abundance in our galaxy makes them likely targets in the hunt for habitable planets, but their strong chromospheric activity produces high-energy radiation and charged particles that may be detrimental to life. We studied the impact of the 1985 April 12 flare from the M dwarf AD Leonis (AD Leo), simulating the effects from both UV radiation and protons on the atmospheric chemistry of a hypothetical, Earth-like planet located within its habitable zone. Based on observations of solar proton events and the Neupert effect, we estimated a proton flux associated with the flare of 5.9 × 10⁸ protons cm⁻² sr⁻¹ s⁻¹ for particles with energies >10 MeV. Then we calculated the abundance of nitrogen oxides produced by the flare by scaling the production of these compounds during a large solar proton event called the Carrington event. The simulations were performed with a 1-D photochemical model coupled to a 1-D radiative/convective model. Our results indicate that the UV radiation emitted during the flare does not produce a significant change in the ozone column depth of the planet. When the action of protons is included, the ozone depletion reaches a maximum of 94% two years after the flare for a planet with no magnetic field. At the peak of the flare, the calculated UV fluxes that reach the surface, in the wavelength ranges that are damaging for life, exceed those received on Earth during less than 100 s. Therefore, flares may not present a direct hazard for life on the surface of an orbiting habitable planet. Given that AD Leo is one of the most magnetically active M dwarfs known, this conclusion should apply to planets around other M dwarfs with lower levels of chromospheric activity.

  16. Die Regenwurmfauna (Oligochaeta: Lumbricidae der Aue der Großen Kokel als Abhängige der Böden im Flusseinzugsgebiet und der Auengradienten

    Directory of Open Access Journals (Sweden)

    Höser, N.

    2011-06-01

    Full Text Available In five floodplain transects along the course of the river Târnava Mare in Rumania, 17 earthworm species werecounted. The species spectrum of the earthworm fauna of the studied floodplains is dependent on the provenance of thefloodplain sediments. On the basis of this provenance, the fauna of three groups of soil localities on the floodplain aredifferentiated: in the upper reaches of the river, the fauna of the floodplain soils derived from brown forest soils and podzolicsoils (near Sub Cetate; on the eastern side of the middle reaches, the fauna of the soils mainly derived from gray-brown podzolicsoils (near Porumbenii Mari, Hoghilag; and on the western side of the middle reaches and the lower reaches, the fauna of thesoils principally derived from planosols (near Alma, Valea Lungă. Proctodrilus tuberculatus occurs in the floodplain sedimentspredominantly derived from the gray-brown podzolic soils, and in those parts of the floodplain derived from planosols P.opisthoductus and Aporrectodea georgii are found. Ap. georgii and Allolobophora leoni are mostly mutually exclusive in thefloodplain transect, were they are apparently indicator species of sediment deposition close to the river and/or the effect of highwater on the soil chemistry. P. tuberculatus and P. opisthoductus occur as vicarious species in the soil profile of the area wheretheir distribution overlaps. Three soil factors that are significant in determining earthworm distribution are emphasized:lessivage, or translocation of clay; the pervection of colloidal organic matter (humus into the soil, and the texture of the soillayers resulting from sedimentation. An additional record of the new species P. thaleri is given.

  17. Taking Charge: Walter Sydney Adams and the Mount Wilson Observatory

    Science.gov (United States)

    Brashear, R.

    2004-12-01

    The growing preeminence of American observational astronomy in the first half of the 20th century is a well-known story and much credit is given to George Ellery Hale and his skill as an observatory-building entrepreneur. But a key figure who has yet to be discussed in great detail is Walter Sydney Adams (1876-1956), Hale's Assistant Director at Mount Wilson Observatory. Due to Hale's illnesses, Adams was Acting Director for much of Hale's tenure, and he became the second Director of Mount Wilson from 1923 to 1946. Behind his New England reserve Adams was instrumental in the growth of Mount Wilson and thus American astronomy in general. Adams was hand-picked by Hale to take charge of stellar spectroscopy work at Yerkes and Mount Wilson and the younger astronomer showed tremendous loyalty to Hale and Hale's vision throughout his career. As Adams assumed the leadership role at Mount Wilson he concentrated on making the observatory a place where researchers worked with great freedom but maintain a high level of cooperation. This paper will concentrate on Adams's early years and look at his growing relationship with Hale and how he came to be the central figure in the early history of Mount Wilson as both a solar and stellar observatory. His education, his years at Dartmouth and Yerkes (including his unfortunate encounter with epsilon Leonis), and his formative years on Mount Wilson are all important in learning how he shaped the direction of Mount Wilson and the development of American astronomy in the first half of the 20th century. This latter history cannot be complete until we bring Adams into better focus.

  18. HERSCHEL/HIFI SEARCH FOR H{sub 2}{sup 17}O AND H{sub 2}{sup 18}O IN IRC+10216: CONSTRAINTS ON MODELS FOR THE ORIGIN OF WATER VAPOR

    Energy Technology Data Exchange (ETDEWEB)

    Neufeld, David A. [Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); Tolls, Volker; Melnick, Gary J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Agundez, Marcelino [LAB, Universite de Bordeaux, UMR 5804, F-33270 Floirac (France); Gonzalez-Alfonso, Eduardo [Universidad de Alcala de Henares, Departamento de Fisica y Matematicas, Campus Universitario, E-28871 Alcala de Henares, Madrid (Spain); Decin, Leen [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, 3001 Leuven (Belgium); Daniel, Fabien; Cernicharo, Jose [Departamento de Astrofisica, Centro de Astrobiologia, CSIC-INTA, Ctra. de Torrejon a Ajalvir km 4, E-28850 Madrid (Spain); Schmidt, Miroslaw; Szczerba, Ryszard [Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Rabianska 8, 87-100 Torun (Poland)

    2013-04-10

    We report the results of a sensitive search for the minor isotopologues of water, H{sub 2}{sup 17}O and H{sub 2}{sup 18}O, toward the carbon-rich asymptotic giant branch star IRC+10216 (a.k.a. CW Leonis) using the HIFI instrument on the Herschel Space Observatory. This search was motivated by the fact that any detection of isotopic enhancement in the H{sub 2}{sup 17}O and H{sub 2}{sup 18}O abundances would have strongly implicated CO photodissociation as the source of the atomic oxygen needed to produce water in a carbon-rich circumstellar envelope. Our observations place an upper limit of 1/470 on the H{sub 2}{sup 17}O/H{sub 2}{sup 16}O abundance ratio. Given the isotopic {sup 17}O/{sup 16}O ratio of 1/840 inferred previously for the photosphere of IRC+10216, this result places an upper limit of a factor 1.8 on the extent of any isotope-selective enhancement of H{sub 2}{sup 17}O in the circumstellar material, and provides an important constraint on any model that invokes CO photodissociation as the source of O for H{sub 2}O production. In the context of the clumpy photodissociation model proposed previously for the origin of water in IRC+10216, our limit implies that {sup 12}C{sup 16}O (not {sup 13}C{sup 16}O or SiO) must be the dominant source of {sup 16}O for H{sub 2}O production, and that the effects of self-shielding can only have reduced the {sup 12}C{sup 16}O photodissociation rate by at most a factor {approx}2.

  19. Selected Abstracts of the 20th National Congress of the Italian Society of Perinatal Medicine (Società Italiana di Medicina Perinatale, SIMP; Catania (Italy; March 22-24, 2018; Session “Perinatal medicine”

    Directory of Open Access Journals (Sweden)

    --- Various Authors

    2018-03-01

    CERVICAL PESSARY FOR PREVEN­TION OF PRETERM BIRTH IN SINGLETON GESTATIONS: FACTORS ASSOCIATED WITH GESTATIONAL AGE AT DELIVERY AND EARLY PESSARY REMOVAL • D. Campana, V. Seravalli, E. Magro-Malosso, M. Aldinucci, M. Di Tommaso, F. PetragliaABS 9. ECHOGRAPHIC DIAGNOSIS OF MARGINAL AND VELAMENTOUS CORD INSERTION: WHICH REAL UTILITY? • M. Andolfatto, S. Visentin, A.P. Londero, I. Dal Molin, E. Riviello, M.G. Sesti, M. Venturini, I. Coati, D. Saraggi, M. Rugge, E. CosmiABS 10. CORRELATIONS BETWEEN BODY COMPOSI­TION CHANGES AND BIOCHEMICAL PA­RAMETERS AND GESTATIONAL DIABETES MELLITUS • L. Di Cerbo, G. Grandi, E. Petrella, I. Neri, F. FacchinettiABS 11. ACCURACY AND CLINICAL UTILITY OF STANDARD POST-MORTEM RADIOLOGICAL IMAGING AFTER EARLY SECOND TRIMESTER TERMINATION OF PREGNANCY FOR CON­GENI­TAL MALFORMATION • I. Fantasia, M. Gregori, R. Bussani, F. Zennaro, G. D’Ottavio, L. Monasta, C. Cortivo, M. Quadrifoglio, G. Maso, G. Ricci, T. StampalijaABS 12. EMOTIONAL AND PSYCHOLOGICAL ASPECTS IN LONGTERM HOSPITALIZED PREGNANT WOMEN • M. Costa, S. Angioni, I. Melis, M. AgusABS 13. POSTPARTUM HAEMORRHAGE AND OB­STETRICAL OUTCOMES IN OOCYTE DONA­TION PREGNANCIES • C. Comito, E. Capannini, F. Lisi, I. Turrini, S. Clemenza, C. Serena, S. Simeone, S. Ottanelli, M.P. Rambaldi, F. Mecacci, F. PetragliaABS 14. FETAL LUNG MATURITY INDUCTION IN LATE PRETERM FETUSES: OUR EXPERIENCE • M.G. Sesti, S. Visentin, C. Florentino, M. Camerin, M. Calanducci, A.P. Londero, E. CosmiABS 15. ARTERIAL BLOOD GAS VALUES OF UMBILICAL CORD: DIFFERENCES BETWEEN UNCLAMPED AND CLAMPED CORD • E. Lanzerotto, E. BusatoABS 16. ABDOMINAL CIRCUMFERENCE GROWTH VELOCITY (ACGV IN PREGNANCIES AT RISK FOR FETAL GROWTH RESTRICTION (FGR • S. Vannuccini, S. Clemenza, S. Simeone, S. Ottanelli, C. Serena, M.P. Rambaldi, F. Lisi, C. Comito, F. Mecacci, F. PetragliaABS 17.  IMPACT OF MODE OF DELIVERY AND PERINEAL MAJOR INJURY ON NEONATAL OUTCOMES • A. Turri, M. Soligo, G. Brembilla, S. Livio, E. De

  20. The Glory of a Nearby Star

    Science.gov (United States)

    2001-08-01

    Optical Light from a Hot Stellar Corona Detected with the VLT Summary The solar corona is a beautiful sight during total solar eclipses . It is the uppermost region of the extended solar atmosphere and consists of a very hot (over 1 million degrees), tenuous plasma of highly ionised elements that emit strong X-ray radiation. There is also a much weaker coronal emission in the optical part of the spectrum . The Sun is a normal star and X-ray observations from rockets and orbiting X-ray telescopes have shown that many other stars also possess coronae . But due to observational limits of the telescopes available so far, the much fainter optical emission from stellar coronae had never been detected. Now, however, an optical coronal line from iron ions that have lost 12 electrons (Fe XIII) has for the first time been observed in a star other than the Sun . The object, a cool star named CN Leonis , is located at a distance of 8 light-years. This impressive observational feat was performed with the UV-Visual Echelle Spectrograph (UVES) on the VLT 8.2-m KUEYEN telescope at the ESO Paranal Observatory , within a programme by German astronomer Jürgen Schmitt and his collaborators at the University of Hamburg Observatory. The possibility to observe stellar coronae with ground-based telescopes opens up new and exciting research opportunities, including the detailed study of stellar cycles , similar to the 11-year solar period. PR Photo 24a/01 : The solar corona during the August 11, 1999, solar eclipse. PR Photo 24b/01 : The nearby star CN Leonis . PR Photo 24c/01 : Ultraviolet spectrum of CN Leonis , obtained with UVES at VLT KUEYEN. PR Photo 24d/01 : The coronal Fe XIII emission line at 3388 Ångstrom in CN Leonis . The 'coronium' mystery ESO PR Photo 24a/01 ESO PR Photo 24a/01 [Preview - JPEG: 450 x 400 pix - 26k] [Normal - JPEG: 899 x 800 pix - 328k] [HiRes - JPEG: 3000 x 2669 pix - 3.1Mk] Caption : Photo of the solar corona, obtained by Philippe Duhoux (ESO) on August 11

  1. The Emergence and Further Development of the Idea of Papal Primacy

    Directory of Open Access Journals (Sweden)

    Mikhail Gratsianskiy

    2015-04-01

    Full Text Available The author analyses how the idea of the papal primacy was formed and developed, papal primacy meaning the particular way in which the place of the bishop of Rome was conceived within the Universal Church. The period in question began with the second century and the emergence of a tradition regarding Peter’s martyrdom in Rome and continued through the papacy of Leo I (440–461. It was Leo who summed up the idea of an exclusive ministry of the Roman pontiff within the Church. The author reviews early testimonies (stretching from the second to the fourth century which note the presence of Peter in Rome, and view him first as a Roman martyr, later as the founder of the Roman episcopal see, and finally as Rome’s first bishop. The idea of the position of Peter in the Church of Rome may be viewed as gradually evolving. The author demonstrates how a rather unreliable ancient tradition connecting the death of Peter with Rome evolved during the fourth and fifth centuries into the idea of Peter as the prince of the apostles (princeps apostolorum, who transmitted his authority or power over the Universal Church to his supposed successors, the bishops of Rome, — an idea which was fully developed by Leo I. The author also wishes to describe the way the Church of Rome was conceived during the first centuries of its existence and underlines the limits of its powers and its susciperent ampliorem, per quos ad unam Petri sedem universalis Ecclesiae cura conflueret, et nihil usquam a suo capite dissideret. Qui ergo scit se quibusdam esse praepositum, non moleste ferat aliquem sibi esse praelatum; sed obedientiam quam exigit, etiam ipse dependat…» (Leonis epistula XIV // PL. T. 54. Col. 676. canonical jurisdiction. It is clear that the concept of the Roman papacy’s universal ministry affording it the possibility to extend its universal jurisdiction over the entire Church within the Roman Empire are based on principles of ecclesiastical

  2. Physical activity in patients with heart failure: barriers and motivations with special focus on sex differences

    Directory of Open Access Journals (Sweden)

    Klompstra L

    2015-11-01

    Full Text Available Leonie Klompstra,1 Tiny Jaarsma,1 Anna Strömberg2,31Department of Social and Welfare Studies, Faculty of Health Sciences, 2Department of Medical and Health Sciences, Division of Nursing, 3Department of Cardiology, Linköping University, Linköping, SwedenBackground: Adherence to recommendations for physical activity is low in both male and female patients with heart failure (HF. Men are more physically active than women. In order to successfully promote physical activity, it is therefore essential to explore how much and why HF patients are physically active and if this is related to sex. The aim of this study was therefore to evaluate physical activity in HF patients, to describe the factors related to physical activity, and to examine potential barriers and motivations to physical activity with special focus on sex differences.Methods: The study had a cross-sectional survey design. HF patients living at home received a questionnaire during May–July 2014, with questions on physical activity (from the Short Form-International Physical Activity Questionnaire, and potential barriers and motivations to physical activity.Results: A total of 154 HF patients, 27% women, with a mean age of 70±10 were included. In total, 23% of the patients reported a high level of physical activity, 46% a moderate level, and 34% a low level. Higher education, self-efficacy, and motivation were significantly associated with a higher amount of physical activity. Symptoms or severity of the disease were not related to physical activity. All the potential barriers to exercise were reported to be of importance. Psychological motivations were most frequently rated as being the most important motivation (41% to be physically active. Physical motivations (33% and social motivations were rated as the least important ones (22%. Women had significantly higher total motivation to be physically active. These differences were found in social, physical, and psychological

  3. [Vulvovaginitis caused by Candida spp. and Trichomonas vaginalis in sexually active women].

    Science.gov (United States)

    Azzam-W, Maha; Cermeño-Vivas, Julman R; Orellán-García, Yida; Penna, Salvador J

    2002-03-01

    Vulvovaginitis accounts for 20 to 30% of gynecological diseases and it is observed in women from 20 to 30 years of age. It has a higher frequency in women using oral contraceptives and during the third trimester of pregnancy. The aim of this research was to assess the prevalence of Candida spp and Trichomonas vaginalis in patients with the diagnosis of vulvovaginitis from the Gynecology Service in Hospital Universitario "Ruiz y Páez" in Ciudad Bolívar and Hospital "Raúl Leoni" in San Félix (Bolívar State, Venezuela). Two hundred women with symptoms of vulvovaginitis were examined, and samples were taken from the uterocervical cul-de-sac. Each patient was asked to fill a questionnaire. The following studies were made in each sample: a) fresh wet mount examination, b) orange acridine and Giemsa stains for Trichomonas and c) culture for the identification of yeasts. The latter were identified by means of the germinal tube assay, resistance to actidione and the presence of clamidospores in rice-cream agar and sugar utilization test, using the commercial kit ID32C (BioMérieux). Only in 57 women of 200 patients with vulvovaginitis the causative agent was demonstrated; Candida spp was present in 84.2% (n = 48) and Trichomonas vaginalis in 14% (n = 8). A single case of Zygosaccharomyces spp (1.8%) was detected. The age group mainly affected was that of 25-35 years old, the 38.6% of the studied population. Candida species detected were: C. albicans in 87% of cases (n = 42), C. glabrata, in 10.42% (n = 5), and C. guillermondii, in 2.08 (n = 1). Vaginal flux, vulvar pruritus and leucorrhoea were observed in significant number of patients with vulvovaginal candidiasis. The use of antibiotics was considered predisposing factor for Trichomonas vaginalis infection. The relationship between age and the etiological agent was not statistically significant. Due to the low specificity of clinical manifestations of infections caused by Candida spp and Trichomonas vaginalis, we

  4. EUV-driven ionospheres and electron transport on extrasolar giant planets orbiting active stars

    Science.gov (United States)

    Chadney, J. M.; Galand, M.; Koskinen, T. T.; Miller, S.; Sanz-Forcada, J.; Unruh, Y. C.; Yelle, R. V.

    2016-03-01

    The composition and structure of the upper atmospheres of extrasolar giant planets (EGPs) are affected by the high-energy spectrum of their host stars from soft X-rays to the extreme ultraviolet (EUV). This emission depends on the activity level of the star, which is primarily determined by its age. In this study, we focus upon EGPs orbiting K- and M-dwarf stars of different ages - ɛ Eridani, AD Leonis, AU Microscopii - and the Sun. X-ray and EUV (XUV) spectra for these stars are constructed using a coronal model. These spectra are used to drive both a thermospheric model and an ionospheric model, providing densities of neutral and ion species. Ionisation - as a result of stellar radiation deposition - is included through photo-ionisation and electron-impact processes. The former is calculated by solving the Lambert-Beer law, while the latter is calculated from a supra-thermal electron transport model. We find that EGP ionospheres at all orbital distances considered (0.1-1 AU) and around all stars selected are dominated by the long-lived H+ ion. In addition, planets with upper atmospheres where H2 is not substantially dissociated (at large orbital distances) have a layer in which H3+ is the major ion at the base of the ionosphere. For fast-rotating planets, densities of short-lived H3+ undergo significant diurnal variations, with the maximum value being driven by the stellar X-ray flux. In contrast, densities of longer-lived H+ show very little day/night variability and the magnitude is driven by the level of stellar EUV flux. The H3+ peak in EGPs with upper atmospheres where H2 is dissociated (orbiting close to their star) under strong stellar illumination is pushed to altitudes below the homopause, where this ion is likely to be destroyed through reactions with heavy species (e.g. hydrocarbons, water). The inclusion of secondary ionisation processes produces significantly enhanced ion and electron densities at altitudes below the main EUV ionisation peak, as

  5. Leslie Peltier, Amateur Astronomer and Observer Extraordinaire

    Science.gov (United States)

    Corbin, B. G.

    2003-12-01

    Leslie Copus Peltier, (Jan. 2, 1900-May 10, 1980) was called "the world's greatest non-professional astronomer" by none other than Harlow Shapley, and also referred to as the "the world's greatest living amateur astronomer". He began observing variable stars on March 1, 1918 with an observation of R. Leonis and at the time of his death had made a total of 132,123 observations of variable stars. These were reported to the AAVSO on a consecutive monthly basis stretching from 1918 to his death in 1980. As of October 2003, he was still on AAVSO's list of the top 25 observers in its history. Born on a farm near Delphos, Ohio, his parents were well read and their home was filled with books on different subjects, including nature guides. As a young man he studied the flora and fauna of the area and in 1915 began his study of the heavens with Vega being the first star he identified. After the purchase of a 2-inch spyglass, his observations of variable stars began to be noticed by professional astronomers and the AAVSO loaned him a 4-inch Mogey refractor; shortly thereafter Henry Norris Russell of Princeton loaned him via the AAVSO a 6-inch refractor, a comet seeker of short focus. He discovered 12 comets, 10 of which carry his name, and 6 novae or recurring novae. His design of the "Merry-Go-Round Observatory" was a novel approach with the whole observatory revolving around the observer while seated in his observing chair. Miami University (Ohio) later donated to him their 12-inch Clark refractor with its dome. His first book, Starlight Nights: The Adventures of a Star-Gazer, appeared in 1965. This autobiography, an ode to the joys of observing both the night sky and nature, was written in beautifully descriptive language that helped lead countless readers into astronomy. Departing from astronomy, in 1977 he published The Place on Jennings Creek. Written in the style of the 19th century naturalist, the book was devoted to his family's home, Brookhaven, and its natural

  6. Mobile Technology Use Across Age Groups in Patients Eligible for Cardiac Rehabilitation: Survey Study.

    Science.gov (United States)

    Gallagher, Robyn; Roach, Kellie; Sadler, Leonie; Glinatsis, Helen; Belshaw, Julie; Kirkness, Ann; Zhang, Ling; Gallagher, Patrick; Paull, Glenn; Gao, Yan; Partridge, Stephanie Ruth; Parker, Helen; Neubeck, Lis

    2017-10-24

    -69 years) was more than twice as likely to use any mobile technology (OR 2.42, 95% CI 1.27-4.59) and mobile technology for health-related purposes (OR 1.92, 95% CI 1.04-3.53). Participants who had completed high school were twice as likely to use mobile technology (OR 2.62, 95% CI 1.45-4.70), mobile apps (OR 2.05, 95% CI 1.09-3.84), and mobile technology for health-related reasons (OR 5.09, 95% CI 2.89-8.95) than those who had not completed high school. Associations were also present between participants living in metropolitan areas and mobile technology use (OR 1.07, 95% CI 1.07-4.24) and employment and mobile app use (OR 2.72, 95% CI 1.44-5.140). Mobile technology offers an important opportunity to improve access to secondary prevention for cardiac patients, particularly when modified to suit subgroups. High levels of mobile technology use and health motivation need to be harnessed for secondary prevention. ©Robyn Gallagher, Kellie Roach, Leonie Sadler, Helen Glinatsis, Julie Belshaw, Ann Kirkness, Ling Zhang, Patrick Gallagher, Glenn Paull, Yan Gao, Stephanie Ruth Partridge, Helen Parker, Lis Neubeck. Originally published in JMIR Mhealth and Uhealth (http://mhealth.jmir.org), 24.10.2017.

  7. Cardiac Patients' Experiences and Perceptions of Social Media: Mixed-Methods Study.

    Science.gov (United States)

    Partridge, Stephanie R; Grunseit, Anne C; Gallagher, Patrick; Freeman, Becky; O'Hara, Blythe J; Neubeck, Lis; Due, Sarah; Paull, Glenn; Ding, Ding; Bauman, Adrian; Phongsavan, Philayrath; Roach, Kellie; Sadler, Leonie; Glinatsis, Helen; Gallagher, Robyn

    2017-09-15

    of Facebook for cardiac rehabilitation and more likely to express interest in providing peer support. Recommended features for a cardiac rehabilitation Facebook group included a closed group, expert cardiac professional involvement, provision of cardiac health information, and ensuring trustworthiness of the group. Cardiac health professionals have an opportunity to capitalize on cardiac patients' motivations and social media, mostly Facebook, as well as the capability for supporting cardiac rehabilitation and secondary prevention. Participants' favored purposeful time spent on Facebook and their cardiac health provides such a purpose for a Facebook intervention. The study results will inform the development of a Facebook intervention for secondary prevention of cardiovascular disease. ©Stephanie R Partridge, Anne C Grunseit, Patrick Gallagher, Becky Freeman, Blythe J O'Hara, Lis Neubeck, Sarah Due, Glenn Paull, Ding Ding, Adrian Bauman, Philayrath Phongsavan, Kellie Roach, Leonie Sadler, Helen Glinatsis, Robyn Gallagher. Originally published in the Journal of Medical Internet Research (http://www.jmir.org), 15.09.2017.

  8. Páginas iniciais

    Directory of Open Access Journals (Sweden)

    Ficha catalográfica e sumário bilíngue

    2013-12-01

    BLICO EM GOIÂNIA – GO – BRASIL QUALITY AND INNOVATION IN PUBLIC TRANSPORTATION SERVICE IN GOIANIA – GO – BRAZIL Maria Regina Silva Lima Bento Alves Costa Filho Cesar Ricardo Maia Vasconcelos CRESCIMENTO OU MANUTENÇÃO DA POSIÇÃO: O DILEMA DOS GESTORES DE UMA INDÚSTRIA DE PLÁSTICOS DA SERRA GAÚCHA GROWTH OR MAINTENANCE OF THE POSITION: THE DILEMMA OF THE MANAGERS OF A PLASTICS INDUSTRY SERRA GAUCHA Julio Cesar Ferro de Guimarães Eliana Andréa Severo Sylvia Maria Azevedo Roesch Pelayo Munhoz Olea Eric Charles Henri Dorion ESTRATÉGIA E COMUNICAÇÃO COM O MERCADO. PERCEPÇÃO DOS GESTORES DAS INSTITUIÇÕES DE ENSINO SUPERIOR SOBRE AS AÇÕES DE RESPONSABILIDADE SOCIAL NA PERSPECTIVA DO MÉTODO FENOMENOLÓGICO STRATEGY AND COMMUNICATION WITH THE MARKET. PERCEPTION OF MANAGERS OF INSTITUTIONS OF HIGHER EDUCATION ON THE CORPORATE SOCIAL RESPONSIBILITY IN THE PHENOMENOLOGICAL METHOD VIEW Roberto Bazanini Ademir Antonio Ferreira Homero Leoni Bazanini Rosalina Florindo da Silva REGIONAL DEVELOPMENT POLICY IN BRAZIL: A REVIEW OF EVALUATION LITERATURE POLÍTICA DE DESENVOLVIMENTO REGIONAL NO BRASIL: UMA REVISÃO DA LITERATURA SOBRE AVALIAÇÃO Guilherme Mendes Resende FLORESTAS E PARTICIPAÇÃO COMO VETORES DO DESENVOLVIMENTO REGIONAL: REFLEXÕES SOBRE OS CASOS ACRE E RIO GRANDE DO SUL FORESTRY AND CIVIC PARTICIPATION AS DRIVERS OF REGIONAL DEVELOPMENT: ANALYSIS OF THE CASES ACRE AND RIO GRANDE DO SUL Markus Erwin Brose A IMPORTÂNCIA DA INTERDISCIPLINARIDADE PARA COMPREENSÃO DAS QUESTÕES AMBIENTAIS THE IMPORTANCE OF INTERDISCIPLINARITY FOR UNDERSTADING OF THE ENVIRONMENTAL SUBJETCTS Cidonea Machado Deponti PROJETOS DE VIDA, MOBILIDADE E METRÓPOLE: AS TRAJETÓRIAS DE JOVENS ADULTOS NO CONTEXTO INTERNACIONAL LIFE PROJECTS, MOBILITY AND METROPOLIS : YOUNG ADULTS’ IN THE INTERNATIONAL CONTEXT Grazielle Betina Brandt Serge Côté

  9. Dos maneras de impulsar el arte: Peggy Guggenheim y Gertrude Vanderbilt

    Directory of Open Access Journals (Sweden)

    Rocamora García Iglesias, Carmen

    2001-03-01

    Full Text Available Not available

    Recogemos en este artículo, la biografía de dos mujeres privilegiadas por la vida.
    Peggy Guggenheim y GertrudeVanderbilt, tuvieron la posibilidad económica y social de impulsar a pintores de distintas procedencias y vanguardias. Sin la primera, el Surrealismo hubiese sido imposible, y, su triunfo, su comprensión y su custodia, se habría esfumado, siendo considerados sus representantes como un grupo de excéntricos deseosos de escandalizar a un público que no entendía su concepto del Arte, y, solo se quedaba en los desenfrenos, las frases sin sentido, las orgías ó el snobismo de algunos de sus representantes.
    La recopilación que hizo Peggy Guggenheim de esta vanguardia, hace comprender al estudioso del Arte que, por detrás de esas arrogancias individuales, había un credo común, un deseo de captar la comprensión del sueño, cuando la razón no está en vigilia, un automatismo psíquico ajeno al razonamiento y, una experimentación de los ámbitos hasta entonces desconocidos como el subconsciente, el azar, la locura ó los estados alucinatorios. Peggy Guggenheim pudo haber empleado su posición económica en viajar, consumir ó tirar su dinero alegremente. No lo hizo así. Su posible excentricidad y sus escándalos, los canalizó por la vía del Arte, ayudando a sus amigos, abriendo Galerías increíbles como la del Soho de Nueva York, en la que: «...Los cuadros estaban montados sobre bates de béisbol, y, las luces se encendían y apagaban componiendo triángulos colgados de cuerdas como si flotaran en el espacio»...
    Y finalmente su auténtico amor por el Arte le llevó a comprar el Pallazo Vernier dei Leoni en Venecia, donde, ya sin excentricidades, el es- pectador puede contemplar y comprender la vanguardia que ella tanto amó. Desde otro punto de vista, Gertrude Vanderbilt, utilizó supuesto en la sociedad para impulsar, no solo a sus amigos sino a aquellos pintores, que, principiantes

  10. Selected Abstracts of the 19th National Congress of the Italian Society of Perinatal Medicine (Società Italiana di Medicina Perinatale, SIMP; Naples (Italy; January 19-21, 2017

    Directory of Open Access Journals (Sweden)

    --- Various Authors

    2017-01-01

    PROSPECTIVE OBSERVATIONAL COHORT STUDY AND CLINICAL AUDIT • F. Monari, E. Petrella, G. Gargano, D. Baronciani, M. Carbone, L. Di Cerbo, A. Coscia, V. Basevi, F. FacchinettiABS 59. A PROSPECTIVE STUDY ON THE USE OF FETAL INTELLIGENT NAVIGATION ECHOCARDIOGRAPHY (FINE • P. Veronese, V.L. Vida, A. Cerutti, S. Rusconi, M.T. GervasiABS 60. CONTINUOUS GLUCOSE MONITORING IN VERY PRETERM INFANTS INCREASES THE TIME SPENT IN EUGLYCEMIA: A RANDOMIZED CONTROLLED TRIAL • A. Galderisi, M. Ghirardo, B. Galeazzo, A. Facchinetti, G. Steil, P. Ortiz-Rubio, E. Baraldi, C. Cobelli, D. TrevisanutoABS 61. IS HYPERGLYCEMIA ASSOCIATED WITH CLINICAL AND/OR PROCEDURAL EVENTS IN VERY LOW BIRTH WEIGHT (VLBW INFANTS? • L. Martini, L. Brombin, A. Galderisi, E. Losiouk, F. Cava, A. Facchinetti, C. Daicampi, E. Baraldi, G. Lanzola, G. Steil, C. Cobelli, D. TrevisanutoABS 62. NASAL CPAP LESIONS AFTER TWO TREATMENT TECHNIQUES (BUBBLE NASAL CPAP VERSUS INFANT FLOW NASAL CPAP IN NEONATAL RESPIRATORY DISTRESS SYNDROME • E. Jazexhiu–Postoli, E. Vevecka, E. Petrela, E. RapushiABS 63. MODIFICATIONS OF THE PERCENTAGE OF BREASTFEEDING IN A COHORT OF PREMATURE BABIES ACCORDING TO THE UNICEF PROJECT – BABY FRIENDLY HOSPITAL (BFH • A.F. Moscatiello, L. Pogliani, P. Pileri, I. Cetin, G.V. ZuccottiABS 64. METABOLOMICS (NMR, GC-MS AS A TOOL FOR INDIVIDUALIZED MEDICINE IN INFANTS WITH NEC: IS GLUCONIC ACID A NEW BIOMARKER? • R. Pintus, A. Dessì, F. Cesare Marincola, S. Corbu, A. De Magistris, L. Barberini, C. Fattuoni, A. Noto, M. Puddu, J.C. Picaud, V. FanosABS 65. THE DURATION OF UMBILICAL CORD PULSATILITY AFTER A VAGINAL DELIVERY IN WOMEN WITH A SINGLETON PREGNANCY AT TERM: AN OBSERVATIONAL STUDY • E.R. Magro Malosso, B. Carotenuto, S. Pinzauti, M. Torricelli, S. D’Ottavio, M. Di TommasoABS 66. MATERNAL AND PERINATAL OUTCOMES IN PREGNANCIES DERIVING FROM ASSISTED REPRODUCTIVE TECHNOLOGIES (ART • F. Perelli, D. Campana, M. Torricelli, L. Troia, M. Di TommasoABS 67. REDUCED SHORT TERM VARIATION

  11. EDITORIAL: Focus on Quantum Cryptography: Theory and Practice FOCUS ON QUANTUM CRYPTOGRAPHY: THEORY AND PRACTICE

    Science.gov (United States)

    Lütkenhaus, N.; Shields, A. J.

    2009-04-01

    distribution network in Vienna M Peev, C Pacher, R Alléaume, C Barreiro, J Bouda, W Boxleitner, T Debuisschert, E Diamanti, M Dianati, J F Dynes, S Fasel, S Fossier, M Fürst, J-D Gautier, O Gay, N Gisin, P Grangier, A Happe, Y Hasani, M Hentschel, H Hübel, G Humer, T Länger, M Legré, R Lieger, J Lodewyck, T Lorünser, N Lütkenhaus, A Marhold, T Matyus, O Maurhart, L Monat, S Nauerth, J-B Page, A Poppe, E Querasser, G Ribordy, S Robyr, L Salvail, A W Sharpe, A J Shields, D Stucki, M Suda, C Tamas, T Themel, R T Thew, Y Thoma, A Treiber, P Trinkler, R Tualle-Brouri, F Vannel, N Walenta, H Weier, H Weinfurter, I Wimberger, Z L Yuan, H Zbinden and A Zeilinger Stable quantum key distribution with active polarization control based on time-division multiplexing J Chen, G Wu, L Xu, X Gu, E Wu and H Zeng Controlling passively quenched single photon detectors by bright light Vadim Makarov Information leakage via side channels in freespace BB84 quantum cryptography Sebastian Nauerth, Martin Fürst, Tobias Schmitt-Manderbach, Henning Weier and Harald Weinfurter Standardization of quantum key distribution and the ETSI standardization initiative ISG-QKD Thomas Länger and Gaby Lenhart Entangled quantum key distribution with a biased basis choice Chris Erven, Xiongfeng Ma, Raymond Laflamme and Gregor Weihs Finite-key analysis for practical implementations of quantum key distribution Raymond Y Q Cai and Valerio Scarani Field test of a continuous-variable quantum key distribution prototype S Fossier, E Diamanti, T Debuisschert, A Villing, R Tualle-Brouri and P Grangier Physics and application of photon number resolving detectors based on superconducting parallel nanowires F Marsili, D Bitauld, A Gaggero, S Jahanmirinejad, R Leoni, F Mattioli and A Fiore Device-independent quantum key distribution secure against collective attacks Stefano Pironio, Antonio Acín, Nicolas Brunner, Nicolas Gisin, Serge Massar and Valerio Scarani 1310 nm differential-phase-shift QKD system using

  12. 5th National Congress of the Italian Society of Physiotherapy

    Directory of Open Access Journals (Sweden)

    Alessandro Aina

    2016-10-01

    knee prosthesis Cislaghi M, Penone G, Marinelli G, Rezzan G, Melegati G, Gatti R P14 The use of Kinesio Taping in the treatment of hematomas: can we distinguish fancy from the effects? Colombo Claudio, Tolosa Francesca, Andrea Moriondo, Vercelli Stefano P15 Who is able to perform explicit motor imagery after stroke? Stefano Doronzio, Matteo Paci P16 Responsiveness of the Bridge tests in Symptomatic Lumbar Spondylolisthesis Silvano Ferrari, Carla Vanti, Marco Monticone P17 The relationship between number of sessions and clinical results in lumbar symptomatic spondylolisthesis Silvano Ferrari, Carla Vanti, Marco Monticone P18 Conservative treatments for upper extremity tendinopathies in occupational medicine: narrative review Garzonio Fabiola, Zanetta Anna, Bargeri Serena, Cerone Giorgia, Sartorio Francesco P19 The time-related effect of roller-massager on extensibility of the hamstring muscles Filippo Ghirlanda, Alessandro Schneebeli, Corrado Cescon, Marco Barbero P20 Effect of two different exercise programs on pain, disability and quality of life in people with subacute and chronic nonspecific neck pain Gioia G, Faccendini S, Aina A, Tettamanti A P21 A bridge between clinical practice and research: how health professionals can study literature and learn on the job Granzotto G, Coppola L, Gava I, Frassinelli M, Gattinoni F P22 Walking capacity improves after neuromotor physiotherapy in stroke patients Lorenzo Guidotti, Marco Postiglione, Bruna Lombardi, Matteo Paci P23 Intra and inter-session reliability of the angle between pain onset and submaximal pain during upper limb neurodynamics test 1: a study in healty individuals Diego Leoni, Davide Storer, Roberto Gatti, Michele Egloff, Marco Barbero P24 Effects of an AO-MI training on balance task in patients affected by multiple sclerosis Magno Tiziano, Tettamanti Andrea P25 Outcomes of treatment with neuromuscular stimulator for chronic anterior knee pain: a clinical case Daniele Maremmani, Sebastiano Cencini, Giuseppe

  13. ESA's Hipparcos satellite revises the scale of the cosmos

    Science.gov (United States)

    1997-02-01

    not recognized as fast pulsators they would give false impressions in the Cepheid distance scale. The miraculous stars Another famous variable star pulsates at more than twice the frequency that theorists would expect. This is Mira, the prototype of the class of stars investigated by Floor van Leeuwen and his colleagues, using the Hipparcos data. To an unaided eye, Omicron Ceti appears and disappears in a cycle of 11 months. In the 17th Century astronomers named it Mira, the miraculous star. Astrophysicists today interpret Mira as a senile star slightly more massive than the Sun. It has swollen into a red giant and started oscillating, as a prelude to greater instabilities that will in due course fling the outer layers of the star into space. Hipparcos fixes Mira's distance at 420 light-years. Other astronomers have gauged the apparent width of the star, as seen from the ground, so the Hipparcos team can compute the diameter of Mira as 650 million kilometres -- somewhat wider than the orbit of Mars. If the Sun were in Mira's state it would swallow up the Earth and all of the inner planets. Astronomers knew that Mira was big, but the Hipparcos result confirms that it is too large to be oscillating in a simple fashion. Again its variation is an overtone, and the same is true of some other variable stars of the same type, known collectively as the Miras. The sixteen Miras in the survey are mostly 300-1000 light-years away, at distances more comfortably within the grasp of Hipparcos parallaxes. Before Hipparcos, there was only one fairly good measurement of a Mira distance, for the star R Leonis. Even in that case, Hipparcos adjusts the distance from 390 to 330 light-years. Patricia Whitelock of the South African Astronomical Observatory played a prominent part in the Mira study. In preparation for the Hipparcos data, observations of selected Miras from South Africa and Russia, with infrared instruments, assessed the extent to which they are dimmed by dust. Taking this