The Abel Prize

CERN Document Server

Holden, Helge

2010-01-01

Presents the winners of the first five Abel Prizes in mathematics: 2003 - Jean-Pierre Serre; 2004 - Sir Michael Atiyah and Isadore Singer; 2005 - Peter D Lax; 2006 - Lennart Carleson; and 2007 - S R Srinivasa Varadhan. This book provides an autobiography or an interview, a curriculum vitae, and a complete bibliography of each laureate

New distances to and peculiar motions of two Abell clusters -evidence for spurious motions?

International Nuclear Information System (INIS)

Lucey, J.R.; Terlevich, R.J.

1991-01-01

We present redshifts and central velocity dispersions (σ) from observations with the FLEX-based multi-object system on the William Herschel 4.2-m telescope for early-type galaxies in three rich clusters, Abell 194, Abell 2199 and Abell 2634. For Abell 194, the new measurements are in excellent agreement with those previously derived with the AAT's FOCAP multi-object system. Photometric diameters (D) derived from CCD observations made with the Isaac Newton 2.5-m telescope and Jacobus Kapteyn 1.0-m telescope are also presented. Relative distances to Abell 2199 and Abell 2634 are derived via the application of the D-σ relation. (author)

The correlation functions for the clustering of galaxies and Abell clusters

International Nuclear Information System (INIS)

Jones, B.J.T.; Jones, J.E.; Copenhagen Univ.

1985-01-01

The difference in amplitudes between the galaxy-galaxy correlation function and the correlation function between Abell clusters is a consequence of two facts. Firstly, most Abell clusters with z<0.08 lie in a relatively small volume of the sampled space, and secondly, the fraction of galaxies lying in Abell clusters differs considerably inside and outside of this volume. (The Abell clusters are confined to a smaller volume of space than are the galaxies.) We discuss the implications of this interpretation of the clustering correlation functions and present a simple model showing how such a situation may arise quite naturally in standard theories for galaxy formation. (orig.)

Interview with Abel Prize Recipient Srinivasa Varadhan

DEFF Research Database (Denmark)

Raussen, Martin; Skau, Christian

2008-01-01

His Majesty King Harald presented the Abel Prize for 2007 to Srinivasa Varadhan at an award ceremony in the University Aula in Oslo on the 22nd May, 2007. The interview was conducted the day before the ceremony.......His Majesty King Harald presented the Abel Prize for 2007 to Srinivasa Varadhan at an award ceremony in the University Aula in Oslo on the 22nd May, 2007. The interview was conducted the day before the ceremony....

An Abel type cubic system

Directory of Open Access Journals (Sweden)

Gary R. Nicklason

2015-07-01

Full Text Available We consider center conditions for plane polynomial systems of Abel type consisting of a linear center perturbed by the sum of 2 homogeneous polynomials of degrees n and 2n-1 where $n \\ge 2$. Using properties of Abel equations we obtain two general systems valid for arbitrary values on n. For the cubic n=2 systems we find several sets of new center conditions, some of which show that the results in a paper by Hill, Lloyd and Pearson which were conjectured to be complete are in fact not complete. We also present a particular system which appears to be a counterexample to a conjecture by Zoladek et al. regarding rational reversibility in cubic polynomial systems.

Video of Christian Skau and Martin Raussen's interview with the Abel Prize Winner John Milnor

DEFF Research Database (Denmark)

Skau, Christian

2011-01-01

The television interview with Abel Laureate John Milnor that was broadcasted on Norwegian television in June is now available on the Abel Prize multimedia page. John Milnor received the Abel Prize «for pioneering discoveries in topology, geometry and algebra» to quote the Abel Committee. King...... Harald presented the Abel Prize to John Milnor at the award ceremony in Oslo, Norway on 24 May. Before the interview there is a short presentation of the award ceremony. John Milnor is interviewed by Martin Raussen and Christian Skau. The Abel Prize that carries a cash award of NOK 6 million (about EUR...

Tauberian theorems for Abel summability of sequences of fuzzy numbers

Science.gov (United States)

Yavuz, Enes; ćoşkun, Hüsamettin

2015-09-01

We give some conditions under which Abel summable sequences of fuzzy numbers are convergent. As corollaries we obtain the results given in [E. Yavuz, Ö. Talo, Abel summability of sequences of fuzzy numbers, Soft computing 2014, doi: 10.1007/s00500-014-1563-7].

El teorema de Abel para la lemniscata Abel's theorem on the lemniscate

Directory of Open Access Journals (Sweden)

Leonardo Solanilla Ch.

2010-07-01

Full Text Available En este artículo demostramos el teorema de Abel para la lemniscata sin la ayuda de la teoría de las funciones elípticas y sin referencia alguna a la moderna teoría de campos. Los ingredientes esenciales de la demostración son las funciones lemniscáticas de Gauss y algunas nociones elementales sobre factorización en el anillo de los polinomios con coeficientes racionales. El procedimiento es muy poderoso. En verdad, no sólo probamos que la construcción geométrica es posible, sino que indicamos las operaciones algebraicas que realizan la construcción.In this article, Abel's theorem for lemniscates has been demonstrated without the help of elliptical function theory and without any reference to the modern theory of fields. Essential ingredients of the demonstration are Gauss' lemniscates functions and some elementary on factorization in the ring of rational coefficients. The procedure is very powerful. It was proved that geometric construction is possible. Algebraic operations which indicated the construction were also indicated.

Radio emission of Abell Clusters in the GB region

International Nuclear Information System (INIS)

Michalec, A.

1977-01-01

In the GB survey region (Maslowski 1972) there are 102 Abell Clusters (Abell 1958) 31 of them coincide with the positions of Gb radio sources. The number of random coincidences was estimated from a Poisson distribution. For 19 cluster from this group, the observations at 2695 MHz were made with the same instrument. The clusters' redshifts were estimated. On the basis of this material, an analysis of the luminosity function for these cluster was carried out. (author)

A variational regularization of Abel transform for GPS radio occultation

OpenAIRE

T.-K. Wee

2018-01-01

In the Global Positioning System (GPS) radio occultation (RO) technique, the inverse Abel transform of measured bending angle (Abel inversion, hereafter AI) is the standard means of deriving the refractivity. While concise and straightforward to apply, the AI accumulates and propagates the measurement error downward. The measurement error propagation is detrimental to the refractivity in lower altitudes. In particular, it builds up negative refractivity bias in the tropical ...

ON THE EQUIVALENCE OF THE ABEL EQUATION

Institute of Scientific and Technical Information of China (English)

无

2006-01-01

This article uses the reflecting function of Mironenko to study some complicated differential equations which are equivalent to the Abel equation. The results are applied to discuss the behavior of solutions of these complicated differential equations.

The GenABEL Project for statistical genomics.

Science.gov (United States)

Karssen, Lennart C; van Duijn, Cornelia M; Aulchenko, Yurii S

2016-01-01

Development of free/libre open source software is usually done by a community of people with an interest in the tool. For scientific software, however, this is less often the case. Most scientific software is written by only a few authors, often a student working on a thesis. Once the paper describing the tool has been published, the tool is no longer developed further and is left to its own device. Here we describe the broad, multidisciplinary community we formed around a set of tools for statistical genomics. The GenABEL project for statistical omics actively promotes open interdisciplinary development of statistical methodology and its implementation in efficient and user-friendly software under an open source licence. The software tools developed withing the project collectively make up the GenABEL suite, which currently consists of eleven tools. The open framework of the project actively encourages involvement of the community in all stages, from formulation of methodological ideas to application of software to specific data sets. A web forum is used to channel user questions and discussions, further promoting the use of the GenABEL suite. Developer discussions take place on a dedicated mailing list, and development is further supported by robust development practices including use of public version control, code review and continuous integration. Use of this open science model attracts contributions from users and developers outside the "core team", facilitating agile statistical omics methodology development and fast dissemination.

The Abel Symposium 2013

CERN Document Server

Irgens, Marius; Wold, Erlend

2015-01-01

This book focuses on complex geometry and covers highly active topics centered around geometric problems in several complex variables and complex dynamics, written by some of the world’s leading experts in their respective fields. This book features research and expository contributions from the 2013 Abel Symposium, held at the Norwegian University of Science and Technology Trondheim on July 2-5, 2013. The purpose of the symposium was to present the state of the art on the topics, and to discuss future research directions.

Generalization of Abel's mechanical problem: The extended isochronicity condition and the superposition principle

Energy Technology Data Exchange (ETDEWEB)

Kinugawa, Tohru, E-mail: kinugawa@phoenix.kobe-u.ac.jp [Institute for Promotion of Higher Education, Kobe University, Kobe 657-8501 (Japan)

2014-02-15

This paper presents a simple but nontrivial generalization of Abel's mechanical problem, based on the extended isochronicity condition and the superposition principle. There are two primary aims. The first one is to reveal the linear relation between the transit-time T and the travel-length X hidden behind the isochronicity problem that is usually discussed in terms of the nonlinear equation of motion (d{sup 2}X)/(dt{sup 2}) +(dU)/(dX) =0 with U(X) being an unknown potential. Second, the isochronicity condition is extended for the possible Abel-transform approach to designing the isochronous trajectories of charged particles in spectrometers and/or accelerators for time-resolving experiments. Our approach is based on the integral formula for the oscillatory motion by Landau and Lifshitz [Mechanics (Pergamon, Oxford, 1976), pp. 27–29]. The same formula is used to treat the non-periodic motion that is driven by U(X). Specifically, this unknown potential is determined by the (linear) Abel transform X(U) ∝ A[T(E)], where X(U) is the inverse function of U(X), A=(1/√(π))∫{sub 0}{sup E}dU/√(E−U) is the so-called Abel operator, and T(E) is the prescribed transit-time for a particle with energy E to spend in the region of interest. Based on this Abel-transform approach, we have introduced the extended isochronicity condition: typically, τ = T{sub A}(E) + T{sub N}(E) where τ is a constant period, T{sub A}(E) is the transit-time in the Abel type [A-type] region spanning X > 0 and T{sub N}(E) is that in the Non-Abel type [N-type] region covering X < 0. As for the A-type region in X > 0, the unknown inverse function X{sub A}(U) is determined from T{sub A}(E) via the Abel-transform relation X{sub A}(U) ∝ A[T{sub A}(E)]. In contrast, the N-type region in X < 0 does not ensure this linear relation: the region is covered with a predetermined potential U{sub N}(X) of some arbitrary choice, not necessarily obeying the Abel-transform relation. In

Abel inverse transformation applied to plasma diagnostics

International Nuclear Information System (INIS)

Zhu Shiyao

1987-01-01

Two methods of Abel inverse transformation are applied to two different test profiles. The effects of random errors of input data, position uncertainty and number of points of input data on the accuracy of inverse transformation have been studied. The two methods are compared in each other

4th Abel Symposium

CERN Document Server

Friedlander, Eric; Jahren, Björn; Østvær, Paul

2009-01-01

The 2007 Abel Symposium took place at the University of Oslo in August 2007. The goal of the symposium was to bring together mathematicians whose research efforts have led to recent advances in algebraic geometry, algebraic K-theory, algebraic topology, and mathematical physics. A common theme of this symposium was the development of new perspectives and new constructions with a categorical flavor. As the lectures at the symposium and the papers of this volume demonstrate, these perspectives and constructions have enabled a broadening of vistas, a synergy between once-differentiated subjects, and solutions to mathematical problems both old and new.

IMAGING AND SPECTROSCOPY OF ABELL-63 (UU SGE)

NARCIS (Netherlands)

WALTON, NA; WALSH, [No Value; POTTASCH, [No Value

UU Sge, the eclipsing binary central star of the low-surface-brightness planetary nebula (PN) Abell 63, has been observed spectroscopically in the visible throughout its 11.2 hour period and especially during the minimum. A determination of the spectral types of the components of the binary system

The Abel symposium 2008 on differential equations: geometry, symmetries and integrability

CERN Document Server

Lychagin, Valentin; Straume, Eldar; Abel symposium 2008; Differential equations; Geometry, symmetries and integrability

2008-01-01

The Abel Symposium 2008 focused on the modern theory of differential equations and their applications in geometry, mechanics, and mathematical physics. Following the tradition of Monge, Abel and Lie, the scientific program emphasized the role of algebro-geometric methods, which nowadays permeate all mathematical models in natural and engineering sciences. The ideas of invariance and symmetry are of fundamental importance in the geometric approach to differential equations, with a serious impact coming from the area of integrable systems and field theories. This volume consists of original contributions and broad overview lectures of the participants of the Symposium. The papers in this volume present the modern approach to this classical subject.

An Analytical Method for the Abel Inversion of Asymmetrical Gaussian Profiles

International Nuclear Information System (INIS)

Xu Guosheng; Wan Baonian

2007-01-01

An analytical algorithm for fast calculation of the Abel inversion for density profile measurement in tokamak is developed. Based upon the assumptions that the particle source is negligibly small in the plasma core region, density profiles can be approximated by an asymmetrical Gaussian distribution controlled only by one parameter V 0 /D and V 0 /D is constant along the radial direction, the analytical algorithm is presented and examined against a testing profile. The validity is confirmed by benchmark with the standard Abel inversion method and the theoretical profile. The scope of application as well as the error analysis is also discussed in detail

The radiation linked to uranium natural radioactivity enlightened by Abel Niepce long time before Henri Becquerel;Les rayonnements lies a la radioactivite naturelle de l'uranium mis en evidence par Abel Niepce bien avant Henri Becquerel

Energy Technology Data Exchange (ETDEWEB)

Fournier, J.; Niepce, J.C.

2009-09-15

Abel Niepce was rarely mentioned during the celebration of the centenary of the radioactivity discovery.This discovery, supposed due to chance alone, is entirely attributed to Henri Becquerel. But Abel Niepce who made the first observation of radiation from uranium with the impression of a photographic plate, but without giving it meaning. This is a slow process which in forty years, from an observation misunderstood by Abel Niepce to its interpretation by Frederick Soddy, through the experiments of Henri Becquerel and thanks to developments in other knowledge (electron, X-rays) has led to a scientific progress known under the term of radioactivity, name given by Marie Slodowska-Curie. (N.C.)

Integrable dissipative nonlinear second order differential equations via factorizations and Abel equations

Energy Technology Data Exchange (ETDEWEB)

Mancas, Stefan C. [Department of Mathematics, Embry–Riddle Aeronautical University, Daytona Beach, FL 32114-3900 (United States); Rosu, Haret C., E-mail: hcr@ipicyt.edu.mx [IPICYT, Instituto Potosino de Investigacion Cientifica y Tecnologica, Apdo Postal 3-74 Tangamanga, 78231 San Luis Potosí, SLP (Mexico)

2013-09-02

We emphasize two connections, one well known and another less known, between the dissipative nonlinear second order differential equations and the Abel equations which in their first-kind form have only cubic and quadratic terms. Then, employing an old integrability criterion due to Chiellini, we introduce the corresponding integrable dissipative equations. For illustration, we present the cases of some integrable dissipative Fisher, nonlinear pendulum, and Burgers–Huxley type equations which are obtained in this way and can be of interest in applications. We also show how to obtain Abel solutions directly from the factorization of second order nonlinear equations.

Non-thermal pressure in the outskirts of Abell 2142

Science.gov (United States)

Fusco-Femiano, Roberto; Lapi, Andrea

2018-03-01

Clumping and turbulence are expected to affect the matter accreted on to the outskirts of galaxy clusters. To determine their impact on the thermodynamic properties of Abell 2142, we perform an analysis of the X-ray temperature data from XMM-Newton via our SuperModel, a state-of-the-art tool for investigating the astrophysics of the intracluster medium already tested on many individual clusters (since Cavaliere, Lapi & Fusco-Femiano 2009). Using the gas density profile corrected for clumpiness derived by Tchernin et al. (2016), we find evidence for the presence of a non-thermal pressure component required to sustain gravity in the cluster outskirts of Abell 2142, that amounts to about 30 per cent of the total pressure at the virial radius. The presence of the non-thermal component implies the gas fraction to be consistent with the universal value at the virial radius and the electron thermal pressure profile to be in good agreement with that inferred from the SZ data. Our results indicate that the presence of gas clumping and of a non-thermal pressure component are both necessary to recover the observed physical properties in the cluster outskirts. Moreover, we stress that an alternative method often exploited in the literature (included Abell 2142) to determine the temperature profile kBT = Pe/ne basing on a combination of the Sunyaev-Zel'dovich (SZ) pressure Pe and of the X-ray electron density ne does not allow us to highlight the presence of non-thermal pressure support in the cluster outskirts.

The generalized Abel-Plana formula. Applications to Bessel functions and Casimir effect

International Nuclear Information System (INIS)

Saharian, A.A.; Institute of Applied Problems in Physics NAS RA, Yerevan; Abdus Salam International Centre for Theoretical Physics, Trieste

2000-02-01

One of the most efficient methods to obtain the vacuum expectation values for the physical observables in the Casimir effect is based on using the Abel-Plana summation formula. This allows us to derive the regularized quantities in a manifestly cutoff independent way and present them in the form of strongly convergent integrals. However, the application of Abel-Plana formula, in its usual form, is restricted by simple geometries when the eigenmodes have a simple dependence on quantum numbers. The author generalized the Abel-Plana formula which essentially enlarges its application range. Based on this generalization, formulae have been obtained for various types of series over the zeros of some combinations of Bessel functions and for integrals involving these functions. It has been shown that these results generalize the special cases existing in literature. Further, the derived summation formulae have been used to summarize series arising in the mode summation approach to the Casimir effect for spherically and cylindrically symmetric boundaries. This allows us to extract the divergent parts from the vacuum expectation values for the local physical observables in a manifestly cutoff independent way. The present paper reviews these results. Some new considerations are also added. (author)

Abell 48 - a rare WN-type central star of a planetary nebula

Science.gov (United States)

Todt, H.; Kniazev, A. Y.; Gvaramadze, V. V.; Hamann, W.-R.; Buckley, D.; Crause, L.; Crawford, S. M.; Gulbis, A. A. S.; Hettlage, C.; Hooper, E.; Husser, T.-O.; Kotze, P.; Loaring, N.; Nordsieck, K. H.; O'Donoghue, D.; Pickering, T.; Potter, S.; Romero-Colmenero, E.; Vaisanen, P.; Williams, T.; Wolf, M.

2013-04-01

A considerable fraction of the central stars of planetary nebulae (CSPNe) are hydrogen-deficient. Almost all of these H-deficient central stars (CSs) display spectra with strong carbon and helium lines. Most of them exhibit emission-line spectra resembling those of massive WC stars. Therefore these stars are classed as CSPNe of spectral type [WC]. Recently, quantitative spectral analysis of two emission-line CSs, PB 8 and IC 4663, revealed that these stars do not belong to the [WC] class. Instead PB 8 has been classified as [WN/WC] type and IC 4663 as [WN] type. In this work we report the spectroscopic identification of another rare [WN] star, the CS of Abell 48. We performed a spectral analysis of Abell 48 with the Potsdam Wolf-Rayet (PoWR) models for expanding atmospheres. We find that the expanding atmosphere of Abell 48 is mainly composed of helium (85 per cent by mass), hydrogen (10 per cent) and nitrogen (5 per cent). The residual hydrogen and the enhanced nitrogen abundance make this object different from the other [WN] star IC 4663. We discuss the possible origin of this atmospheric composition.

Protective effect of Camellia oleifera Abel. on silica-induced ...

African Journals Online (AJOL)

Background: Camellia oleifera Abel. belongs to the family Theaceae and genus Camellia. It is commonly cultivated in southern China. The seeds of C. oleifera have been reported to exhibit a diversity of pharmacological activities which include, but are not limited to, antioxidant, anti-cancer and antimicrobial. Pulmonary ...

A variational regularization of Abel transform for GPS radio occultation

Directory of Open Access Journals (Sweden)

T.-K. Wee

2018-04-01

Full Text Available In the Global Positioning System (GPS radio occultation (RO technique, the inverse Abel transform of measured bending angle (Abel inversion, hereafter AI is the standard means of deriving the refractivity. While concise and straightforward to apply, the AI accumulates and propagates the measurement error downward. The measurement error propagation is detrimental to the refractivity in lower altitudes. In particular, it builds up negative refractivity bias in the tropical lower troposphere. An alternative to AI is the numerical inversion of the forward Abel transform, which does not incur the integration of error-possessing measurement and thus precludes the error propagation. The variational regularization (VR proposed in this study approximates the inversion of the forward Abel transform by an optimization problem in which the regularized solution describes the measurement as closely as possible within the measurement's considered accuracy. The optimization problem is then solved iteratively by means of the adjoint technique. VR is formulated with error covariance matrices, which permit a rigorous incorporation of prior information on measurement error characteristics and the solution's desired behavior into the regularization. VR holds the control variable in the measurement space to take advantage of the posterior height determination and to negate the measurement error due to the mismodeling of the refractional radius. The advantages of having the solution and the measurement in the same space are elaborated using a purposely corrupted synthetic sounding with a known true solution. The competency of VR relative to AI is validated with a large number of actual RO soundings. The comparison to nearby radiosonde observations shows that VR attains considerably smaller random and systematic errors compared to AI. A noteworthy finding is that in the heights and areas that the measurement bias is supposedly small, VR follows AI very closely in the

A variational regularization of Abel transform for GPS radio occultation

Science.gov (United States)

Wee, Tae-Kwon

2018-04-01

In the Global Positioning System (GPS) radio occultation (RO) technique, the inverse Abel transform of measured bending angle (Abel inversion, hereafter AI) is the standard means of deriving the refractivity. While concise and straightforward to apply, the AI accumulates and propagates the measurement error downward. The measurement error propagation is detrimental to the refractivity in lower altitudes. In particular, it builds up negative refractivity bias in the tropical lower troposphere. An alternative to AI is the numerical inversion of the forward Abel transform, which does not incur the integration of error-possessing measurement and thus precludes the error propagation. The variational regularization (VR) proposed in this study approximates the inversion of the forward Abel transform by an optimization problem in which the regularized solution describes the measurement as closely as possible within the measurement's considered accuracy. The optimization problem is then solved iteratively by means of the adjoint technique. VR is formulated with error covariance matrices, which permit a rigorous incorporation of prior information on measurement error characteristics and the solution's desired behavior into the regularization. VR holds the control variable in the measurement space to take advantage of the posterior height determination and to negate the measurement error due to the mismodeling of the refractional radius. The advantages of having the solution and the measurement in the same space are elaborated using a purposely corrupted synthetic sounding with a known true solution. The competency of VR relative to AI is validated with a large number of actual RO soundings. The comparison to nearby radiosonde observations shows that VR attains considerably smaller random and systematic errors compared to AI. A noteworthy finding is that in the heights and areas that the measurement bias is supposedly small, VR follows AI very closely in the mean refractivity

On the interpretation of dark matter self-interactions in Abell 3827

International Nuclear Information System (INIS)

Kahlhoefer, Felix; Schmidt-Hoberg, Kai; Kummer, Janis; Sarkar, Subir

2015-04-01

Self-interactions of dark matter particles can potentially lead to an observable separation between the dark matter halo and the stars of a galaxy moving through a region of large dark matter density. Such a separation has recently been observed in a galaxy falling into the core of the galaxy cluster Abell 3827. We estimated the DM self-interaction cross section needed to reproduce the observed effects and find that the sensitivity of Abell 3827 has been significantly overestimated in a previous study. Our corrected estimate is σ/m DM ∝3 cm 2 g -1 when self-interactions result in an effective drag force and σ/m DM ∝ 1.5 cm 2 g -1 for the case of contact interactions, in some tension with previous upper bounds.

3rd Abel Symposium

CERN Document Server

Owren, Brynjulf

2008-01-01

The 2006 Abel symposium is focusing on contemporary research involving interaction between computer science, computational science and mathematics. In recent years, computation has been affecting pure mathematics in fundamental ways. Conversely, ideas and methods of pure mathematics are becoming increasingly important within computational and applied mathematics. At the core of computer science is the study of computability and complexity for discrete mathematical structures. Studying the foundations of computational mathematics raises similar questions concerning continuous mathematical structures. There are several reasons for these developments. The exponential growth of computing power is bringing computational methods into ever new application areas. Equally important is the advance of software and programming languages, which to an increasing degree allows the representation of abstract mathematical structures in program code. Symbolic computing is bringing algorithms from mathematical analysis into the...

Serre duality, Abel's theorem, and Jacobi inversion for supercurves over a thick superpoint

Science.gov (United States)

Rothstein, Mitchell J.; Rabin, Jeffrey M.

2015-04-01

The principal aim of this paper is to extend Abel's theorem to the setting of complex supermanifolds of dimension 1 | q over a finite-dimensional local supercommutative C-algebra. The theorem is proved by establishing a compatibility of Serre duality for the supercurve with Poincaré duality on the reduced curve. We include an elementary algebraic proof of the requisite form of Serre duality, closely based on the account of the reduced case given by Serre in Algebraic groups and class fields, combined with an invariance result for the topology on the dual of the space of répartitions. Our Abel map, taking Cartier divisors of degree zero to the dual of the space of sections of the Berezinian sheaf, modulo periods, is defined via Penkov's characterization of the Berezinian sheaf as the cohomology of the de Rham complex of the sheaf D of differential operators. We discuss the Jacobi inversion problem for the Abel map and give an example demonstrating that if n is an integer sufficiently large that the generic divisor of degree n is linearly equivalent to an effective divisor, this need not be the case for all divisors of degree n.

Eesti tervishoid on tõesti hea. Aitäh, USA! / Scott Abel

Index Scriptorium Estoniae

Abel, Scott

2010-01-01

Ameeriklane Scott Abel kirjutab, et president Barack Obama tervishoiureform mõjutab arstiabi ka Eestis. Vastukaja artiklile: Turay, Abdul. Kindla individualismi traditsioon // Postimees (2010) 30. märts, lk. 12

Abel y la imposibilidad de resolver la “quíntica” por radicales

Directory of Open Access Journals (Sweden)

José Manuel Sánchez Muñoz

2011-10-01

Full Text Available Este artículo ofrece en su última sección, una traducción comentadade la memoria que Niels Henrik Abel publicó en 1824, para demostrarla imposibilidad de resolver la ecuación de quinto grado mediante radicales (Teorema de Abel-Ruffini. Además se ofrece una visión general de las dificultades que debió sufrir a lo largo de su vida, anhelando siempre un puesto de privilegio entre la comunidad científica de su tiempo, que sistemáticamente le negó el lugar que la historia de la matemática acabó reservándole.

Topology in two dimensions. II - The Abell and ACO cluster catalogues

Science.gov (United States)

Plionis, Manolis; Valdarnini, Riccardo; Coles, Peter

1992-09-01

We apply a method for quantifying the topology of projected galaxy clustering to the Abell and ACO catalogues of rich clusters. We use numerical simulations to quantify the statistical bias involved in using high peaks to define the large-scale structure, and we use the results obtained to correct our observational determinations for this known selection effect and also for possible errors introduced by boundary effects. We find that the Abell cluster sample is consistent with clusters being identified with high peaks of a Gaussian random field, but that the ACO shows a slight meatball shift away from the Gaussian behavior over and above that expected purely from the high-peak selection. The most conservative explanation of this effect is that it is caused by some artefact of the procedure used to select the clusters in the two samples.

2nd Abel Symposium

CERN Document Server

Nunno, Giulia; Lindstrøm, Tom; Øksendal, Bernt; Zhang, Tusheng

2007-01-01

Kiyosi Ito, the founder of stochastic calculus, is one of the few central figures of the twentieth century mathematics who reshaped the mathematical world. Today stochastic calculus is a central research field with applications in several other mathematical disciplines, for example physics, engineering, biology, economics and finance. The Abel Symposium 2005 was organized as a tribute to the work of Kiyosi Ito on the occasion of his 90th birthday. Distinguished researchers from all over the world were invited to present the newest developments within the exciting and fast growing field of stochastic analysis. The present volume combines both papers from the invited speakers and contributions by the presenting lecturers. A special feature is the Memoirs that Kiyoshi Ito wrote for this occasion. These are valuable pages for both young and established researchers in the field.

Interferogram analysis using the Abel inversion technique

International Nuclear Information System (INIS)

Yusof Munajat; Mohamad Kadim Suaidi

2000-01-01

High speed and high resolution optical detection system were used to capture the image of acoustic waves propagation. The freeze image in the form of interferogram was analysed to calculate the transient pressure profile of the acoustic waves. The interferogram analysis was based on the fringe shift and the application of the Abel inversion technique. An easier approach was made by mean of using MathCAD program as a tool in the programming; yet powerful enough to make such calculation, plotting and transfer of file. (Author)

Hadamard Multipliers and Abel Dual of Hardy Spaces

Directory of Open Access Journals (Sweden)

Paweł Mleczko

2016-01-01

Full Text Available The paper is devoted to the study of Hadamard multipliers of functions from the abstract Hardy classes generated by rearrangement invariant spaces. In particular the relation between the existence of such multiplier and the boundedness of the appropriate convolution operator on spaces of measurable functions is presented. As an application, the description of Hadamard multipliers into H∞ is given and the Abel type theorem for mentioned Hardy spaces is proved.

The GenABEL Project for statistical genomics [version 1; referees: 2 approved

Directory of Open Access Journals (Sweden)

Lennart C. Karssen

2016-05-01

Full Text Available Development of free/libre open source software is usually done by a community of people with an interest in the tool. For scientific software, however, this is less often the case. Most scientific software is written by only a few authors, often a student working on a thesis. Once the paper describing the tool has been published, the tool is no longer developed further and is left to its own device. Here we describe the broad, multidisciplinary community we formed around a set of tools for statistical genomics. The GenABEL project for statistical omics actively promotes open interdisciplinary development of statistical methodology and its implementation in efficient and user-friendly software under an open source licence. The software tools developed withing the project collectively make up the GenABEL suite, which currently consists of eleven tools. The open framework of the project actively encourages involvement of the community in all stages, from formulation of methodological ideas to application of software to specific data sets. A web forum is used to channel user questions and discussions, further promoting the use of the GenABEL suite. Developer discussions take place on a dedicated mailing list, and development is further supported by robust development practices including use of public version control, code review and continuous integration. Use of this open science model attracts contributions from users and developers outside the “core team”, facilitating agile statistical omics methodology development and fast dissemination.

On monotonic solutions of an integral equation of Abel type

International Nuclear Information System (INIS)

Darwish, Mohamed Abdalla

2007-08-01

We present an existence theorem of monotonic solutions for a quadratic integral equation of Abel type in C[0, 1]. The famous Chandrasekhar's integral equation is considered as a special case. The concept of measure of noncompactness and a fi xed point theorem due to Darbo are the main tools in carrying out our proof. (author)

Diffuse radio emission in the Coma cluster and Abell 1367: observations at 430 and 1400 MHz

International Nuclear Information System (INIS)

Hanisch, R.J.

1980-01-01

Two rich clusters of galaxies, Abell 1656 (the Coma cluster) and Abell 1367, have been mapped at both 430 and 1400 MHz with the 305-m telescope at Arecibo. The contribution to the observed radio emission due to known discrete sources has been calculated by convolving interferometrically determined source lists with observed Arecibo beam patterns, and maps of the diffuse radio emission alone have been constructed. Both clusters contain regions of diffuse radio emission, although the source in Coma is larger and much more luminous than the source in Abell 1367. The linear extent of the diffuse emission and its dependence on frequency have been used to study particle propagation rates and modes of diffusion in the intracluster medium. The possible correlations between the diffuse radio emission and x-ray emission in these clusters have been investigated, and it has been found that the observed x-ray luminosities can be accounted for if the intracluster gas is heated through Coulomb interactions with the relativistic electrons responsible for the diffuse radio emission

Suzaku observations of the outskirts of the galaxy cluster Abell 3395, including a filament toward Abell 3391

Science.gov (United States)

Sugawara, Yuuki; Takizawa, Motokazu; Itahana, Madoka; Akamatsu, Hiroki; Fujita, Yutaka; Ohashi, Takaya; Ishisaki, Yoshitaka

2017-12-01

The results of Suzaku observations of the outskirts of Abell 3395, including a large-scale structure filament toward Abell 3391, are presented. We measured temperature and abundance distributions from the southern outskirt of A 3395 to the north at the virial radius, where a filament structure has been found in the former X-ray and Sunyaev-Zel'dovich (SZ) effect observations between A 3391 and A 3395. The overall temperature structure is consistent with the universal profile proposed by Okabe, N., et al. 2014, PASJ, 66, 99 for relaxed clusters, except for the filament region. A hint of intracluster medium heating is found between the two clusters, which might be due to their interaction in the early phase of a cluster merger. Although we obtained a relatively low metal abundance of Z=0.169^{+0.164+0.009+0.018}_{-0.150-0.004-0.015} solar, where the first, second, and third errors are statistical, cosmic X-ray background systematic, and non-X-ray background systematic, respectively, at the virial radius in the filament, our results are still consistent with previous results for other clusters (Z ˜ 0.3 solar) within errors. Therefore, our results are also consistent with the early enrichment scenario. We estimated Compton y parameters only from X-ray results in the region between A 3391 and A 3395 assuming a simple geometry. They are smaller than the previous SZ results with the Planck satellite. The difference could be attributed to a more elaborate geometry such as a filament inclined to the line-of-sight direction, or underestimation of the X-ray temperature because of the unresolved multi-temperature structures or undetected hot X-ray emission of the shock-heated gas.

On the interpretation of dark matter self-interactions in Abell 3827

DEFF Research Database (Denmark)

Kahlhoefer, Felix; Schmidt-Hoberg, Kai; Kummer, Janis

2015-01-01

Self-interactions of dark matter (DM) particles can potentially lead to an observable separation between the DM halo and the stars of a galaxy moving through a region of large DM density. Such a separation has recently been observed in a galaxy falling into the core of the galaxy cluster Abell 3827...

Evidence for highly processed material ejected from Abell 30

International Nuclear Information System (INIS)

Hazard, C.; Terlvich, R.; Ferland, G.; Sargent, W.L.W.

1980-01-01

The discovery of compact knots of highly processed material apparently ejected from the central star of the emission nebula Abell 30 is reported here. Spectra obtained from the compact nebulosities surrounding the central star, which indicate a remarkable enhancement of helium relative to hydrogen, are discussed. Preliminary model calculations to investigate the properties of hydrogen deficient nebulae and to study the abundances of some heavy elements have been applied to the results. (UK)

The Noble-Abel Stiffened-Gas equation of state

Science.gov (United States)

Le Métayer, Olivier; Saurel, Richard

2016-04-01

Hyperbolic two-phase flow models have shown excellent ability for the resolution of a wide range of applications ranging from interfacial flows to fluid mixtures with several velocities. These models account for waves propagation (acoustic and convective) and consist in hyperbolic systems of partial differential equations. In this context, each phase is compressible and needs an appropriate convex equation of state (EOS). The EOS must be simple enough for intensive computations as well as boundary conditions treatment. It must also be accurate, this being challenging with respect to simplicity. In the present approach, each fluid is governed by a novel EOS named "Noble Abel stiffened gas," this formulation being a significant improvement of the popular "Stiffened Gas (SG)" EOS. It is a combination of the so-called "Noble-Abel" and "stiffened gas" equations of state that adds repulsive effects to the SG formulation. The determination of the various thermodynamic functions and associated coefficients is the aim of this article. We first use thermodynamic considerations to determine the different state functions such as the specific internal energy, enthalpy, and entropy. Then we propose to determine the associated coefficients for a liquid in the presence of its vapor. The EOS parameters are determined from experimental saturation curves. Some examples of liquid-vapor fluids are examined and associated parameters are computed with the help of the present method. Comparisons between analytical and experimental saturation curves show very good agreement for wide ranges of temperature for both liquid and vapor.

Universal centers in the cubic trigonometric Abel equation

Directory of Open Access Journals (Sweden)

Jaume Giné

2014-02-01

Full Text Available We study the center problem for the trigonometric Abel equation $d \\rho/ d \\theta= a_1 (\\theta \\rho^2 + a_2(\\theta \\rho^3,$ where $a_1(\\theta$ and $a_2(\\theta$ are cubic trigonometric polynomials in $\\theta$. This problem is closely connected with the classical Poincaré center problem for planar polynomial vector fields. A particular class of centers, the so-called universal centers or composition centers, is taken into account. An example of non-universal center and a characterization of all the universal centers for such equation are provided.

ISO far-infrared observations of rich galaxy clusters I. Abell 2670

DEFF Research Database (Denmark)

Hansen, Lene; Jorgensen, H.E.; Nørgaard-Nielsen, Hans Ulrik

1999-01-01

As part of an investigation of far-infrared emission from rich galaxy clusters the central part of Abell 2670 has been mapped with ISO at 60 mu m, 100 mu m, 135 mu m, and 200 mu m using the PHT-C camera. Point sources detected in the field have infrared fluxes comparable to normal spirals...

A ring galaxy at z = 1 lensed by the cluster Abell 370

NARCIS (Netherlands)

Soucail, G.; Kneib, J. P.; Bézecourt, J.; Metcalfe, L.; Altieri, B.; Borgne, J. F. le

1999-01-01

Published in: Astron. Astrophys. 343 (1999) L70 citations recorded in [Science Citation Index] Abstract: We present a study of a very peculiar object found in the field of the cluster-lens Abell 370. This object displays, in HST imaging, a spectacular morphology comparable to nearby ring-galaxies.

Suzaku observations of low surface brightness cluster Abell 1631

Science.gov (United States)

Babazaki, Yasunori; Mitsuishi, Ikuyuki; Ota, Naomi; Sasaki, Shin; Böhringer, Hans; Chon, Gayoung; Pratt, Gabriel W.; Matsumoto, Hironori

2018-06-01

We present analysis results for a nearby galaxy cluster Abell 1631 at z = 0.046 using the X-ray observatory Suzaku. This cluster is categorized as a low X-ray surface brightness cluster. To study the dynamical state of the cluster, we conduct four-pointed Suzaku observations and investigate physical properties of the Mpc-scale hot gas associated with the A 1631 cluster for the first time. Unlike relaxed clusters, the X-ray image shows no strong peak at the center and an irregular morphology. We perform spectral analysis and investigate the radial profiles of the gas temperature, density, and entropy out to approximately 1.5 Mpc in the east, north, west, and south directions by combining with the XMM-Newton data archive. The measured gas density in the central region is relatively low (a few ×10-4 cm-3) at the given temperature (˜2.9 keV) compared with X-ray-selected clusters. The entropy profile and value within the central region (r clusters. These features are also observed in another low surface brightness cluster, Abell 76. The spatial distributions of galaxies and the hot gas appear to be different. The X-ray luminosity is relatively lower than that expected from the velocity dispersion. A post-merger scenario may explain the observed results.

A ring galaxy at z=1 lensed by the cluster Abell 370

NARCIS (Netherlands)

Soucail, G; Kneib, JP; Bezecourt, J; Metcalfe, L; Altieri, B; Le Borgne, JF

We present a study of a very peculiar object found in the field of the cluster-lens Abell 370. This object displays, in HST imaging, a spectacular morphology comparable to nearby ring-galaxies. From spectroscopic observations at the CFHT, we measured a redshift of z = 1.062 based on the

Morphologies and stellar populations of galaxies in the core of Abell 2218

NARCIS (Netherlands)

Sánchez, S. F.; Cardiel, N.; Verheijen, M. A. W.; Pedraz, S.; Covone, G.

2007-01-01

We present a study of the stellar populations and morphologies of galaxies in the core of the galaxy cluster Abell 2218. Integral field spectroscopy (IFS) observations were performed using PMAS in the PPAK mode covering a field of view of similar to 74 x 64 arcsec(2) centred on the core of the

Plasma diagnostics by Abel inversion in hyperbolic geometry

International Nuclear Information System (INIS)

Alhasi, A.S.; Elliott, J.A.

1992-01-01

Plasma confined in the UMIST linear quadrupole adopts a configuration with approximately hyperbolic symmetry. The normal diagnostic is a Langmuir probe, but we have developed an alternative method using optical emission tomography based upon an analytic Abel inversion. Plasma radiance is obtained as a function of a parameter identifying magnetic flux surfaces. The inversion algorithm has been tested using artificial data. Experimentally, the results show that ionizing collisions cause the confined plasma distribution to broaden as the plasma travels through the confining field. This is shown to be a consequence of the approximate incompressibility of the E x B flow. (author)

HI-deficient spiral galaxies in the Coma cluster and Abell 1367

International Nuclear Information System (INIS)

Sullivan, W.T. III; Johnson, P.E.

1978-01-01

A sample of 11 spiral galaxies in each of the clusters Abell 1367 and Coma (Abell 1656) was observed in the 21-cm H I line with the Arecibo 305-m radio telescope. Nine galaxies are detected in Al367 and three in Coma. Comparison of the quantity log M/sub H/L/sub pg/ for each galaxy with the mean value for its Hubble type from the standard samples of nearby spirals compiled by Balkowski and by Roberts indicates that the A1367 and Coma spirals have lower values of log M/sub H/L/sub pg/ than field spirals by a factor of at least 4, with the Coma values probably more extreme. It is argued that little of this effect (perhaps a factor approx. 1.5) can be attributed to the bias toward high luminosities in the sample, and thus that these spirals are deficient in H I by factors of at least 3 to 5 in comparison with the standard samples. For the present limited sample, several mechanisms seem adequate to account qualitatively for stripping of H I from the Coma cluster spirals, but the case of the A1367 spirals is puzzling. 2 figures

Translation and Adaptation of the Auditory Behavior in Everyday Life (ABEL Questionnaire into Persian: A Pilot Study

Directory of Open Access Journals (Sweden)

Mohammad Majid Oryadi-Zanjani

2015-09-01

Full Text Available Background: Auditory rehabilitation is one of the important tasks of speechlanguage pathologists. So, it is necessary to know auditory behaviors in order to make some decisions about the children with hearing loss such as determining the effectiveness of the current rehabilitation programs and/or devices. The Auditory Behavior in Everyday Life (ABEL questionnaire is a valid and reliable assessment tool in English which is developed by Purdy et al. (1995. The aim of this study was to translate and adapt ABEL questionnaire for Persian language. Methods: The ABEL consists of three factors of auditory-oral, auditory awareness, and conversational/social skills. First, the questionnaire was translated and culturally adapted from English to Persian by an independent Iranian translator. The back translated version was compared with the original one in terms of the semantic/idiomatic equivalence. Then the questionnaire was completed two times by 43 mothers of 4-to-6 year old children with hearing loss who were using either hearing aids or cochlear implants. Finally, the results of the test-retest reliability were statistically compared in order to assess internal consistency. The statistical tests which were used include Cronbach’s Alpha, Spearman correlation, and Pearson correlation tests in significance level of 0.05. Results: There was a significant strength correlation among the items of the factor 1 (Alpha=0.94, factor 2 (Alpha=0.86, factor 3 (Alpha=0.82 and three factors (Alpha=0.96. There was a significant strength correlation at the 0.01 level between the scores of each factor in test-retest include auditory-oral (Spearman’s rho=0.94, P<0.001, auditory awareness (Spearman’s rho=0.92, P<0.001, and conversational/social skills (Spearman’s rho=0.82, P<0.001. Conclusion: The Persian version of ABEL questionnaire is a valid and reliable tool for the assessment of auditory performance development in Persianspeaking children wearing hearing aids

The genus curve of the Abell clusters

Science.gov (United States)

Rhoads, James E.; Gott, J. Richard, III; Postman, Marc

1994-01-01

We study the topology of large-scale structure through a genus curve measurement of the recent Abell catalog redshift survey of Postman, Huchra, and Geller (1992). The structure is found to be spongelike near median density and to exhibit isolated superclusters and voids at high and low densities, respectively. The genus curve shows a slight shift toward 'meatball' topology, but remains consistent with the hypothesis of Gaussian random phase initial conditions. The amplitude of the genus curve corresponds to a power-law spectrum with index n = 0.21-0.47+0.43 on scales of 48/h Mpc or to a cold dark matter power spectrum with omega h = 0.36-0.17+0.46.

The genus curve of the Abell clusters

Science.gov (United States)

Rhoads, James E.; Gott, J. Richard, III; Postman, Marc

1994-01-01

We study the topology of large-scale structure through a genus curve measurement of the recent Abell catalog redshift survey of Postman, Huchra, and Geller (1992). The structure is found to be spongelike near median density and to exhibit isolated superclusters and voids at high and low densities, respectively. The genus curve shows a slight shift toward 'meatball' topology, but remains consistent with the hypothesis of Gaussian random phase initial conditions. The amplitude of the genus curve corresponds to a power-law spectrum with index n = 0.21(sub -0.47 sup +0.43) on scales of 48/h Mpc or to a cold dark matter power spectrum with omega h = 0.36(sub -0.17 sup +0.46).

Five-dimensional Monopole Equation with Hedge-Hog Ansatz and Abel's Differential Equation

OpenAIRE

Kihara, Hironobu

2008-01-01

We review the generalized monopole in the five-dimensional Euclidean space. A numerical solution with the Hedge-Hog ansatz is studied. The Bogomol'nyi equation becomes a second order autonomous non-linear differential equation. The equation can be translated into the Abel's differential equation of the second kind and is an algebraic differential equation.

Torsion zero-cycles and the Abel-Jacobi map over the real numbers

NARCIS (Netherlands)

Hamel, J. van

1999-01-01

This is a study of the torsion in the Chow group of zero-cycles on a variety over the real numbers. The first section recalls important results from the literature. The rest of the paper is devoted to the study of the Abel–Jacobi map a: A0XAlbXR restricted to torsion subgroups. Using Roitman’s

The generalized Abel-Plana formula with applications to Bessel functions and casimir effect

International Nuclear Information System (INIS)

Saharian, Aram A.

2007-08-01

One of the most efficient methods for the evaluation of the vacuum expectation values for physical observables in the Casimir effect is based on using the Abel-Plana summation formula. This enables to derive the renormalized quantities in a manifestly cutoff independent way and to present them in the form of strongly convergent integrals. However, applications of the Abel- Plana formula, in its usual form, are restricted by simple geometries when the eigenmodes have a simple dependence on quantum numbers. The author generalized the Abel-Plana formula which essentially enlarges its application range. Based on this generalization, formulae have been obtained for various types of series over the zeros of combinations of Bessel functions and for integrals involving these functions. It has been shown that these results generalize the special cases existing in literature. Further, the derived summation formulae have been used to summarize series arising in the direct mode summation approach to the Casimir effect for spherically and cylindrically symmetric boundaries, for boundaries moving with uniform proper acceleration, and in various braneworld scenarios. This allows to extract from the vacuum expectation values of local physical observables the parts corresponding to the geometry without boundaries and to present the boundary-induced parts in terms of integrals strongly convergent for the points away from the boundaries. As a result, the renormalization procedure for these observables is reduced to the corresponding procedure for bulks without boundaries. The present paper reviews these results. We also aim to collect the results on vacuum expectation values for local physical observables such as the field square and the energy-momentum tensor in manifolds with boundaries for various bulk and boundary geometries. (author)

Letter to the EditorAbel transform inversion of radio occultation measurements made with a receiver inside the Earth’s atmosphere

Directory of Open Access Journals (Sweden)

S. B. Healy

2002-08-01

Full Text Available Radio occultation measurements made with a receiver inside the Earth’s atmosphere can be inverted, assuming local spherical symmetry, with an Abel transform to provide an estimate of the atmospheric refractive index profile. The measurement geometry is closely related to problems encountered when inverting seismic time-travel data and solar occultation measurements, where the Abel solution is well known. The method requires measuring both rays that originate from above and below the local horizon of the receiver. The Abel transform operates on a profile of "partial bending angles" found by subtracting the positive elevation measurement from the negative elevation value with the same impact parameter. In principle, the refractive index profile can be derived from measurements with a single frequency GPS receiver because the ionospheric bending is removed when the partial bending angle is evaluated.Key words. Atmospheric composition and structure (pressure, density and temperature – Radio science (remote sensing

Letter to the EditorAbel transform inversion of radio occultation measurements made with a receiver inside the Earth’s atmosphere

Directory of Open Access Journals (Sweden)

J. Haase

Full Text Available Radio occultation measurements made with a receiver inside the Earth’s atmosphere can be inverted, assuming local spherical symmetry, with an Abel transform to provide an estimate of the atmospheric refractive index profile. The measurement geometry is closely related to problems encountered when inverting seismic time-travel data and solar occultation measurements, where the Abel solution is well known. The method requires measuring both rays that originate from above and below the local horizon of the receiver. The Abel transform operates on a profile of "partial bending angles" found by subtracting the positive elevation measurement from the negative elevation value with the same impact parameter. In principle, the refractive index profile can be derived from measurements with a single frequency GPS receiver because the ionospheric bending is removed when the partial bending angle is evaluated.Key words. Atmospheric composition and structure (pressure, density and temperature – Radio science (remote sensing

CHANDRA OBSERVATION OF ABELL 1142: A COOL-CORE CLUSTER LACKING A CENTRAL BRIGHTEST CLUSTER GALAXY?

Energy Technology Data Exchange (ETDEWEB)

Su, Yuanyuan; Weeren, Reinout van [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Buote, David A. [Department of Physics and Astronomy, University of California, Irvine, 4129 Frederick Reines Hall, Irvine, CA 92697 (United States); Gastaldello, Fabio, E-mail: yuanyuan.su@cfa.harvard.edu [INAF-IASF-Milano, Via E. Bassini 15, I-20133 Milano (Italy)

2016-04-10

Abell 1142 is a low-mass galaxy cluster at low redshift containing two comparable brightest cluster galaxies (BCGs) resembling a scaled-down version of the Coma Cluster. Our Chandra analysis reveals an X-ray emission peak, roughly 100 kpc away from either BCG, which we identify as the cluster center. The emission center manifests itself as a second beta-model surface brightness component distinct from that of the cluster on larger scales. The center is also substantially cooler and more metal-rich than the surrounding intracluster medium (ICM), which makes Abell 1142 appear to be a cool-core cluster. The redshift distribution of its member galaxies indicates that Abell 1142 may contain two subclusters, each of which contain one BCG. The BCGs are merging at a relative velocity of ≈1200 km s{sup −1}. This ongoing merger may have shock-heated the ICM from ≈2 keV to above 3 keV, which would explain the anomalous L{sub X}–T{sub X} scaling relation for this system. This merger may have displaced the metal-enriched “cool core” of either of the subclusters from the BCG. The southern BCG consists of three individual galaxies residing within a radius of 5 kpc in projection. These galaxies should rapidly sink into the subcluster center due to the dynamical friction of a cuspy cold dark matter halo.

Analysis of the optical emission of the young precataclysmic variables HS 1857+5144 and ABELL 65

Science.gov (United States)

Shimansky, V. V.; Pozdnyakova, S. A.; Borisov, N. V.; Bikmaev, I. F.; Vlasyuk, V. V.; Spiridonova, O. I.; Galeev, A. I.; Mel'Nikov, S. S.

2009-10-01

We analyze the physical state and the properties of the close binary systems HS 1857+5144 and Abell 65. We took the spectra of both systems over a wide range of orbital phases with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS) and obtained their multicolor light curves with the RTT150 and Zeiss-1000 telescopes of the SAO RAS. We demonstrate that both Abell 65 and HS 1857+5144 are young precataclysmic variables (PV) with orbital periods of P orb = 1. d 003729 and P orb = 0. d 26633331, respectively. The observed brightness and spectral variations during the orbital period are due to the radiation of the cold component, which absorbs the short-wave radiation of the hot component and reemits it in the visual part of the spectrum. A joint analysis of the brightness and radial velocity curves allowed us to find the possible and optimum sets of their fundamental parameters. We found the luminosity excesses of the secondary components of HS 1857+5144 and Abell 65 with respect to the corresponding Main Sequence stars to be typical for such objects. The excess luminosities of the secondary components of all young PVs are indicative of their faster relaxation rate towards the quiescent state compared to the rates estimated in earlier studies.

Suzaku observations of low surface brightness cluster Abell 1631

Science.gov (United States)

Babazaki, Yasunori; Mitsuishi, Ikuyuki; Ota, Naomi; Sasaki, Shin; Böhringer, Hans; Chon, Gayoung; Pratt, Gabriel W.; Matsumoto, Hironori

2018-04-01

We present analysis results for a nearby galaxy cluster Abell 1631 at z = 0.046 using the X-ray observatory Suzaku. This cluster is categorized as a low X-ray surface brightness cluster. To study the dynamical state of the cluster, we conduct four-pointed Suzaku observations and investigate physical properties of the Mpc-scale hot gas associated with the A 1631 cluster for the first time. Unlike relaxed clusters, the X-ray image shows no strong peak at the center and an irregular morphology. We perform spectral analysis and investigate the radial profiles of the gas temperature, density, and entropy out to approximately 1.5 Mpc in the east, north, west, and south directions by combining with the XMM-Newton data archive. The measured gas density in the central region is relatively low (a few ×10-4 cm-3) at the given temperature (˜2.9 keV) compared with X-ray-selected clusters. The entropy profile and value within the central region (r < 0.1 r200) are found to be flatter and higher (≳400 keV cm2). The observed bolometric luminosity is approximately three times lower than that expected from the luminosity-temperature relation in previous studies of relaxed clusters. These features are also observed in another low surface brightness cluster, Abell 76. The spatial distributions of galaxies and the hot gas appear to be different. The X-ray luminosity is relatively lower than that expected from the velocity dispersion. A post-merger scenario may explain the observed results.

From Messier to Abell: 200 years of science with galaxy clusters

OpenAIRE

Biviano, Andrea

2000-01-01

I review the history of scientific research on galaxy clusters, from 1784, the year of publication of Messier's catalogue, to 1983, the year of George O. Abell's premature death. My review covers four main topics: 1) the distribution of clusters, 2) the cluster components, 3) the cluster structure, 4) the evolution of clusters. I consider both theoretical and observational aspects, but not technical aspects, such as the development of new telescopes and instruments. In total, 529 papers are c...

Dark matter dynamics in Abell 3827: new data consistent with standard cold dark matter

Science.gov (United States)

Massey, Richard; Harvey, David; Liesenborgs, Jori; Richard, Johan; Stach, Stuart; Swinbank, Mark; Taylor, Peter; Williams, Liliya; Clowe, Douglas; Courbin, Frédéric; Edge, Alastair; Israel, Holger; Jauzac, Mathilde; Joseph, Rémy; Jullo, Eric; Kitching, Thomas D.; Leonard, Adrienne; Merten, Julian; Nagai, Daisuke; Nightingale, James; Robertson, Andrew; Romualdez, Luis Javier; Saha, Prasenjit; Smit, Renske; Tam, Sut-Ieng; Tittley, Eric

2018-06-01

We present integral field spectroscopy of galaxy cluster Abell 3827, using Atacama Large Millimetre Array (ALMA) and Very Large Telescope/Multi-Unit Spectroscopic Explorer. It reveals an unusual configuration of strong gravitational lensing in the cluster core, with at least seven lensed images of a single background spiral galaxy. Lens modelling based on Hubble Space Telescope imaging had suggested that the dark matter associated with one of the cluster's central galaxies may be offset. The new spectroscopic data enable better subtraction of foreground light, and better identification of multiple background images. The inferred distribution of dark matter is consistent with being centred on the galaxies, as expected by Λ cold dark matter. Each galaxy's dark matter also appears to be symmetric. Whilst, we do not find an offset between mass and light (suggestive of self-interacting dark matter) as previously reported, the numerical simulations that have been performed to calibrate Abell 3827 indicate that offsets and asymmetry are still worth looking for in collisions with particular geometries. Meanwhile, ALMA proves exceptionally useful for strong lens image identifications.

Oleiferoside W from the roots of Camellia oleifera C. Abel, inducing cell cycle arrest and apoptosis in A549 cells.

Science.gov (United States)

Wu, Jiang-Ping; Kang, Nai-Xin; Zhang, Mi-Ya; Gao, Hong-Wei; Li, Xiao-Ran; Liu, Yan-Li; Xu, Qiong-Ming; Yang, Shi-Lin

2017-07-06

Camellia oleifera C. Abel has been widely cultivated in China, and a group of bioactive constituents such as triterpeniod saponin have been isolated from C. oleifera C. Abel. In the current study, a new triterpeniod saponin was isolated from the EtOH extract of the roots of C. oleifera C. Abel, named as oleiferoside W, and the cytotoxic properties of oleiferoside W were evaluated in non-small cell lung cancer A549 cells. At the same time the inducing apoptosis, the depolarization of mitochondrial membrane potential (Δψ), the up-regulation of related pro-apoptotic proteins, such as cleaved-PARP, cleaved-caspase-3, and the down-regulation of anti-apoptotic marker Bcl-2/Bax were measured on oleiferoside W. Furthermore, the function, inducing the generation of reactive oxygen species (ROS) and apoptosis, of oleiferoside W could be reversed by N-acetylcysteine (NAC). In conclusion, our findings showed that oleiferoside W induced apoptosis involving mitochondrial pathway and increasing intracellular ROS production in the A549 cells, suggesting that oleiferoside W may have the possibility to be a useful anticancer agent for therapy in lung cancer.

Resenha crítica do livro Escuela de la Guitarra: Exposición de la teoría instrumental de Abel Carlevaro

Directory of Open Access Journals (Sweden)

Aluísio Coelho Barros

2014-07-01

Full Text Available Esta resenha pretende apresentar e discutir alguns dos pontos abordados por Abel Carlevaro em seu livro Escuela de la Guitarra: Exposición de la teoría instrumental. O objetivo é de aproximar violonistas estudantes e profissionais à escola técnica de violão criada por Abel Carlevaro, já considerada uma das mais importantes escolas técnicas do século XX. Dentro dos limites de uma resenha, os principais assuntos abordados por Carlevaro são detalhadamente discutidos com uma abordagem crítica.

Flexion in Abell 2744

Science.gov (United States)

Bird, J. P.; Goldberg, D. M.

2018-05-01

We present the first flexion-focused gravitational lensing analysis of the Hubble Frontier Field observations of Abell 2744 (z = 0.308). We apply a modified Analytic Image Model technique to measure source galaxy flexion and shear values at a final number density of 82 arcmin-2. By using flexion data alone, we are able to identify the primary mass structure aligned along the heart of the cluster in addition to two major substructure peaks, including an NE component that corresponds to previous lensing work and a new peak detection offset 1.43 arcmin from the cluster core towards the east. We generate two types of non-parametric reconstructions: flexion aperture mass maps, which identify central core, E, and NE substructure peaks with mass signal-to-noise contours peaking at 3.5σ, 2.7σ, and 2.3σ, respectively; and convergence maps derived directly from the smoothed flexion field. For the primary peak, we find a mass of (1.62 ± 0.12) × 1014 h-1 M⊙ within a 33 arcsec (105 h-1 kpc) aperture, a mass of (2.92 ± 0.26) × 1013 h-1 M⊙ within a 16 arcsec (50 h-1 kpc) aperture for the north-eastern substructure, and (8.81 ± 0.52) × 1013 h-1 M⊙ within a 25 arcsec (80 h-1 kpc) aperture for the novel eastern substructure.

Mýtus židovského konvertity - Šimon Abeles v literatuře 19. a 20. století

Czech Academy of Sciences Publication Activity Database

Soukup, Daniel

2011-01-01

Roč. 3, č. 1 (2011), s. 39-48 ISSN 0231-634X Institutional research plan: CEZ:AV0Z90560517 Keywords : Czech literature * Jews * Abeles, Shimon * Jesuits Subject RIV: AJ - Letters, Mass-media, Audiovision

UV spectroscopy including ISM line absorption: of the exciting star of Abell 35

Science.gov (United States)

Ziegler, M.; Rauch, T.; Werner, K.; Kruk, J. W.

Reliable spectral analysis that is based on high-resolution UV observations requires an adequate, simultaneous modeling of the interstellar line absorption and reddening. In the case of the central star of the planetary nebula Abell 35, BD-22 3467, we demonstrate our current standard spectral-analysis method that is based on the Tübingen NLTE Model-Atmosphere Package (TMAP). We present an on- going spectral analysis of FUSE and HST/STIS observations of BD-22 3467.

MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063 I. Data products and redshift identifications

NARCIS (Netherlands)

Karman, W.; Caputi, K. I.; Grillo, C.; Balestra, I.; Rosati, P.; Vanzella, E.; Coe, D.; Christensen, L.; Koekemoer, A. M.; Kruehler, T.; Lombardi, M.; Mercurio, A.; Nonino, M.; van der Wel, A.

We present the first observations of the Frontier Fields cluster Abell S1063 taken with the newly commissioned Multi Unit Spectroscopic Explorer ( MUSE) integral field spectrograph. Because of the relatively large field of view ( 1 arcmin(2)), MUSE is ideal to simultaneously target multiple galaxies

SHOCKING TAILS IN THE MAJOR MERGER ABELL 2744

Energy Technology Data Exchange (ETDEWEB)

Owers, Matt S.; Couch, Warrick J. [Center for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122 (Australia); Nulsen, Paul E. J.; Randall, Scott W., E-mail: mowers@aao.gov.au [Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-05-01

We identify four rare 'jellyfish' galaxies in Hubble Space Telescope imagery of the major merger cluster Abell 2744. These galaxies harbor trails of star-forming knots and filaments which have formed in situ in gas tails stripped from the parent galaxies, indicating they are in the process of being transformed by the environment. Further evidence for rapid transformation in these galaxies comes from their optical spectra, which reveal starburst, poststarburst, and active galactic nucleus features. Most intriguingly, three of the jellyfish galaxies lie near intracluster medium features associated with a merging 'Bullet-like' subcluster and its shock front detected in Chandra X-ray images. We suggest that the high-pressure merger environment may be responsible for the star formation in the gaseous tails. This provides observational evidence for the rapid transformation of galaxies during the violent core passage phase of a major cluster merger.

Single florescent nanodiamond in a three dimensional ABEL trap

Science.gov (United States)

Kayci, Metin; Radenovic, Aleksandra

2015-01-01

Three dimensional single particle trapping and manipulation is an outstanding challenge in various fields ranging from basic physics to life sciences. By monitoring the response of a trapped particle to a designed environment one can extract its characteristics. In addition, quantum dynamics of a spatially scanned well-known particle can provide environmental information. Precise tracking and positioning of such a particle in aqueous environment is crucial task for achieving nano-scale resolution. Here we experimentally demonstrate three dimensional ABEL trap operating at high frequency by employing a hybrid approach in particle tracking. The particle location in the transverse plane is detected via a scanning laser beam while the axial position is determined by defocused imaging. The scanning of the trapped particle is accomplished through a nano positioning stage integrated to the trap platform. PMID:26559890

On interpolation series related to the Abel-Goncharov problem, with applications to arithmetic-geometric mean relationship and Hellinger integrals

NARCIS (Netherlands)

K.O. Dzhaparidze (Kacha)

1998-01-01

textabstractIn this paper a convergence class is characterized for special series associated with Gelfond's interpolation problem (a generalization of the Abel-Goncharov problem) when the interpolation nodes are equidistantly distributed within the interval $[0,1]$. As a result, an expansion is

Dark matter dynamics in Abell 3827: new data consistent with standard cold dark matter

OpenAIRE

Massey , Richard; Harvey , David; Liesenborgs , Jori; Richard , Johan; Stach , Stuart; Swinbank , Mark; Taylor , Peter; Williams , Liliya; Clowe , Douglas; Courbin , Frédéric; Edge , Alastair; Israel , Holger; Jauzac , Mathilde; Joseph , Remy; Jullo , Eric

2018-01-01

10 pages, 5 figures. Comments welcome; International audience; We present integral field spectroscopy of galaxy cluster Abell 3827, using ALMA and VLT/MUSE. It reveals an unusual configuration of strong gravitational lensing in the cluster core, with at least seven lensed images of a single background spiral galaxy. Lens modelling based on HST imaging had suggested that the dark matter associated with one of the cluster's central galaxies may be offset. The new spectroscopic data enable bette...

XMM-Newton and Chandra Observations of the Remarkable Dynamics of the Intracluster Medium and Radio Sources in the Clusters Abell 2061 and 3667

Science.gov (United States)

Sarazin, C.; Hogge, T.; Chatzikos, M.; Wik, D.; Giacintucci, S.; Clarke, T.; Wong, K.; Gitti, M.; Finoguenov, A.

2014-07-01

XMM-Newton and Chandra observations of remarkable dynamic structures in the X-ray gas and connected radio sources in three clusters are presented. Abell 2061 is a highly irregular, merging cluster in the Corona Borealis supercluster. X-ray observations show that there is a plume of very cool gas (˜1 keV) to the NE of the cluster, and a hot (7.6 keV) shock region just NE of the center. There is a very bright radio relic to the far SW of the cluster, and a central radio halo/relic with an extension to the NE. Comparison to SLAM simulations show that this is an offset merger of a ˜5 × 10^{13} M⊙ subcluster with a ˜2.5 × 10^{14} M⊙ cluster seen after first core passage. The plume is the cool-core gas from the subcluster, which has been ``slingshot'' to the NE of the cluster. The plume gas is now falling back into the cluster center, and shocks when it hits the central gas. The model predicts a strong shock to the SW at the location of the bright radio relic, and another shock at the NE radio extension. Time permitting, the observations of Abell 2626 and Abell 3667 will also be presented.

The galaxy population of Abell 1367: the stellar mass-metallicity relation

Science.gov (United States)

Mouhcine, M.; Kriwattanawong, W.; James, P. A.

2011-04-01

Using wide baseline broad-band photometry, we analyse the stellar population properties of a sample of 72 galaxies, spanning a wide range of stellar masses and morphological types, in the nearby spiral-rich and dynamically young galaxy cluster Abell 1367. The sample galaxies are distributed from the cluster centre out to approximately half the cluster Abell radius. The optical/near-infrared colours are compared with simple stellar population synthesis models from which the luminosity-weighted stellar population ages and metallicities are determined. The locus of the colours of elliptical galaxies traces a sequence of varying metallicity at a narrow range of luminosity-weighted stellar ages. Lenticular galaxies in the red sequence, however, exhibit a substantial spread of luminosity-weighted stellar metallicities and ages. For red-sequence lenticular galaxies and blue cloud galaxies, low-mass galaxies tend to be on average dominated by stellar populations of younger luminosity-weighted ages. Sample galaxies exhibit a strong correlation between integrated stellar mass and luminosity-weighted stellar metallicity. Galaxies with signs of morphological disturbance and ongoing star formation activity, tend to be underabundant with respect to passive galaxies in the red sequence of comparable stellar masses. We argue that this could be due to tidally driven gas flows towards the star-forming regions, carrying less enriched gas and diluting the pre-existing gas to produce younger stellar populations with lower metallicities than would be obtained prior to the interaction. Finally, we find no statistically significant evidence for changes in the luminosity-weighted ages and metallicities for either red-sequence or blue-cloud galaxies, at fixed stellar mass, with location within the cluster. We dedicate this work to the memory of our friend and colleague C. Moss who died suddenly recently.

75 FR 62424 - EDS, an HP Company (Re-Branded as HP-Enterprise Services) Including On-Site Workers From: Abel...

Science.gov (United States)

2010-10-08

...-Branded as HP--Enterprise Services) Including On-Site Workers From: Abel Personnel Inc., Advantage Tech... February 4, 2010, applicable to workers of EDS, an HP Company (Re- branded as HP--Enterprise Services...-branded as HP-- Enterprise Services). These employees provided various activities related to the supply of...

Evolution of the UV upturn in cluster galaxies: Abell 1689

Science.gov (United States)

Ali, S. S.; Bremer, M. N.; Phillipps, S.; De Propris, R.

2018-05-01

We have measured the strength of the UV upturn for red sequence galaxies in the Abell 1689 cluster at z = 0.18, reaching to or below the L* level and therefore probing the general evolution of the upturn phenomenon. We find that the range of UV upturn strengths in the population as a whole has not declined over the past 2.2 Gyrs. This is consistent with a model where hot horizontal branch stars, produced by a Helium-enriched population, provide the required UV flux. Based on local counterparts, this interpretation of the result implies Helium abundances of at least 1.5 times the primordial value for this HB population, along with high formation and assembly redshifts for the galaxies and at least a subset of their stellar populations.

Statistical Analysis for High-Dimensional Data : The Abel Symposium 2014

CERN Document Server

Bühlmann, Peter; Glad, Ingrid; Langaas, Mette; Richardson, Sylvia; Vannucci, Marina

2016-01-01

This book features research contributions from The Abel Symposium on Statistical Analysis for High Dimensional Data, held in Nyvågar, Lofoten, Norway, in May 2014. The focus of the symposium was on statistical and machine learning methodologies specifically developed for inference in “big data” situations, with particular reference to genomic applications. The contributors, who are among the most prominent researchers on the theory of statistics for high dimensional inference, present new theories and methods, as well as challenging applications and computational solutions. Specific themes include, among others, variable selection and screening, penalised regression, sparsity, thresholding, low dimensional structures, computational challenges, non-convex situations, learning graphical models, sparse covariance and precision matrices, semi- and non-parametric formulations, multiple testing, classification, factor models, clustering, and preselection. Highlighting cutting-edge research and casting light on...

Asymptotic behaviour of a special solution of Abel's equation relating to a cusp catastrophe. II. Large values of the parameter t

International Nuclear Information System (INIS)

Il'in, Arlen M; Suleimanov, Bulat I

2007-01-01

An asymptotic formula as t→∞ for the solution of the ordinary differential Abel's equation of the first kind u' x +u 3 -tu-x=0, which is uniform in the x-variable, is constructed and substantiated. Bibliography: 13 titles.

CARACTERIZACIÓN DEL NEONATO ASISTIDO CON VENTILACIÓN MECÁNICA. HOSPITAL “ABEL SANTAMARÍA” AGOSTO 2009 – MARZO 2013

Directory of Open Access Journals (Sweden)

Adrián Naranjo

2014-03-01

Full Text Available Objetive: to characterize the mechanical ventilation on neonates of "Abel Santamaria" Hospital, in Pinar del Rio, Cuba Material and Methods: An observational, cross-sectional, descriptive study, conducted between August 2009 and March 2013. A total of 164 mechanically ventilated infants were studied in the Neonatal Intensive Care Unit of the Hospital Abel Santamaria. We analyzed: gestational age, birth weight, medical history of the mother, causes of ventilation and complications of ventilation Results: 62% were male, gestational age was predominanlly more than 32 weeks, 37% of infants had less than 2500 g. Pregnancy induced hypertension was present as maternal history in 17% of ventilated infants, the most common cause for ventilation was acute respiratory distress syndorme (ARDS, digestive dysfunction occurred in 14% as a complication, pulmonary hemorrhage was the leading cause of death conclusions: The lower the duration of mechanical ventilation, the longer survival. Pulmonary haemorrhage was the leading cause of death.

A comparison of void distributions in Abell cluster catalogue with numerical simulations

International Nuclear Information System (INIS)

Jing Yipeng.

1989-08-01

We measured the void probability functions (VPF) for two virtually redshift complete samples of Abell clusters, and used them to test four current theoretical models. The VPF of R ≥ 1 clusters is lower than that of the explosion model by about one order. The open CDM model (Ω = 0.2) is excluded at ≥ 3 σ also due to oversuperclustering. The VPF of the flat neutrinos dominated universe is consistent with the observations, and the flat CDM model could be marginally accepted at 2 σ in matching the observational VPF. However, all four models are unsuccessful if we combine the two-point correlation function and VPF. (author). 15 refs, 3 figs

Vitamins and Violence: Can Micronutrients Make Students Behave, Schools Safer and Test Scores Better? The Abell Report. Volume 23, No.6

Science.gov (United States)

Rodgers, Joann Ellison

2010-01-01

The notion that vitamins, minerals, and other "supplemental" nutrients profoundly change behavior, mood, and intellect has origins as old as recorded history. Research has indeed suggested connections between nutrient deficiencies and behavior problems, but correlations are not the same as causality. This "Abell Report" is an…

The merging cluster Abell 1758: an optical and dynamical view

Science.gov (United States)

Monteiro-Oliveira, Rogerio; Serra Cypriano, Eduardo; Machado, Rubens; Lima Neto, Gastao B.

2015-08-01

The galaxy cluster Abell 1758-North (z=0.28) is a binary system composed by the sub-structures NW and NE. This is supposed to be a post-merging cluster due to observed detachment between the NE BCG and the respective X-ray emitting hot gas clump in a scenario very close to the famous Bullet Cluster. On the other hand, the projected position of the NW BCG coincides with the local hot gas peak. This system was been targeted previously by several studies, using multiple wavelengths and techniques, but there is still no clear picture of the scenario that could have caused this unusual configuration. To help solving this complex puzzle we added some pieces: firstly, we have used deep B, RC and z' Subaru images to perform both weak lensing shear and magnification analysis of A1758 (including here the South component that is not in interaction with A1758-North) modeling each sub-clump as an NFW profile in order to constrain masses and its center positions through MCMC methods; the second piece is the dynamical analysis using radial velocities available in the literature (143) plus new Gemini-GMOS/N measurements (68 new redshifts).From weak lensing we found that independent shear and magnification mass determinations are in excellent agreement between them and combining both we could reduce mass error bar by ~30% compared to shear alone. By combining this two weak-lensing probes we found that the position of both Northern BCGs are consistent with the masses centers within 2σ and and the NE hot gas peak to be offseted of the respective mass peak (M200=5.5 X 1014 M⊙) with very high significance. The most massive structure is NW (M200=7.95 X 1014 M⊙ ) where we observed no detachment between gas, DM and BCG.We have calculated a low line-of-sight velocity difference (plane of collision and the sky (<40 degrees). Dynamic modeling shows that the point of maximum approximation taken place 0.55 Gyr ago, pointing Abell 1758-North as a young merger cluster.

Galaxy evolution in the cluster Abell 85: new insights from the dwarf population

Science.gov (United States)

Habas, Rebecca; Fadda, Dario; Marleau, Francine R.; Biviano, Andrea; Durret, Florence

2018-04-01

We present the first results of a new spectroscopic survey of the cluster Abell 85 targeting 1466 candidate cluster members within the central ˜1 deg2 of the cluster and having magnitudes mr behaviour based on their mass. At the low-mass end, the galaxies have had their star formation recently quenched, while more massive galaxies show no significant change. The time-scales probed here favour fast quenching mechanisms, such as ram-pressure stripping. Galaxies within the green valley, defined similarly, do not show evidence of quenching. Instead, the low-mass galaxies maintain their levels of star-forming activity, while the more massive galaxies have experienced a recent burst.

On the number of polynomial solutions of Bernoulli and Abel polynomial differential equations

Science.gov (United States)

Cima, A.; Gasull, A.; Mañosas, F.

2017-12-01

In this paper we determine the maximum number of polynomial solutions of Bernoulli differential equations and of some integrable polynomial Abel differential equations. As far as we know, the tools used to prove our results have not been utilized before for studying this type of questions. We show that the addressed problems can be reduced to know the number of polynomial solutions of a related polynomial equation of arbitrary degree. Then we approach to these equations either applying several tools developed to study extended Fermat problems for polynomial equations, or reducing the question to the computation of the genus of some associated planar algebraic curves.

Abel transforms with low regularity with applications to x-ray tomography on spherically symmetric manifolds

Science.gov (United States)

de Hoop, Maarten V.; Ilmavirta, Joonas

2017-12-01

We study ray transforms on spherically symmetric manifolds with a piecewise C1, 1 metric. Assuming the Herglotz condition, the x-ray transform is injective on the space of L 2 functions on such manifolds. We also prove injectivity results for broken ray transforms (with and without periodicity) on such manifolds with a C1, 1 metric. To make these problems tractable in low regularity, we introduce and study a class of generalized Abel transforms and study their properties. This low regularity setting is relevant for geophysical applications.

The near-infrared Tully-Fisher relation - A preliminary study of the Coma and Abell 400 clusters

Science.gov (United States)

Guhathakurta, Puragra; Bernstein, Gary; Raychaudhury, Somak; Haynes, Martha; Giovanelli, Riccardo; Herter, Terry; Vogt, Nicole

1993-01-01

We have started a large project to study the NIR Tully-Fisher (TF) relation using H- and I-band surface photometry of spiral galaxies. A preliminary study of 20 spirals in the Coma and Abell 400 clusters is presented. The NIR images have been used to derive accurate inclinations and total magnitudes, and rotational linewidths are measured from high-quality 21-cm Arecibo data. The scatter in the Coma TF plot is found to be 0.19 mag in the H band and 0.20 mag in the I band for a set of 13 galaxies, if we assume that they are all at the same distance. The deviation of the Coma galaxies from the best-fit Tully-Fisher relation is correlated with their redshift, indicating that some of the galaxies are not bound to the cluster. Indeed, if we treat all the galaxies in the Coma sample as undergoing free Hubble expansion, the TF scatter drops to 0.12 and 0.13 mag for the H- and I-band datasets, respectively. The Abell 400 sample is best fit by a common distance model, yielding a scatter of 0.12 mag for seven galaxies in H using a fixed TF slope. We are in the process of studying cluster and field spirals out to about 10,000 km/s in order to calibrate the NIR TF relation and will apply it to more nearby galaxies to measure the peculiar velocity field in the local universe.

MUSE integral-field spectroscopy towards the Frontier Fields Cluster Abell S1063

DEFF Research Database (Denmark)

Karman, W.; Caputi, K. I.; Grillo, C.

2015-01-01

We present the first observations of the Frontier Fields Cluster Abell S1063 taken with the newly commissioned Multi Unit Spectroscopic Explorer (MUSE) integral field spectrograph. Because of the relatively large field of view (1 arcmin^2), MUSE is ideal to simultaneously target multiple galaxies...... the cluster, we find 17 galaxies at higher redshift, including three previously unknown Lyman-alpha emitters at z>3, and five multiply-lensed galaxies. We report the detection of a new z=4.113 multiply lensed galaxy, with images that are consistent with lensing model predictions derived for the Frontier...... of scientific topics that can be addressed with a single MUSE pointing. We conclude that MUSE is a very efficient instrument to observe galaxy clusters, enabling their mass modelling, and to perform a blind search for high-redshift galaxies....

Inhibition of α-glucosidase by polysaccharides from the fruit hull of Camellia oleifera Abel.

Science.gov (United States)

Zhang, Sheng; Li, Xiang-Zhou

2015-01-22

We isolated and purified polysaccharides from the Camellia oleifera Abel. fruit hull and studied its hypoglycemic potential. Our results revealed six polysaccharides (CFPA-1-5 & CFPB) from the aqueous extract from the defatted C. oleifera fruit hull. Purified polysaccharides (purity >90%) were investigated for the inhibition of α-glucosidase activity in vitro. Two polysaccharides, CFPB and CFPA-3 were present in high concentration in the fruit hull and showed a dose-dependent inhibition of α-glucosidase activity, with IC50 concentrations of 11.80 and 10.95 μg/mL, respectively. This result suggests that polysaccharides (CFP) extracted from the fruit hull of C. oleifera may have potential as functional foods with featuring a hypoglycemic effect. Copyright © 2014 Elsevier Ltd. All rights reserved.

The double galaxy cluster Abell 2465 - I. Basic properties: optical imaging and spectroscopy

Science.gov (United States)

Wegner, Gary A.

2011-05-01

Optical imaging and spectroscopic observations of the z= 0.245 double galaxy cluster Abell 2465 are described. This object appears to be undergoing a major merger. It is a double X-ray source and is detected in the radio at 1.4 GHz. The purpose of this paper is to investigate signatures of the interaction of the two components. Redshifts were measured to determine velocity dispersions and virial radii of each component. The technique of fuzzy clustering was used to assign membership weights to the galaxies in each clump. Using redshifts of 93 cluster members within 1.4 Mpc of the subcluster centres, the virial masses of the north-east (NE) and south-west (SW) components are Mv= 4.1 ± 0.8 × 1014 and 3.8 ± 0.8 × 1014 M⊙, respectively. These agree within the errors with masses from X-ray scaling relations. The projected velocity difference between the two subclusters is 205 ± 149 km s-1. The anisotropy parameter, β, is found to be low for both components. Spectra of 37 per cent of the spectroscopically observed galaxies show emission lines and are predominantly star forming in the diagnostic diagram. No strong active galactic nucleus sources were found. The emission-line galaxies tend to lie between the two cluster centres with more near the SW clump. The luminosity functions of the two subclusters differ. The NE component is similar to many rich clusters, while the SW component has more faint galaxies. The NE clump’s light profile follows a single Navarro-Frenk-White profile with c= 10 while the SW is better fitted with an extended outer region and a compact inner core, consistent with available X-ray data indicating that the SW clump has a cooling core. The observed differences and properties of the two components of Abell 2465 are interpreted to have been caused by a collision 2-4 Gyr ago, after which they have moved apart and are now near their apocentres, although the start of a merger remains a possibility. The number of emission-line galaxies gives

Radio emission of Abell galaxy clusters with red shifts from 0.02 to 0.075 at 102.5 MHz. Observations of clusters southward from the galactic plane

International Nuclear Information System (INIS)

Gubanov, A.G.

1983-01-01

The sample of 121 Abell clusters of galaxies with measured red shifts from 0.02 to 0.075, delta= 10 deg - +80 deg and within the completeness galactic-latitude region is presented. The completeness. with respect to the Abell's catalog is 80%. The completeness of the sample in function of distance (the completeness function) was constructed and the mean cluster density of 1.5x10 -6 Mpc -3 was derived. Observations at 102.5 MHz of 39 clusters southward from the galactic plane were carried out with BSA radio telescope. Flux density measurements for radio sources in the directions of the clusters have been made, integrated fluxes of clusters and luminosity estimations for their radio halos are presented. Radio emission of 11 clusters was detected , and for two of these and for other clust rs radio sources detected in the directions to the outskirts of clusters. Radio halos having the luminosity comparable to that of the A1656 (Coma) cluster are not typical for clusters

X-ray constraints on the shape of the dark matter in five Abell clusters

Science.gov (United States)

Buote, David A.; Canizares, Claude R.

1992-01-01

X-ray observations obtained with the Einstein Observatory are used to constrain the shape of the dark matter in the inner regions of Abell clusters A401, A426, A1656, A2029, and A2199, each of which exhibits highly flattened optical isopleths. The dark matter is modeled as an ellipsoid with a mass density of about r exp -2. The possible shapes of the dark matter is constrained by comparing these model isophotes to the image isophotes. The X-ray isophotes, and therefore the gravitational potentials, have ellipticities of about 0.1-0.2. The dark matter within the central 1 Mpc is found to be substantially rounder for all the clusters. It is concluded that the shape of the galaxy distributions in these clusters traces neither the gravitational potential nor the gravitating matter.

Dynamical history of a binary cluster: Abell 3653

Science.gov (United States)

Caglar, Turgay; Hudaverdi, Murat

2017-12-01

We study the dynamical structure of a bimodal galaxy cluster Abell 3653 at z = 0.1089 using optical and X-ray data. Observations include archival data from the Anglo-Australian Telescope, X-ray observatories XMM-Newton and Chandra. We draw a global picture for A3653 using galaxy density, X-ray luminosity and temperature maps. The galaxy distribution has a regular morphological shape at the 3 Mpc size. The galaxy density map shows an elongation in the east-west direction, which perfectly aligns with the extended diffuse X-ray emission. We detect two dominant groups around the two brightest cluster galaxies (BCGs). BCG1 (z = 0.1099) can be associated with the main cluster A3653E, and a foreground subcluster A3653W is concentrated at BCG2 (z = 0.1075). Both X-ray peaks are dislocated from the BCGs by ∼35 kpc, which suggest an ongoing merger process. We measure the subcluster gas temperatures of 4.67 and 3.66 keV, respectively. Two-body dynamical analysis shows that A3653E and A3653W are very likely gravitationally bound (93.5 per cent probability). The highly favoured scenario suggests that the two subclusters have a mass ratio of 1.4 and are colliding close to the plane of sky (α = 17.61°) at 2400 km s-1, and will undergo core passage in 380 Myr. The temperature map also significantly shows a shock-heated gas (6.16 keV) between the subclusters, which confirms the supersonic infalling scenario.

On the Merging Cluster Abell 578 and Its Central Radio Galaxy 4C+67.13

Science.gov (United States)

Hagino, K.; Stawarz, Ł.; Siemiginowska, A.; Cheung, C. C.; Kozieł-Wierzbowska, D.; Szostek, A.; Madejski, G.; Harris, D. E.; Simionescu, A.; Takahashi, T.

2015-06-01

Here we analyze radio, optical, and X-ray data for the peculiar cluster Abell 578. This cluster is not fully relaxed and consists of two merging sub-systems. The brightest cluster galaxy (BCG), CGPG 0719.8+6704, is a pair of interacting ellipticals with projected separation ˜10 kpc, the brighter of which hosts the radio source 4C+67.13. The Fanaroff-Riley type-II radio morphology of 4C+67.13 is unusual for central radio galaxies in local Abell clusters. Our new optical spectroscopy revealed that both nuclei of the CGPG 0719.8+6704 pair are active, albeit at low accretion rates corresponding to the Eddington ratio ˜ {{10}-4} (for the estimated black hole masses of ˜ 3× {{10}8} {{M}⊙ } and ˜ {{10}9} {{M}⊙ }). The gathered X-ray (Chandra) data allowed us to confirm and to quantify robustly the previously noted elongation of the gaseous atmosphere in the dominant sub-cluster, as well as a large spatial offset (˜60 kpc projected) between the position of the BCG and the cluster center inferred from the modeling of the X-ray surface brightness distribution. Detailed analysis of the brightness profiles and temperature revealed also that the cluster gas in the vicinity of 4C+67.13 is compressed (by a factor of about ˜1.4) and heated (from ≃ 2.0 keV up to 2.7 keV), consistent with the presence of a weak shock (Mach number ˜1.3) driven by the expanding jet cocoon. This would then require the jet kinetic power of the order of ˜ {{10}45} erg s-1, implying either a very high efficiency of the jet production for the current accretion rate, or a highly modulated jet/accretion activity in the system. Based on service observations made with the WHT operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias.

AM I MY BROTHER’S KEEPER? Émile Zola’s Thérèse Raquin as a retelling of Cain and Abel

Directory of Open Access Journals (Sweden)

William Bradley Holley

2017-12-01

Full Text Available Émile Zola’s Thérèse Raquin exemplifies what the author would develop as his naturalist philosophy. This philosophy, based upon what the Zola considered to be a scientific and empirical process to understand the human condition, appears at a time in France where many different philosophical thoughts converge. This paper looks at how Zola’s declared scientific study of the “human-beast” is in fact a retelling of the Biblical tale of Cain and Abel, perhaps spurred by the confusion of the competing philosophies.Thérèse Raquin d'Émile Zola illustre ce que l'auteur développera comme sa philosophie naturaliste. Cette philosophie, basée sur ce que Zola considérait comme un processus scientifique et empirique pour comprendre la condition humaine, apparaît à un moment en France où convergent de nombreuses pensées philosophiques différentes. Cet article examine comment l'étude scientifique sur la « bête humaine » (déclarée ainsi par Zola est en fait une réécriture du récit biblique de Caïn et Abel, peut-être stimulée par la confusion des philosophies concurrentes.

Measurement of lower-hybrid-driven current profile by Abel inversion of electron-cyclotron wave transmission spectra

International Nuclear Information System (INIS)

Fidone, I.; Giruzzi, G.; Caron, X.; Meyer, R.L.

1991-01-01

A method for measuring the radial profile of the lower-hybrid-driven current in a low-density tokamak plasma using electron-cyclotron wave attenuation is discussed. This diagnostic scheme is reminiscent of the transmission interferometry approach, commonly used in tokamaks to measure the plasma density, but now the wave amplitude instead of the phase is measured. Wave attenuation of the ordinary mode at ω p much-lt ω c along vertical chords is measured; at these frequencies, the waves are absorbed by the superthermal tail sustained by lower-hybrid waves and the local wave absorption coefficient is proportional to the noninductive current density. The radial profile of this current is obtained from Abel inversion. An application to the Tore Supra tokamak is presented

The complete larval development of Eurypanopeus canalensis Abele and Kim, 1989 (Crustacea: Brachyura: Panopeidae described from laboratory reared material

Directory of Open Access Journals (Sweden)

Marcelo U. García-Guerrero

2005-09-01

Full Text Available The estuarine panopeid crab Eurypanopeus canalensis Abele and Kim, 1989, is an eastern tropical Pacific species with a known distribution from the southeastern Gulf of California, Mexico, to Panama. Its complete larval development is fully described and illustrated from laboratory-reared material. The four zoeal stages and the megalopa are compared with two congeneric species from the West Atlantic, E. abbreviatus (Stimpson, 1860 and E. depressus (Smith, 1869. The main differences between larvae of E. canalensis and those of these two species include telson setation and the presence/absence of a stout hook-like spine in the megalopae cheliped ischium.

BRIGHT STRONGLY LENSED GALAXIES AT REDSHIFT z ∼ 6-7 BEHIND THE CLUSTERS ABELL 1703 AND CL0024+16

International Nuclear Information System (INIS)

Zheng, W.; Bradley, L. D.; Ford, H. C.; Shu, X.W.; Bouwens, R. J.; Illingworth, G. D.; BenItez, N.; Broadhurst, T.; Zitrin, A.; Frye, B.; Infante, L.; Jee, M. J.; Motta, V.

2009-01-01

We report on the discovery of three bright, strongly lensed objects behind Abell 1703 and CL0024+16 from a dropout search over 25 arcmin 2 of deep NICMOS data, with deep ACS optical coverage. They are undetected in the deep ACS images below 8500 A and have clear detections in the J and H bands. Fits to the ACS, NICMOS, and IRAC data yield robust photometric redshifts in the range z ∼ 6-7 and largely rule out the possibility that they are low-redshift interlopers. All three objects are extended, and resolved into a pair of bright knots. The bright i-band dropout in Abell 1703 has an H-band AB magnitude of 23.9, which makes it one of the brightest known galaxy candidates at z > 5.5. Our model fits suggest a young, massive galaxy only ∼60 million years old with a mass of ∼10 10 M sun . The dropout galaxy candidates behind CL0024+16 are separated by 2.''5 (∼2 kpc in the source plane), and have H-band AB magnitudes of 25.0 and 25.6. Lensing models of CL0024+16 suggest that the objects have comparable intrinsic magnitudes of AB ∼27.3, approximately one magnitude fainter than L* at z ∼ 6.5. Their similar redshifts, spectral energy distribution, and luminosities, coupled with their very close proximity on the sky, suggest that they are spatially associated, and plausibly are physically bound. Combining this sample with two previously reported, similarly magnified galaxy candidates at z ∼ 6-8, we find that complex systems with dual nuclei may be a common feature of high-redshift galaxies.

Diffuse X-ray emission from Abell clusters 401 and 399 - A gravitationally bound system

Science.gov (United States)

Ulmer, M. P.; Kinzer, R.; Cruddace, R. G.; Wood, K.; Evans, W.; Byram, E. T.; Chubb, T. A.; Friedman, H.

1979-01-01

The X-ray emission from the Abell 401-399 region has been studied using data obtained by the A-1 proportional counter aboard HEAO 1 in two different ways. The first involved routine scanning of the region during the all-sky survey, and the second was an observation in which the instrument was pointed at A401 during a lunar occultation. The emission is shown to be unusually extended and to be centered on a point lying between A401 and A399. The best fit of a uniform disk model to the data yielded a radius of 25.5 + or -4.4 arcmin for the lunar occultation and 42 + or - 17 arcmin for the scans. A possible explanation of the results is that A401 and A399 are both diffuse cluster X-ray sources. Alternatively, the emission may come from a large gas cloud of at least 10 to the 15th solar masses enveloping both clusters.

STRONG GRAVITATIONAL LENSING BY THE SUPER-MASSIVE cD GALAXY IN ABELL 3827

International Nuclear Information System (INIS)

Carrasco, E. R.; Gomez, P. L.; Lee, H.; Diaz, R.; Bergmann, M.; Turner, J. E. H.; Miller, B. W.; West, M. J.; Verdugo, T.

2010-01-01

We have discovered strong gravitational lensing features in the core of the nearby cluster Abell 3827 by analyzing Gemini South GMOS images. The most prominent strong lensing feature is a highly magnified, ring-shaped configuration of four images around the central cD galaxy. GMOS spectroscopic analysis puts this source at z ∼ 0.2. Located ∼20'' away from the central galaxy is a secondary tangential arc feature which has been identified as a background galaxy with z ∼ 0.4. We have modeled the gravitational potential of the cluster core, taking into account the mass from the cluster, the brightest cluster galaxy (BCG), and other galaxies. We derive a total mass of (2.7 ± 0.4) x 10 13 M sun within 37 h -1 kpc. This mass is an order of magnitude larger than that derived from X-ray observations. The total mass derived from lensing data suggests that the BCG in this cluster is perhaps the most massive galaxy in the nearby universe.

Discovery of Ram-pressure Stripped Gas around an Elliptical Galaxy in Abell 2670

International Nuclear Information System (INIS)

Sheen, Yun-Kyeong; Kim, Minjin; Smith, Rory; Yi, Sukyoung K.; Jaffé, Yara; Duc, Pierre-Alain; Nantais, Julie; Candlish, Graeme; Demarco, Ricardo; Treister, Ezequiel

2017-01-01

Studies of cluster galaxies are increasingly finding galaxies with spectacular one-sided tails of gas and young stars, suggestive of intense ram-pressure stripping. These so-called “jellyfish” galaxies typically have late-type morphology. In this paper, we present Multi Unit Spectroscopic Explorer (MUSE) observations of an elliptical galaxy in Abell 2670 with long tails of material visible in the optical spectra, as well as blobs with tadpole-like morphology. The spectra in the central part of the galaxy reveal a stellar component as well as ionized gas. The stellar component does not have significant rotation, while the ionized gas defines a clear star-forming gas disk. We argue, based on deep optical images of the galaxy, that the gas was most likely acquired during a past wet merger. It is possible that the star-forming blobs are also remnants of the merger. In addition, the direction and kinematics of the one-sided ionized tails, combined with the tadpole morphology of the star-forming blobs, strongly suggests that the system is undergoing ram pressure from the intracluster medium. In summary, this paper presents the discovery of a post-merger elliptical galaxy undergoing ram-pressure stripping.

Discovery of Ram-pressure Stripped Gas around an Elliptical Galaxy in Abell 2670

Energy Technology Data Exchange (ETDEWEB)

Sheen, Yun-Kyeong; Kim, Minjin [Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon, 34055 (Korea, Republic of); Smith, Rory; Yi, Sukyoung K. [Department of Astronomy, Yonsei University, 50 Yonsei-ro, Seodaemun-gu, Seoul, 03722 (Korea, Republic of); Jaffé, Yara [European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago de Chile (Chile); Duc, Pierre-Alain [Laboratoire AIM Paris-Saclay, CEA/Irfu/SAp CNRS Universite Paris Diderot, F-91191 Gif-sur-Yvette Cedex (France); Nantais, Julie [Departamento de Ciencias Físicas, Universidad Andres Bello, Fernandez Concha 700, 7591538 Las Condes, Santiago (Chile); Candlish, Graeme [Instituto de Física y Astronomía, Universidad de Valparaíso, Gran Bretaña 1111, Valparaíso (Chile); Demarco, Ricardo [Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción (Chile); Treister, Ezequiel, E-mail: yksheen@kasi.re.kr [Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago (Chile)

2017-05-01

Studies of cluster galaxies are increasingly finding galaxies with spectacular one-sided tails of gas and young stars, suggestive of intense ram-pressure stripping. These so-called “jellyfish” galaxies typically have late-type morphology. In this paper, we present Multi Unit Spectroscopic Explorer (MUSE) observations of an elliptical galaxy in Abell 2670 with long tails of material visible in the optical spectra, as well as blobs with tadpole-like morphology. The spectra in the central part of the galaxy reveal a stellar component as well as ionized gas. The stellar component does not have significant rotation, while the ionized gas defines a clear star-forming gas disk. We argue, based on deep optical images of the galaxy, that the gas was most likely acquired during a past wet merger. It is possible that the star-forming blobs are also remnants of the merger. In addition, the direction and kinematics of the one-sided ionized tails, combined with the tadpole morphology of the star-forming blobs, strongly suggests that the system is undergoing ram pressure from the intracluster medium. In summary, this paper presents the discovery of a post-merger elliptical galaxy undergoing ram-pressure stripping.

Reseña de libro Contabilidad gerencial y presupuestaria aplicada a las ciencias económicas, administrativas y contables, de Abel Cano Morales

OpenAIRE

Macías Cardona, Hugo

2013-01-01

En el mes de febrero de 2013, Ediciones de la U publicó el libro Contabilidad gerencial y presupuestaria, escrito por el profesor Abel Cano Morales, de la Universidad de Medellín. El libro es novedoso desde su título, ya que hace referencia a la contabilidad gerencial y no a la contabilidad de gestión, administrativa o de costos, como lo hacen varios libros de texto que circulan de tiempo atrás en Colombia. El cambio en la denominación es intencional y tiene un sentido profundo que se present...

Spatially-resolved velocities of thermally-produced spray droplets using a velocity-divided Abel inversion of photographed streaks

Science.gov (United States)

Kawaguchi, Y.; Kobayashi, N.; Yamagata, Y.; Miyazaki, F.; Yamasaki, M.; Muraoka, K.

2017-10-01

Droplet velocities of thermal spray are known to have profound effects on important coating qualities, such as adhesive strength, porosity, and hardness, for various applications. For obtaining the droplet velocities, therefore, the TOF (time-of-flight) technique has been widely used, which relies on observations of emitted radiation from the droplets, where all droplets along the line-of-sight contribute to signals. Because droplets at and near the flow axis mostly contribute coating layers, it has been hoped to get spatially resolved velocities. For this purpose, a velocity-divided Abel inversion was devised from CMOS photographic data. From this result, it has turned out that the central velocity is about 25% higher than that obtained from the TOF technique for the case studied (at the position 150 mm downstream of the plasma spray gun, where substrates for spray coatings are usually placed). Further implications of the obtained results are discussed.

ERKÜ valimiste tulemused

Index Scriptorium Estoniae

2006-01-01

8. aprilli koosolekul kinnitas valimiste peakomitee XIX Esinduskogu liikmed: Mati Kõiva, Ylo Anson, Juhan Simonson, Airi Vaga, Gilda M. Karu, Taavo Virkhaus, Marju Rink-Abel, Markus Vaga, Eric Suuberg, Endel Reinpõld, Jaak Juhansoo, Ülle Ederma, Lya Karm, Heino Jõgis, Kersti Linask, Jaak Rakfeldt, Erik Puskar, Jüri Linask, Viiu Vanderer, Andres Kurrik, Mati Valdek Laan, Ilmar Vanderer, Henno Uus, Jüri Tults, Urmas Wompa, Astrid Jaanson, Jüri Virkus, Lilian G. G. Bein, Tiina Harris, Tõnu Vanderer

19 August 2013 - German Member of the Parliament of North Rhine-Westphalia M.-S. Abel MdL visiting the ATLAS experimental area with Senior physicist C. Rembser and German members of the collaboration B. Heinemann with G. Gaycken and D. Hirschbuehl.

CERN Multimedia

Anna Pantelia

2013-01-01

19 August 2013 - German Member of the Parliament of North Rhine-Westphalia M.-S. Abel MdL visiting the ATLAS experimental area with Senior physicist C. Rembser and German members of the collaboration B. Heinemann with G. Gaycken and D. Hirschbuehl.

Bright Strongly Lensed Galaxies at Redshift z ~ 6-7 behind the Clusters Abell 1703 and CL0024+16

Science.gov (United States)

Zheng, W.; Bradley, L. D.; Bouwens, R. J.; Ford, H. C.; Illingworth, G. D.; Benítez, N.; Broadhurst, T.; Frye, B.; Infante, L.; Jee, M. J.; Motta, V.; Shu, X. W.; Zitrin, A.

2009-06-01

We report on the discovery of three bright, strongly lensed objects behind Abell 1703 and CL0024+16 from a dropout search over 25 arcmin2 of deep NICMOS data, with deep ACS optical coverage. They are undetected in the deep ACS images below 8500 Å and have clear detections in the J and H bands. Fits to the ACS, NICMOS, and IRAC data yield robust photometric redshifts in the range z ~ 6-7 and largely rule out the possibility that they are low-redshift interlopers. All three objects are extended, and resolved into a pair of bright knots. The bright i-band dropout in Abell 1703 has an H-band AB magnitude of 23.9, which makes it one of the brightest known galaxy candidates at z > 5.5. Our model fits suggest a young, massive galaxy only ~60 million years old with a mass of ~1010 M sun. The dropout galaxy candidates behind CL0024+16 are separated by 2farcs5 (~2 kpc in the source plane), and have H-band AB magnitudes of 25.0 and 25.6. Lensing models of CL0024+16 suggest that the objects have comparable intrinsic magnitudes of AB ~27.3, approximately one magnitude fainter than L* at z ~ 6.5. Their similar redshifts, spectral energy distribution, and luminosities, coupled with their very close proximity on the sky, suggest that they are spatially associated, and plausibly are physically bound. Combining this sample with two previously reported, similarly magnified galaxy candidates at z ~ 6-8, we find that complex systems with dual nuclei may be a common feature of high-redshift galaxies. Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities of Research in Astronomy, Inc., under NASA contract NAS5-26555, and at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Particle

DISCOVERY OF ULTRA-STEEP SPECTRUM GIANT RADIO GALAXY WITH RECURRENT RADIO JET ACTIVITY IN ABELL 449

International Nuclear Information System (INIS)

Hunik, Dominika; Jamrozy, Marek

2016-01-01

We report a discovery of a 1.3 Mpc diffuse radio source with extremely steep spectrum fading radio structures in the vicinity of the Abell 449 cluster of galaxies. Its extended diffuse lobes are bright only at low radio frequencies and their synchrotron age is about 160 Myr. The parent galaxy of the extended relic structure, which is the dominant galaxy within the cluster, is starting a new jet activity. There are three weak X-rays sources in the vicinity of the cluster as found in the ROSAT survey, however it is not known if they are connected with this cluster of galaxies. Just a few radio galaxy relics are currently known in the literature, as finding them requires sensitive and high angular resolution low-frequency radio observations. Objects of this kind, which also are starting a new jet activity, are important for understanding the life cycle and evolution of active galactic nuclei. A new 613 MHz map as well as the archival radio data pertaining to this object are presented and analyzed

Radio observations of the double-relic galaxy cluster Abell 1240

Science.gov (United States)

Hoang, D. N.; Shimwell, T. W.; van Weeren, R. J.; Intema, H. T.; Röttgering, H. J. A.; Andrade-Santos, F.; Akamatsu, H.; Bonafede, A.; Brunetti, G.; Dawson, W. A.; Golovich, N.; Best, P. N.; Botteon, A.; Brüggen, M.; Cassano, R.; de Gasperin, F.; Hoeft, M.; Stroe, A.; White, G. J.

2018-05-01

We present LOFAR 120 - 168 MHz images of the merging galaxy cluster Abell 1240 that hosts double radio relics. In combination with the GMRT 595 - 629 MHz and VLA 2 - 4 GHz data, we characterised the spectral and polarimetric properties of the radio emission. The spectral indices for the relics steepen from their outer edges towards the cluster centre and the electric field vectors are approximately perpendicular to the major axes of the relics. The results are consistent with the picture that these relics trace large-scale shocks propagating outwards during the merger. Assuming diffusive shock acceleration (DSA), we obtain shock Mach numbers of M=2.4 and 2.3 for the northern and southern shocks, respectively. For M≲ 3 shocks, a pre-existing population of mildly relativistic electrons is required to explain the brightness of the relics due to the high (>10 per cent) particle acceleration efficiency required. However, for M≳ 4 shocks the required efficiency is ≳ 1% and ≳ 0.5%, respectively, which is low enough for shock acceleration directly from the thermal pool. We used the fractional polarization to constrain the viewing angle to ≥53 ± 3° and ≥39 ± 5° for the northern and southern shocks, respectively. We found no evidence for diffuse emission in the cluster central region. If the halo spans the entire region between the relics (˜1.8 Mpc) our upper limit on the power is P1.4GHz = (1.4 ± 0.6) × 1023 W Hz-1 which is approximately equal to the anticipated flux from a cluster of this mass. However, if the halo is smaller than this, our constraints on the power imply that the halo is underluminous.

Complex Structure of Galaxy Cluster Abell 1689: Evidence for a Merger from X-Ray Data?

Energy Technology Data Exchange (ETDEWEB)

Andersson, K

2004-01-29

Abell 1689 is a galaxy cluster at z = 0:183 where previous measurements of its mass using various techniques gave discrepant results. We present a new detailed measurement of the mass with the data based on X-ray observations with the European Photon Imaging Camera aboard the XMM-Newton Observatory, determined by using an unparameterized deprojection technique. Fitting the total mass profile to a Navarro-Frenk-White model yields halo concentration c = 7.2{sub -2.4}{sup +1.6} and r{sub 200} = 1.13 {+-} 0.21 h{sup -1} Mpc, corresponding to a mass which is less than half of what is found from gravitational lensing. Adding to the evidence of substructure from optical observations, X-ray analysis shows a highly asymmetric temperature profile and a non-uniform redshift distribution implying large scale relative motion of the gas. A lower than expected gas mass fraction f{sub gas} = 0.072 {+-} 0.008 (for a flat {Lambda}CDM cosmology) suggests a complex spatial and/or dynamical structure. We also find no signs of any additional absorbing component previously reported on the basis of the Chandra data, confirming the XMM low energy response using data from ROSAT.

A Statistical Study of Multiply Imaged Systems in the Lensing Cluster Abell 68

Science.gov (United States)

Richard, Johan; Kneib, Jean-Paul; Jullo, Eric; Covone, Giovanni; Limousin, Marceau; Ellis, Richard; Stark, Daniel; Bundy, Kevin; Czoske, Oliver; Ebeling, Harald; Soucail, Geneviève

2007-06-01

We have carried out an extensive spectroscopic survey with the Keck and VLT telescopes, targeting lensed galaxies in the background of the massive cluster Abell 68. Spectroscopic measurements are obtained for 26 lensed images, including a distant galaxy at z=5.4. Redshifts have been determined for 5 out of 7 multiple-image systems. Through a careful modeling of the mass distribution in the strongly lensed regime, we derive a mass estimate of 5.3×1014 Msolar within 500 kpc. Our mass model is then used to constrain the redshift distribution of the remaining multiply imaged and singly imaged sources. This enables us to examine the physical properties for a subsample of 7 Lyα emitters at 1.7financial support of the W. M. Keck Foundation. Also based on observations collected at the Very Large Telescope (Antu/UT1 and Melipal/UT3), European Southern Observatory, Paranal, Chile (ESO programs 070.A-0643 and 073.A-0774), the NASA/ESA Hubble Space Telescope (program 8249) obtained at the Space Telescope Science Institute, which is operated by AURA under NASA contract NAS5-26555, and the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.

TRACING MULTIPLE GENERATIONS OF ACTIVE GALACTIC NUCLEUS FEEDBACK IN THE CORE OF ABELL 262

International Nuclear Information System (INIS)

Clarke, T. E.; Kassim, N. E.; Blanton, E. L.; Anderson, L. D.; Douglass, E. M.; Sarazin, C. L.; Gopal-Krishna

2009-01-01

We present new radio and X-ray observations of Abell 262. The X-ray residual image provides the first evidence of an X-ray tunnel in this system while the radio data reveal that the central radio source is more than three times larger than previously known. We find that the well-known cluster-center S-shaped radio source B2 0149+35 is surrounded by extended emission to the east and southwest. The south-western extension is cospatial with the X-ray tunnel seen in our new Chandra images while the eastern extension shows three clumps of emission with the innermost coincident with a faint X-ray cavity. The outer two eastern radio extensions are coincident with a newly detected X-ray depression. We use the projected separation of the emission regions to estimate a lower limit of τ rep = 28 Myr to the outburst repetition timescale of the central active galactic nucleus (AGN). The total energy input into the cluster over multiple outburst episodes is estimated to be 2.2 x 10 58 erg, more than an order of magnitude larger than previously thought. The total AGN energy output determined from our new observations shows that the source should be capable of offsetting radiative cooling over several outburst episodes.

Structure and Formation of cD Galaxies: NGC 6166 in ABELL 2199

Science.gov (United States)

Bender, Ralf; Kormendy, John; Cornell, Mark E.; Fisher, David B.

2015-07-01

 Hobby-Eberly Telescope (HET) spectroscopy is used to measure the velocity dispersion profile of the nearest prototypical cD galaxy, NGC 6166 in the cluster Abell 2199. We also present composite surface photometry from many telescopes. We confirm the defining feature of a cD galaxy; i.e., (we suggest), a halo of stars that fills the cluster center and that is controlled dynamically by cluster gravity, not by the central galaxy. Our HET spectroscopy shows that the velocity dispersion of NGC 6166 rises from σ ≃ 300 km s-1 in the inner r˜ 10\\prime\\prime to σ =865+/- 58 km s-1 at r ˜ 100″ in the cD halo. This extends published observations of an outward σ increase and shows for the first time that σ rises all the way to the cluster velocity dispersion of 819 ± 32 km s-1. We also observe that the main body of NGC 6166 moves at +206 ± 39 km s-1 with respect to the cluster mean velocity, but the velocity of the inner cD halo is ˜70 km s-1 closer to the cluster velocity. These results support our picture that cD halos consist of stars that were stripped from individual cluster galaxies by fast tidal encounters.  However, our photometry does not confirm the widespread view that cD halos are identifiable as an extra, low-surface-brightness component that is photometrically distinct from the inner, steep-Sérsic-function main body of an otherwise-normal giant elliptical galaxy. Instead, all of the brightness profile of NGC 6166 outside its core is described to ±0.037 V mag arcsec-2 by a single Sérsic function with index n≃ 8.3. The cD halo is not recognizable from photometry alone. This blurs the distinction between cluster-dominated cD halos and the similarly-large-Sérsic-index halos of giant, core-boxy-nonrotating ellipticals. These halos are believed to be accreted onto compact, high-redshift progenitors (“red nuggets”) by large numbers of minor mergers. They belong dynamically to their central galaxies. Still, cDs and core-boxy-nonrotating Es

Review: Petia Genkova & Andrea E. Abele (Eds.) (2008). Lernen und Entwicklung im globalen Kontext. "Heimliche Lehrpläne" und Basiskompetenzen [Learning and Development in a Global Context. Hidden Curriculum and Base Competencies

OpenAIRE

Dörte Bernhard

2011-01-01

This anthology addresses globalization with regard to the world of work. How can women pursue their career and enjoy equal opportunities in the labor market? How can employees be supported during the process of company acquisition? How can the existential crises of young adults that were triggered through institutional work experiences be met and coped with? How can violence among children and adolescents be prevented? Seventeen contributions in Petia GENKOVA's and Andrea E. ABELE's anthology...

„This is just a fucking movie. Also fahrt ab damit!“ Eine Rezensionsreise durch Abel Ferraras Film ‚Pasolini‘, anlässlich des 40. Todestages von Pier Paolo Pasolini

Directory of Open Access Journals (Sweden)

Angela Oster

2015-06-01

Full Text Available Das Leben Pasolinis ist bereits zu wiederholten Malen der Gegenstand von Texten und Filmen gewesen. Aufgrund des skandalträchtigen Todes des Linksintellektuellen – er wurde unter nie genau geklärten Umständen 1975 ermordet – ranken sich viele Mythen um den letzten Tag Pasolinis. Genau diesen 'ultimo giorno' verfilmt Abel Ferrara (1914 und setzt dabei eigene Akzente. Mit literar- und dokumentargenauer Perspektive bietet Ferrara gleichwohl innovative Interpretationen in Hinblick auf einen der wichtigsten Künstler Italiens.

ASTROMETRY WITH THE HUBBLE SPACE TELESCOPE: TRIGONOMETRIC PARALLAXES OF PLANETARY NEBULA NUCLEI NGC 6853, NGC 7293, ABELL 31, AND DeHt 5

International Nuclear Information System (INIS)

Benedict, G. Fritz; McArthur, Barbara E.; Napiwotzki, Ralf; Harrison, Thomas E.; Harris, Hugh C.; Nelan, Edmund; Bond, Howard E.; Patterson, Richard J.; Ciardullo, Robin

2009-01-01

We present absolute parallaxes and relative proper motions for the central stars of the planetary nebulae NGC 6853 (The Dumbbell), NGC 7293 (The Helix), Abell 31, and DeHt 5. This paper details our reduction and analysis using DeHt 5 as an example. We obtain these planetary nebula nuclei (PNNi) parallaxes with astrometric data from Fine Guidance Sensors FGS 1r and FGS 3, white-light interferometers on the Hubble Space Telescope. Proper motions, spectral classifications and VJHKT 2 M and DDO51 photometry of the stars comprising the astrometric reference frames provide spectrophotometric estimates of reference star absolute parallaxes. Introducing these into our model as observations with error, we determine absolute parallaxes for each PNN. Weighted averaging with previous independent parallax measurements yields an average parallax precision, σ π /π = 5%. Derived distances are: d NGC6853 = 405 +28 -25 pc, d NGC7293 = 216 +14 -12 pc, d Abell31 = 621 +91 -70 pc, and d DeHt5 = 345 +19 -17 pc. These PNNi distances are all smaller than previously derived from spectroscopic analyses of the central stars. To obtain absolute magnitudes from these distances requires estimates of interstellar extinction. We average extinction measurements culled from the literature, from reddening based on PNNi intrinsic colors derived from model SEDs, and an assumption that each PNN experiences the same rate of extinction as a function of distance as do the reference stars nearest (in angular separation) to each central star. We also apply Lutz-Kelker bias corrections. The absolute magnitudes and effective temperatures permit estimates of PNNi radii through both the Stefan-Boltzmann relation and Eddington fluxes. Comparing absolute magnitudes with post-AGB models provides mass estimates. Masses cluster around 0.57 M odot , close to the peak of the white dwarf mass distribution. Adding a few more PNNi with well-determined distances and masses, we compare all the PNNi with cooler white

Twin radio relics in the nearby low-mass galaxy cluster Abell 168

Science.gov (United States)

Dwarakanath, K. S.; Parekh, V.; Kale, R.; George, L. T.

2018-06-01

We report the discovery of twin radio relics in the outskirts of the low-mass merging galaxy cluster Abell 168 (redshift=0.045). One of the relics is elongated with a linear extent ˜800 kpc and projected width of ˜80 kpc and is located ˜900 kpc towards the north of the cluster centre, oriented roughly perpendicular to the major axis of the X-ray emission. The second relic is ring-shaped with a size ˜220 kpc and is located near the inner edge of the elongated relic at a distance of ˜600 kpc from the cluster centre. These radio sources were imaged at 323 and 608 MHz with the Giant Meterwave Radio Telescope and at 1520 MHz with the Karl G. Jansky Very Large Array (VLA). The elongated relic was detected at all frequencies, with a radio power of 1.38 ± 0.14 × 1023 W Hz-1 at 1.4 GHz and a power law in the frequency range 70-1500 MHz (S ∝ να, α = -1.1 ± 0.04). This radio power is in good agreement with that expected from the known empirical relation between the radio powers of relics and host cluster masses. This is the lowest mass (M500 = 1.24 × 1014 M⊙) cluster in which relics due to merger shocks are detected. The ring-shaped relic has a steeper spectral index (α) of -1.74 ± 0.29 in the frequency range 100-600 MHz. We propose this relic to be an old plasma, revived due to adiabatic compression by the outgoing shock that produced the elongated relic.

Discovery of large-scale diffuse radio emission in low-mass galaxy cluster Abell 1931

Science.gov (United States)

Brüggen, M.; Rafferty, D.; Bonafede, A.; van Weeren, R. J.; Shimwell, T.; Intema, H.; Röttgering, H.; Brunetti, G.; Di Gennaro, G.; Savini, F.; Wilber, A.; O'Sullivan, S.; Ensslin, T. A.; De Gasperin, F.; Hoeft, M.

2018-04-01

Extended, steep-spectrum radio synchrotron sources are pre-dominantly found in massive galaxy clusters as opposed to groups. LOFAR Two-Metre Sky Survey images have revealed a diffuse, ultra-steep spectrum radio source in the low-mass cluster Abell 1931. The source has a fairly irregular morphology with a largest linear size of about 550 kpc. The source is only seen in LOFAR observations at 143 MHz and GMRT observations at 325 MHz. The spectral index of the total source between 143 MHz and 325 MHz is α _{143}^{325} = -2.86 ± 0.36. The source remains invisible in Very Large Array (1-2 GHz) observations as expected given the spectral index. Chandra X-ray observations of the cluster revealed a bolometric luminosity of LX = (1.65 ± 0.39) × 1043 erg s-1 and a temperature of 2.92_{-0.87}^{+1.89} keV which implies a mass of around ˜1014M⊙. We conclude that the source is a remnant radio galaxy that has shut off around 200 Myr ago. The brightest cluster galaxy, a radio-loud elliptical galaxy, could be the source for this extinct source. Unlike remnant sources studied in the literature, our source has a steep spectrum at low radio frequencies. Studying such remnant radio galaxies at low radio frequencies is important for understanding the scarcity of such sources and their role in feedback processes.

Abell-35 Phenomena in Symbiotic Stars: Discovery of 1.2 and 6.4 Day Periods in VV8 (V471 Per

Directory of Open Access Journals (Sweden)

Munari U.

2012-06-01

Full Text Available We have collected high precision optical photometry of VV8, so far 782 individual observing runs uniformly distributed over the period 2005 - 2011. This dataset allows us to refine the known long periodicity of VV8 to P = 16.8 yr, with peak-to-valley amplitudes of ΔB = 0.18 and ΔV = 0.14 mag. In addition, we have discovered two new periodicities: 6.431 d (total amplitude ΔB = ΔV = ΔI = 0.05 mag and 1.185 d (ΔB = 0.022, ΔV = 0.018, ΔI = 0.014 mag. These two short periods are reminiscent of the Abell-35 phenomena displayed by binary nuclei of planetary nebulae that have gone through a common envelope phase. Twice the 6.431 d period would nicely correspond to the double-peaked light-curve that the G5 III star in VV8 would display if its Roche lobe would be ellipsoidally distorted.

Uniform Contribution of Supernova Explosions to the Chemical Enrichment of Abell 3112 out to R{sub 200}

Energy Technology Data Exchange (ETDEWEB)

Ezer, Cemile; Ercan, E. Nihal [Department of Physics, Boğaziçi University, Istanbul (Turkey); Bulbul, Esra; Bautz, Mark W.; McDonald, Mike; Miller, Eric D. [Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States); Smith, Randall K. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Loewenstein, Mike, E-mail: cemile.ezer@boun.edu.tr [NASA Goddard Space Flight Center, Greenbelt, MD (United States)

2017-02-10

The spatial distribution of the metals residing in the intra-cluster medium (ICM) of galaxy clusters records all the information on a cluster’s nucleosynthesis and chemical enrichment history. We present measurements from a total of 1.2 Ms Suzaku XIS and 72 ks Chandra observations of the cool-core galaxy cluster Abell 3112 out to its virial radius (∼1470 kpc). We find that the ratio of the observed supernova type Ia explosions to the total supernova explosions has a uniform distribution at a level of 12%–16% out to the cluster’s virial radius. The observed fraction of type Ia supernova explosions is in agreement with the corresponding fraction found in our Galaxy and the chemical enrichment of our Galaxy. The non-varying supernova enrichment suggests that the ICM in cluster outskirts was enriched by metals at an early stage before the cluster itself was formed during a period of intense star formation activity. Additionally, we find that the 2D delayed detonation model CDDT produce significantly worse fits to the X-ray spectra compared to simple 1D W7 models. This is due to the relative overestimate of Si, and the underestimate of Mg in these models with respect to the measured abundances.

EVALUACIÓN DE LA POLÍTICA SOCIAL DE COMBATE A LA POBREZA DE LA ADMINISTRACIÓN DEL DR. ABEL PACHECO DE LA ESPRIELLA (2002-2005

Directory of Open Access Journals (Sweden)

Roxana Morales Ramos

2005-12-01

Full Text Available Ante la severidad de la pobreza imperante en América Latina, los mandatarios de los países de la región, en una reunión en el año 2000 (Cumbre del Milenio organizada por las Naciones Unidas,acordaron como prioridad inmediata la reducción de la pobreza extrema a nivel mundial. El gobierno del presidente Abel ha sido parte de este compromiso dando prioridad al combate a la pobreza mediante sus “políticas sociales”, por ello pretendemos en nuestro trabajo realizar una evaluación de la estrategia propuesta por el mismo, con el fin de ver si se han cumplido o no los objetivos y las metas propuestas en el “Plan Nacional de Desarrollo” y “Plan Vida Nueva”.

Empiema pleural no tuberculoso: resultados en el Hospital «Abel Santamaría Cuadrado» (2000 a 2004 Non-tuberculous pleural empyema: results in “Abel Santamaría Cuadrado” Hospital (2000-2004

Directory of Open Access Journals (Sweden)

Ivanis Ruizcalderón Cabrera

2007-03-01

Full Text Available El empiema pleural es una enfermedad infecciosa de incidencia moderada en nuestro medio, de diagnóstico fácil y de tratamiento exitoso cuando se logra descubrir a tiempo. Sin embargo, su persistencia determina la aparición de secuelas con impacto importante en la morbilidad y mortalidad del paciente. Realizamos un estudio retrospectivo, transversal y descriptivo en el que se hace una evaluación del tratamiento de los pacientes con empiema pleural no tuberculoso tratados en el Servicio de Cirugía General del Hospital «Abel Santamaría Cuadrado» entre enero de 2000 y diciembre de 2004. En una muestra de 34 pacientes fueron estudiadas las variables: edad, sexo, causa, gérmenes, tratamiento adoptado. Se observó que el grupo de edad más afectado fue el de 41 a 60 años (17 pacientes; 50 % y sobre todo, los pacientes del sexo masculino (82,4 %, con una relación de 3,8:1. En el 61,8 % de los pacientes se encontraron enfermedades pulmonares asociadas y los gérmenes patógenos más frecuentes fueron el Staphylococcus aureus (29,4 % y el Streptococcus pneumoniae(20,6 %. El mayor porcentaje de los casos fue resuelto mediante cirugía torácica videoasistida (32,4 %. La mayoría de los pacientes llegó a los servicios quirúrgicos en las fases avanzadas de la afección y se apreció un incremento de los cultivos mixtos de gérmenes patógenos. El tratamiento más agresivo de las colecciones purulentas fue el de mejor resultado

Revolving scheme for solving a cascade of Abel equations in dynamics of planar satellite rotation

Directory of Open Access Journals (Sweden)

Sergey V. Ershkov

2017-05-01

Full Text Available The main objective for this research was the analytical exploration of the dynamics of planar satellite rotation during the motion of an elliptical orbit around a planet. First, we revisit the results of J. Wisdom et al. (1984, in which, by the elegant change of variables (considering the true anomaly f as the independent variable, the governing equation of satellite rotation takes the form of an Abel ordinary differential equation (ODE of the second kind, a sort of generalization of the Riccati ODE. We note that due to the special character of solutions of a Riccati-type ODE, there exists the possibility of sudden jumping in the magnitude of the solution at some moment of time. In the physical sense, this jumping of the Riccati-type solutions of the governing ODE could be associated with the effect of sudden acceleration/deceleration in the satellite rotation around the chosen principle axis at a definite moment of parametric time. This means that there exists not only a chaotic satellite rotation regime (as per the results of J. Wisdom et al. (1984, but a kind of gradient catastrophe (Arnold, 1992 could occur during the satellite rotation process. We especially note that if a gradient catastrophe could occur, this does not mean that it must occur: such a possibility depends on the initial conditions. In addition, we obtained asymptotical solutions that manifest a quasi-periodic character even with the strong simplifying assumptions e→0, p=1, which reduce the governing equation of J. Wisdom et al. (1984 to a kind of Beletskii’s equation.

VizieR Online Data Catalog: Ultradiffuse galaxies found in deep HST images of HFF (Lee+, 2017)

Science.gov (United States)

Lee, M. G.; Kang, J.; Lee, J. H.; Jang in, S.

2018-03-01

Abell S1063 and Abell 2744 are located at redshift z=0.348 and z=0.308, respectively, so their HST fields cover a relatively large fraction of each cluster. They are part of the target galaxy clusters in the Hubble Frontier Fields (HFF) Program, for which deep Hubble Space Telescope (HST) images are available (Lotz+ 2017ApJ...837...97L). We used ACS/F814W(I) and WFC3/F105W(Y) images for Abell S1063 and Abell 2744 in the HFF. The effective wavelengths of the F814W and F105W filters for the redshifts of Abell S1063 and Abell 2744 (6220 and 8030Å) correspond approximately to SDSS r' and Cousins I (or SDSS i') in the rest frame, respectively. Figure 1 display color images of the HST fields for Abell S1063 and Abell 2744. In this study we adopt the cosmological parameters H0=73km/s/Mpc, ΩM=0.27, and ΩΛ=0.73. For these parameters, luminosity distance moduli of Abell S1063 and Abell 2744 are (m-M)0=41.25 (d=1775Mpc) and 40.94 (d=1540Mpc), and angular diameter distances are 978 and 901Mpc, respectively. (5 data files).

Interview with Mikhail Gromov

DEFF Research Database (Denmark)

Raussen, Martin; Skau, Christian

2010-01-01

Mikhail Gromov is the recipient of the 2009 Abel Prize. The interview was made on May 18th, 2009, prior to the Abel Prize Celebration.......Mikhail Gromov is the recipient of the 2009 Abel Prize. The interview was made on May 18th, 2009, prior to the Abel Prize Celebration....

A multiwavelength view of the galaxy cluster Abell 523 and its peculiar diffuse radio source

Science.gov (United States)

Girardi, M.; Boschin, W.; Gastaldello, F.; Giovannini, G.; Govoni, F.; Murgia, M.; Barrena, R.; Ettori, S.; Trasatti, M.; Vacca, V.

2016-03-01

We study the structure of the galaxy cluster Abell 523 (A523) at z = 0.104 using new spectroscopic data for 132 galaxies acquired at the Telescopio Nazionale Galileo, new photometric data from the Isaac Newton Telescope, and X-ray and radio data from the Chandra and Very Large Array archives. We estimate the velocity dispersion of the galaxy population, σ _V=949_{-60}^{+80} km s-1, and the X-ray temperature of the hot intracluster medium, kT = 5.3 ± 0.3 keV. We infer that A523 is a massive system: M200 ˜ 7-9 × 1014 M⊙. The analysis of the optical data confirms the presence of two subclusters, 0.75 Mpc apart, tracing the SSW-NNE direction and dominated by the two brightest cluster galaxies (BCG1 and BCG2). The X-ray surface brightness is strongly elongated towards the NNE direction, and its peak is clearly offset from both the brightest cluster galaxies (BCGs). We confirm the presence of a 1.3 Mpc large radio halo, elongated in the ESE-WNW direction and perpendicular to the optical/X-ray elongation. We detect a significant radio/X-ray offset and radio polarization, two features which might be the result of a magnetic field energy spread on large spatial scales. A523 is found consistent with most scaling relations followed by clusters hosting radio haloes, but quite peculiar in the Pradio-LX relation: it is underluminous in the X-rays or overluminous in radio. A523 can be described as a binary head-on merger caught after a collision along the SSW-NNE direction. However, minor optical and radio features suggest a more complex cluster structure, with A523 forming at the crossing of two filaments along the SSW-NNE and ESE-WNW directions.

POST-MERGER SIGNATURES OF RED-SEQUENCE GALAXIES IN RICH ABELL CLUSTERS AT z ∼< 0.1

International Nuclear Information System (INIS)

Sheen, Yun-Kyeong; Yi, Sukyoung K.; Lee, Jaehyun; Ree, Chang H.

2012-01-01

We have investigated the post-merger signatures of red-sequence galaxies in rich Abell clusters at z ∼ r < –20) cluster red-sequence galaxies show post-merger signatures in four clusters consistently. Most (∼71%) of the featured galaxies were found to be bulge dominated, and for the subsample of bulge-dominated red-sequence galaxies, the post-merger fraction rises to ∼38%. We also found that roughly 4% of bulge-dominated red-sequence galaxies interact (ongoing merger). A total of 42% (38% post-merger, 4% ongoing merger) of galaxies show merger-related features. Compared to a field galaxy study with a similar limiting magnitude by van Dokkum in 2005, our cluster study presents a similar post-merger fraction but a markedly lower ongoing merger fraction. The merger fraction derived is surprisingly high for the high density of our clusters, where the fast internal motions of galaxies are thought to play a negative role in galaxy mergers. The fraction of post-merger and ongoing merger galaxies can be explained as follows. Most of the post-merger galaxies may have carried over their merger features from their previous halo environment, whereas interacting galaxies interact in the current cluster in situ. According to our semi-analytic calculation, massive cluster halos may very well have experienced tens of halo mergers over the last 4-5 Gyr; post-merger features last that long, allowing these features to be detected in our clusters today. The apparent lack of dependence of the merger fraction on the clustocentric distance is naturally explained this way. In this scenario, the galaxy morphology and properties can be properly interpreted only when the halo evolution characteristics are understood first.

LOFAR discovery of a double radio halo system in Abell 1758 and radio/X-ray study of the cluster pair

Science.gov (United States)

Botteon, A.; Shimwell, T. W.; Bonafede, A.; Dallacasa, D.; Brunetti, G.; Mandal, S.; van Weeren, R. J.; Brüggen, M.; Cassano, R.; de Gasperin, F.; Hoang, D. N.; Hoeft, M.; Röttgering, H. J. A.; Savini, F.; White, G. J.; Wilber, A.; Venturi, T.

2018-05-01

Radio halos and radio relics are diffuse synchrotron sources that extend over Mpc-scales and are found in a number of merger galaxy clusters. They are believed to form as a consequence of the energy that is dissipated by turbulence and shocks in the intra-cluster medium (ICM). However, the precise physical processes that generate these steep synchrotron spectrum sources are still poorly constrained. We present a new LOFAR observation of the double galaxy cluster Abell 1758. This system is composed of A1758N, a massive cluster hosting a known giant radio halo, and A1758S, which is a less massive cluster whose diffuse radio emission is confirmed here for the first time. Our observations have revealed a radio halo and a candidate radio relic in A1758S, and a suggestion of emission along the bridge connecting the two systems which deserves confirmation. We combined the LOFAR data with archival VLA and GMRT observations to constrain the spectral properties of the diffuse emission. We also analyzed a deep archival Chandra observation and used this to provide evidence that A1758N and A1758S are in a pre-merger phase. The ICM temperature across the bridge that connects the two systems shows a jump which might indicate the presence of a transversal shock generated in the initial stage of the merger.

Abell 1367: a high fraction of late-type galaxies displaying H I morphological and kinematic perturbations

Science.gov (United States)

Scott, T. C.; Brinks, E.; Cortese, L.; Boselli, A.; Bravo-Alfaro, H.

2018-04-01

To investigate the effects the cluster environment has on late-type galaxies (LTGs), we studied H I perturbation signatures for all Abell 1367 LTGs with H I detections. We used new Very Large Array H I observations combined with AGES single-dish blind survey data. Our study indicates that the asymmetry between the high- and low-velocity wings of the characteristic double-horn-integrated H I spectrum as measured by the asymmetry parameter, A_{flux}, can be a useful diagnostic for ongoing and/or recent H I stripping. 26 per cent of A1367 LTGs have an A_{flux} ratio, more asymmetrical than 3 times the 1σ spread in the A_{flux} ratio distribution of an undisturbed sample of isolated galaxies (2 per cent) and samples from other denser environments (10 per cent-20 per cent). Over half of the A1367 LTGs, which are members of groups or pairs, have an A_{flux} ratio larger than twice the 1σ spread found in the isolated sample. This suggests intergroup/pair interactions could be making a significant contribution to the LTGs displaying such A_{flux} ratios. The study also demonstrates that the definition of the H I offset from the optical centre of LTGs is resolution dependent, suggesting that unresolved AGES H I offsets that are significantly larger than the pointing uncertainties (>2σ), reflect interactions which have asymmetrically displaced, significant masses of lower density H I, while having minimal impact on the location of the highest density H I in resolved maps. The distribution of A_{flux} from a comparable sample of Virgo galaxies provides a clear indication that the frequency of H I profile perturbations is lower than in A1367.

An R package "VariABEL" for genome-wide searching of potentially interacting loci by testing genotypic variance heterogeneity

Directory of Open Access Journals (Sweden)

Struchalin Maksim V

2012-01-01

Full Text Available Abstract Background Hundreds of new loci have been discovered by genome-wide association studies of human traits. These studies mostly focused on associations between single locus and a trait. Interactions between genes and between genes and environmental factors are of interest as they can improve our understanding of the genetic background underlying complex traits. Genome-wide testing of complex genetic models is a computationally demanding task. Moreover, testing of such models leads to multiple comparison problems that reduce the probability of new findings. Assuming that the genetic model underlying a complex trait can include hundreds of genes and environmental factors, testing of these models in genome-wide association studies represent substantial difficulties. We and Pare with colleagues (2010 developed a method allowing to overcome such difficulties. The method is based on the fact that loci which are involved in interactions can show genotypic variance heterogeneity of a trait. Genome-wide testing of such heterogeneity can be a fast scanning approach which can point to the interacting genetic variants. Results In this work we present a new method, SVLM, allowing for variance heterogeneity analysis of imputed genetic variation. Type I error and power of this test are investigated and contracted with these of the Levene's test. We also present an R package, VariABEL, implementing existing and newly developed tests. Conclusions Variance heterogeneity analysis is a promising method for detection of potentially interacting loci. New method and software package developed in this work will facilitate such analysis in genome-wide context.

The mystery of the "Kite" radio source in Abell 2626: Insights from new Chandra observations

Science.gov (United States)

Ignesti, A.; Gitti, M.; Brunetti, G.; O'Sullivan, E.; Sarazin, C.; Wong, K.

2018-03-01

Context. We present the results of a new Chandra study of the galaxy cluster Abell 2626. The radio emission of the cluster shows a complex system of four symmetric arcs without known correlations with the thermal X-ray emission. The mirror symmetry of the radio arcs toward the center and the presence of two optical cores in the central galaxy suggested that they may be created by pairs of precessing radio jets powered by dual active galactic nuclei (AGNs) inside the core dominant galaxy. However, previous observations failed to observe the second jetted AGN and the spectral trend due to radiative age along the radio arcs, thus challenging this interpretation. Aim. The new Chandra observation had several scientific objectives, including the search for the second AGN that would support the jet precession model. We focus here on the detailed study of the local properties of the thermal and non-thermal emission in the proximity of the radio arcs, in order to obtain further insights into their origin. Methods: We performed a standard data reduction of the Chandra dataset deriving the radial profiles of temperature, density, pressure and cooling time of the intra-cluster medium. We further analyzed the two-dimensional (2D) distribution of the gas temperature, discovering that the south-western junction of the radio arcs surrounds the cool core of the cluster. Results: We studied the X-ray surface brightness and spectral profiles across the junction, finding a cold front spatially coincident with the radio arcs. This may suggest a connection between the sloshing of the thermal gas and the nature of the radio filaments, raising new scenarios for their origin. A tantalizing possibility is that the radio arcs trace the projection of a complex surface connecting the sites where electrons are most efficiently reaccelerated by the turbulence that is generated by the gas sloshing. In this case, diffuse emission embedded by the arcs and with extremely steep spectrum should be

Low frequency radio observations of five rich clusters of galaxies

International Nuclear Information System (INIS)

Hanisch, R.J.; Erickson, W.C.

1980-01-01

Observations have been made at 43.0 and 73.8 MHz of five rich x-ray emitting clusters of galaxies: Abell 399/401, Abell 426 (the Perseus cluster), Abell 1367, Abell 1656 (the Coma cluster), and the Virgo cluster. A fan beam synthesis system has been used to search for extended radio emission, i.e., radio halos, in these clusters. Radio halos were detected in the Coma and Virgo clusters. No evidence was found for the existence of 3C84B, the halo source previously thought to exist in the Perseus cluster. If halo sources exist in Abell 399/401 or Abell 1367, they must be quite weak at frequencies less than 100 MHz. The observed sizes of the extended sources in Coma and Virgo imply that the rate of particle propagation away from strong radio galaxies greatly exceeds the Alfven velocity and is probably independent of particle energy

Close entrainment of massive molecular gas flows by radio bubbles in the central galaxy of Abell 1795

Science.gov (United States)

Russell, H. R.; McNamara, B. R.; Fabian, A. C.; Nulsen, P. E. J.; Combes, F.; Edge, A. C.; Hogan, M. T.; McDonald, M.; Salomé, P.; Tremblay, G.; Vantyghem, A. N.

2017-12-01

We present new ALMA observations tracing the morphology and velocity structure of the molecular gas in the central galaxy of the cluster Abell 1795. The molecular gas lies in two filaments that extend 5-7 kpc to the N and S from the nucleus and project exclusively around the outer edges of two inner radio bubbles. Radio jets launched by the central active galactic nucleus have inflated bubbles filled with relativistic plasma into the hot atmosphere surrounding the central galaxy. The N filament has a smoothly increasing velocity gradient along its length from the central galaxy's systemic velocity at the nucleus to -370 km s^{-1}, the average velocity of the surrounding galaxies, at the furthest extent. The S filament has a similarly smooth but shallower velocity gradient and appears to have partially collapsed in a burst of star formation. The close spatial association with the radio lobes, together with the ordered velocity gradients and narrow velocity dispersions, shows that the molecular filaments are gas flows entrained by the expanding radio bubbles. Assuming a Galactic XCO factor, the total molecular gas mass is 3.2 ± 0.2 × 109 M⊙. More than half lies above the N radio bubble. Lifting the molecular clouds appears to require an infeasibly efficient coupling between the molecular gas and the radio bubble. The energy required also exceeds the mechanical power of the N radio bubble by a factor of 2. Stimulated feedback, where the radio bubbles lift low-entropy X-ray gas that becomes thermally unstable and rapidly cools in situ, provides a plausible model. Multiple generations of radio bubbles are required to lift this substantial gas mass. The close morphological association then indicates that the cold gas either moulds the newly expanding bubbles or is itself pushed aside and shaped as they inflate.

The Kormendy relation of galaxies in the Frontier Fields clusters: Abell S1063 and MACS J1149.5+2223

Science.gov (United States)

Tortorelli, Luca; Mercurio, Amata; Paolillo, Maurizio; Rosati, Piero; Gargiulo, Adriana; Gobat, Raphael; Balestra, Italo; Caminha, G. B.; Annunziatella, Marianna; Grillo, Claudio; Lombardi, Marco; Nonino, Mario; Rettura, Alessandro; Sartoris, Barbara; Strazzullo, Veronica

2018-06-01

We analyse the Kormendy relations (KRs) of the two Frontier Fields clusters, Abell S1063, at z = 0.348, and MACS J1149.5+2223, at z = 0.542, exploiting very deep Hubble Space Telescope photometry and Very Large Telescope (VLT)/Multi Unit Spectroscopic Explorer (MUSE) integral field spectroscopy. With this novel data set, we are able to investigate how the KR parameters depend on the cluster galaxy sample selection and how this affects studies of galaxy evolution based on the KR. We define and compare four different galaxy samples according to (a) Sérsic indices: early-type (`ETG'), (b) visual inspection: `ellipticals', (c) colours: `red', (d) spectral properties: `passive'. The classification is performed for a complete sample of galaxies with mF814W ≤ 22.5 ABmag (M* ≳ 1010.0 M⊙). To derive robust galaxy structural parameters, we use two methods: (1) an iterative estimate of structural parameters using images of increasing size, in order to deal with closely separated galaxies and (2) different background estimations, to deal with the intracluster light contamination. The comparison between the KRs obtained from the different samples suggests that the sample selection could affect the estimate of the best-fitting KR parameters. The KR built with ETGs is fully consistent with the one obtained for ellipticals and passive. On the other hand, the KR slope built on the red sample is only marginally consistent with those obtained with the other samples. We also release the photometric catalogue with structural parameters for the galaxies included in the present analysis.

14. II kell 14 esitletakse EKMi Rüütelkonna hoones...

Index Scriptorium Estoniae

2005-01-01

Esitletakse raamatuid "Eesti kunst. 101 teost Eesti kunstimuuseumi kogudest" (autorid: Tiina Abel, Eha Komissarov, Hanno Soans, koostanud T. Abel, E. Komissarov, H. Soans ja Kädi Talvoja, kujundanud Anu Lemsalu), "Kunstnik ja tema kodu. C. T. von Neffi kunstikogu Piira ja Muuga mõisast" (koostanud Tiina Abel, kujundanud Andres Tali) ja Kiwa "Roboti tee on nihe. Salatühik"

Probing the non-thermal emission in Abell 2146 and the Perseus cluster with the JVLA

Science.gov (United States)

Gendron-Marsolais, Marie-Lou; Hlavacek-Larrondo, Julie; van Weeren, Reinout; Clarke, Tracy; Intema, Huib; Russell, Helen; Edge, Alastair; Fabian, Andy; Olamaie, Malak; Rumsey, Clare; King, Lindsay; McNamara, Brian; Fecteau-Beaucage, David; Hogan, Michael; Mezcua, Mar; Taylor, Gregory; Blundell, Katherine; Sanders, Jeremy

2018-01-01

Jets created from accretion onto supermassive black holes release relativistic particles on large distances. These strongly affect the intracluster medium when located in the center of a brightest cluster galaxy. The hierarchical merging of subclusters and groups, from which cluster originate, also generates perturbations into the intracluster medium through shocks and turbulence, constituting a potential source of reacceleration for these particles. I will present deep multi-configuration low radio frequency observations from the Karl G. Jansky Very Large Array of two unique clusters, probing the non-thermal emission from the old particle population of the AGN outflows.Recently awarded of 550 hours of Chandra observations, Abell 2146 is one of the rare clusters undergoing a spectacular merger in the plane of the sky. Our recent deep multi-configuration JVLA 1.4 GHz observations have revealed the presence of a structure extending to 850 kpc in size, consisting of one component associated with the upstream shock and classified as a radio relic, and one associated with the subcluster core, consistent with a radio halo bounded by the bow shock. Theses structures have some of the lowest radio powers detected thus far in any cluster. The flux measurements of the halo, its morphology and measurements of the dynamical state of the cluster suggest that the halo was recently created (~ 0.3 Gyr after core passage). This makes A2146 extremely interesting to study, allowing us to probe the complete evolutionary stages of halos.I will also present results on 230-470 MHz JVLA observations of the Perseus cluster. Our observations of this nearby relaxed cool core cluster have revealed a multitude of new structures associated with the mini-halo, extending to hundreds of kpc in size. Its irregular morphology seems to be have been influenced both by the AGN activity and by the sloshing motion of the cluster’ gas. In addition, it has a filamentary structure similar to that seen in

PHYSICAL PROPERTIES AND MORPHOLOGY OF A NEWLY IDENTIFIED COMPACT z = 4.04 LENSED SUBMILLIMETER GALAXY IN ABELL 2218

International Nuclear Information System (INIS)

Knudsen, Kirsten K.; Kneib, Jean-Paul; Richard, Johan; Petitpas, Glen; Egami, Eiichi

2010-01-01

We present the identification of a bright submillimeter (submm) source, SMM J163555.5+661300, detected in the lensing cluster Abell 2218, for which we have accurately determined the position using observations from the Submillimeter Array (SMA). The identified optical counterpart has a spectroscopic redshift of z = 4.044 ± 0.001 if we attribute the single emission line detected at λ = 6140 A to Lyα. This redshift identification is in good agreement with the optical/near-infrared photometric redshift as well as the submm flux ratio S 450 /S 850 ∼ 1.6, the radio-submm flux ratio S 1.4 /S 850 24 /S 850 12 L sun , which implies a star formation rate (SFR) of 230 M sun yr -1 . This makes it the lowest-luminosity submillimeter galaxy (SMG) known at z>4 to date. Previous CO(4-3) emission line observations yielded a non-detection, for which we derived an upper limit of the CO line luminosity of L CO ' = 0.3x10 10 K km s -1 pc -2 , which is not inconsistent with the L ' CO -L FIR relation for starburst galaxies. The best-fit model to the optical and near-infrared photometry give a stellar population with an age of 1.4 Gyr and a stellar mass of 1.6 x 10 10 M sun . The optical morphology is compact and in the source plane the galaxy has an extent of ∼6 x 3 kpc with individual star-forming knots of sun yr -1 kpc 2 . The redshift of J163556 extends the redshift distribution of faint, lensed SMGs, and we find no evidence that these have a different redshift distribution than bright SMGs.

Extracting Galaxy Cluster Gas Inhomogeneity from X-Ray Surface Brightness: A Statistical Approach and Application to Abell 3667

Science.gov (United States)

Kawahara, Hajime; Reese, Erik D.; Kitayama, Tetsu; Sasaki, Shin; Suto, Yasushi

2008-11-01

Our previous analysis indicates that small-scale fluctuations in the intracluster medium (ICM) from cosmological hydrodynamic simulations follow the lognormal probability density function. In order to test the lognormal nature of the ICM directly against X-ray observations of galaxy clusters, we develop a method of extracting statistical information about the three-dimensional properties of the fluctuations from the two-dimensional X-ray surface brightness. We first create a set of synthetic clusters with lognormal fluctuations around their mean profile given by spherical isothermal β-models, later considering polytropic temperature profiles as well. Performing mock observations of these synthetic clusters, we find that the resulting X-ray surface brightness fluctuations also follow the lognormal distribution fairly well. Systematic analysis of the synthetic clusters provides an empirical relation between the three-dimensional density fluctuations and the two-dimensional X-ray surface brightness. We analyze Chandra observations of the galaxy cluster Abell 3667, and find that its X-ray surface brightness fluctuations follow the lognormal distribution. While the lognormal model was originally motivated by cosmological hydrodynamic simulations, this is the first observational confirmation of the lognormal signature in a real cluster. Finally we check the synthetic cluster results against clusters from cosmological hydrodynamic simulations. As a result of the complex structure exhibited by simulated clusters, the empirical relation between the two- and three-dimensional fluctuation properties calibrated with synthetic clusters when applied to simulated clusters shows large scatter. Nevertheless we are able to reproduce the true value of the fluctuation amplitude of simulated clusters within a factor of 2 from their two-dimensional X-ray surface brightness alone. Our current methodology combined with existing observational data is useful in describing and inferring the

Analyse de l'évolution et modélisation des besoins énergétiques français. Application du modèle ABEL à des scénarios contrastés aux horizons 2000 et 2020 Evolutionary Analysis and Modeling of French Energy Needs. Applying the ABEL Model to Contrasting Scenarios for the Horizons 2000 and 2020

Directory of Open Access Journals (Sweden)

Roncato J. P.

2006-11-01

Full Text Available Devant l'enchérissement du pétrole, les pays industrialisés à faibles ressources énergétiques fossiles nationales devront recourir dans le futur à d'autres formes d'énergie (nucléaire, charbon, solaire. La transformation de ces énergies primaires en vecteurs commercialisables est caractérisée par des coûts d'investissement élevés. Cela impose de rechercher le meilleur taux d'utilisation des équipements face à une demande fortement modulée. L'étude de tels systèmes énergétiques procède en deux étapes : analyse des besoins en énergie, puis optimisation des équipements depuis le niveau de production jusqu'à l'utilisation. L'objet de cette communication est de présenter un modèle d'étude de la consommation (ABEL, qui s'appuie sur une analyse du système socio-économique national expliquant la formation et l'évolution des besoins d'énergie. Cette analyse aboutit à la construction de modèles de simulation des consommations d'énergie par secteur. Cette modélisation rend compte des variations saisonnières des besoins. Un modèle macro-économique de cohérence traduit les relations entre niveaux d'activité des différents secteurs, de façon à éviter des distorsions grossières dans une projection à long terme. Des scénarios permettent de simuler diverses hypothèses de développement économique et social. Faced with increasing oil prices, the industrialized countries with smail national fossil energy resources will have to look to other types of energy in the future (nuclear energy, coal, solar energy. The transformation of such primary energy sources into marketable carriers is characterized by high investment costs. This means that the best utilization factor for equipment will have to be sought after in the face of highly modulated demand. A survey of such energy systems is made in two steps: (a analyzing energy needs, and (b optimizing equipment all the way from initial production to end use. The aim of

Frequency of Anaplasma marginale (Theiler 1910 and Babesia sp in mestizo bovine Zebu, in the Municipality of Ixiamas county Abel Iturralde Department of The La Paz, Bolivia

Directory of Open Access Journals (Sweden)

Mercado Alvaro

2011-08-01

Full Text Available The present work one carries out in the Municipality of Ixiamas County Abel Iturralde of the department of Peace-Bolivia, between May and August of 2010. The objective was to determine the presence of Anaplama sp and Babesia sp, through sanguine smear, they took 160 samples of blood, 40 bovine of the four areas they have been evaluated. The results indicate the presence of Anaplasma sp 6,90%, 6,20% in females and 9,70% in males, this represents 2,50% for the area TO, 5,00% area B, 17,50% area C and 2,50% area D. According to the category 12,50% in calves, 0,00% in torillos, 4,80% in bulls, 6,20% in cows and 14,30% in heifers. The presence of Babesia sp 3,13%, with relationship to the sex 3,10% in females and 3,22% in males, being observed 2,50% in the area TO, 5,00% in the area B, 5,00% in the area C and 0,00% in the area D, according to the category 0,00% in calves, torillos 4,80% bulls, 2,73% vacates and 7,14% in heifers.

Physiochemical characteristics, fatty acid profile and tocopherol composition of the oil from Camellia oleifera Abel cultivated in Henan, China

Directory of Open Access Journals (Sweden)

J. B. Hu

2018-06-01

Full Text Available As a unique woody oil tree, Camellia oleifera Abel originates from southern China and is now being cultivated in central China, such as the southern Henan province. The aim of this work is to determine some physiochemical parameters, fatty acid profile and tocopherol composition of the Camellia oleifera seed oils harvested in southern Henan in the 2016 season. The lipid contents of the kernel are in the range of 28.39- 56.94% on dry matter. The acid value (AV, saponification value (SV, iodine value (IV, and refractive index of the oils are in the ranges: 0.22-5.17 mg KOH/g, 178.90-196.91 mg KOH/g, 82.0-87.1 g I2/100g, and 1.4667-1.4720 (nD25 , respectively. The main fatty acids are: palmitic 7.07-9.52%, palmitoleic 0.09-0.22%, stearic 1.45-2.94%, oleic 77.02-84.33%, linoleic 5.19-11.23%, linolenic 0.53-0.70% and arachidic 0.22-0.70%. The sn-2 fatty acid composition is: 84.36-91.33% oleic, 7.14-14.22% linoleic, and 0.89-1.96% others. The tocopherol content is in the range of 39.55-75.94 mg/100g oil, including mainly α-tocopherol (33.98-67.82 mg/100g and γ-tocopherol (5.57- 8.27 mg/100g when the oils are extracted with hexane; and 14.91-44.36 mg/100g, including mainly α-tocopherol (9.42-37.08 mg/100g and γ-tocopherol (5.50-7.33 mg/100g when the oils are extracted by ethyl ether. The physiochemical properties C. oleifera seed oils from southern Henan are similar to those from other districts of China.

UVIT view of ram-pressure stripping in action: Star formation in the stripped gas of the GASP jellyfish galaxy JO201 in Abell 85

Science.gov (United States)

George, K.; Poggianti, B. M.; Gullieuszik, M.; Fasano, G.; Bellhouse, C.; Postma, J.; Moretti, A.; Jaffé, Y.; Vulcani, B.; Bettoni, D.; Fritz, J.; Côté, P.; Ghosh, S. K.; Hutchings, J. B.; Mohan, R.; Sreekumar, P.; Stalin, C. S.; Subramaniam, A.; Tandon, S. N.

2018-06-01

Jellyfish are cluster galaxies that experience strong ram-pressure effects that strip their gas. Their Hα images reveal ionized gas tails up to 100 kpc, which could be hosting ongoing star formation. Here we report the ultraviolet (UV) imaging observation of the jellyfish galaxy JO201 obtained at a spatial resolution ˜ 1.3 kpc. The intense burst of star formation happening in the tentacles is the focus of the present study. JO201 is the "UV-brightest cluster galaxy" in Abell 85 (z ˜ 0.056) with knots and streams of star formation in the ultraviolet. We identify star forming knots both in the stripped gas and in the galaxy disk and compare the UV features with the ones traced by Hα emission. Overall, the two emissions remarkably correlate, both in the main body and along the tentacles. Similarly, also the star formation rates of individual knots derived from the extinction-corrected FUV emission agree with those derived from the Hα emission and range from ˜ 0.01 -to- 2.07 M⊙ yr-1. The integrated star formation rate from FUV flux is ˜ 15 M⊙ yr-1. The unprecedented deep UV imaging study of the jellyfish galaxy JO201 shows clear signs of extraplanar star-formation activity due to a recent/ongoing gas stripping event.

A HIGH FIDELITY SAMPLE OF COLD FRONT CLUSTERS FROM THE CHANDRA ARCHIVE

International Nuclear Information System (INIS)

Owers, Matt S.; Nulsen, Paul E. J.; Markevitch, Maxim; Couch, Warrick J.

2009-01-01

This paper presents a sample of 'cold front' clusters selected from the Chandra archive. The clusters are selected based purely on the existence of surface brightness edges in their Chandra images which are modeled as density jumps. A combination of the derived density and temperature jumps across the fronts is used to select nine robust examples of cold front clusters: 1ES0657 - 558, Abell 1201, Abell 1758N, MS1455.0+2232, Abell 2069, Abell 2142, Abell 2163, RXJ1720.1+2638, and Abell 3667. This sample is the subject of an ongoing study aimed at relating cold fronts to cluster merger activity, and understanding how the merging environment affects the cluster constituents. Here, temperature maps are presented along with the Chandra X-ray images. A dichotomy is found in the sample in that there exists a subsample of cold front clusters which are clearly mergers based on their X-ray morphologies, and a second subsample of clusters which harbor cold fronts, but have surprisingly relaxed X-ray morphologies, and minimal evidence for merger activity at other wavelengths. For this second subsample, the existence of a cold front provides the sole evidence for merger activity at X-ray wavelengths. We discuss how cold fronts can provide additional information which may be used to constrain merger histories, and also the possibility of using cold fronts to distinguish major and minor mergers.

The VLT/MUSE view of the central galaxy in Abell 2052. Ionized gas swept by the expanding radio source

Science.gov (United States)

Balmaverde, Barbara; Capetti, Alessandro; Marconi, Alessandro; Venturi, Giacomo

2018-04-01

We report observations of the radio galaxy 3C 317 (at z = 0.0345) located at the center of the Abell cluster A2052, obtained with the VLT/MUSE integral field spectrograph. The Chandra images of this cluster show cavities in the X-ray emitting gas, which were produced by the expansion of the radio lobes inflated by the active galactic nucleus (AGN). Our exquisite MUSE data show with unprecedented detail the complex network of line emitting filaments enshrouding the northern X-ray cavity. We do not detect any emission lines from the southern cavity, with a luminosity asymmetry between the two regions higher than 75. The emission lines produced by the warm phase of the interstellar medium (WIM) enable us to obtain unique information on the properties of the emitting gas. We find dense gas (up to 270 cm-3) that makes up part of a global quasi spherical outflow that is driven by the radio source, and obtain a direct estimate of the expansion velocity of the cavities (265 km s-1). The emission lines diagnostic rules out ionization from the AGN or from star-forming regions, suggesting instead ionization from slow shocks or from cosmic rays. The striking asymmetric line emission observed between the two cavities contrasts with the less pronounced differences between the north and south sides in the hot gas; this represents a significant new ingredient for our understanding of the process of the exchange of energy between the relativistic plasma and the external medium. We conclude that the expanding radio lobes displace the hot tenuous phase of the interstellar medium (ISM), but also impact the colder and denser ISM phases. These results show the effects of the AGN on its host and the importance of radio mode feedback. The reduced datacube is only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/612/A19

Deep spectroscopy of nearby galaxy clusters - IV. The quench of the star formation in galaxies in the infall region of Abell 85

Science.gov (United States)

Aguerri, J. A. L.; Agulli, I.; Méndez-Abreu, J.

2018-06-01

Our aim is to understand the role of the environment in the quenching of star formation of galaxies located in the infall cluster region of Abell 85 (A85). This is achieved by studying the post-starburst galaxy population as tracer of recent quenching. By measuring the equivalent width (EW) of the [O II] and Hδ spectral lines, we classify the galaxies into three groups: passive (PAS), emission line (EL), and post-starburst (PSB) galaxies. The PSB galaxy population represents ˜ 4.5 per cent of the full sample. Dwarf galaxies (Mr > -18.0) account for ˜ 70 - 80 per cent of PSBs, which indicates that most of the galaxies undergoing recent quenching are low-mass objects. Independently of the environment, PSB galaxies are disc-like objects with g - r colour between the blue ELs and the red PAS ones. The PSB and EL galaxies in low-density environments show similar luminosities and local galaxy densities. The dynamics and local galaxy density of the PSB population in high-density environments are shared with PAS galaxies. However, PSB galaxies inside A85 are at shorter clustercentric radius than PAS and EL ones. The value of the EW(Hδ) is larger for those PSBs closer to the cluster centre. We propose two different physical mechanisms producing PSB galaxies depending on the environment. In low-density environments, gas-rich minor mergers or accretions could produce the PSB galaxies. For high-density environments like A85, PSBs would be produced by the removal of the gas reservoirs of EL galaxies by ram-pressure stripping when they pass near the cluster centre.

Evaluation of Inversion Methods Applied to Ionospheric ro Observations

Science.gov (United States)

Rios Caceres, Arq. Estela Alejandra; Rios, Victor Hugo; Guyot, Elia

The new technique of radio-occultation can be used to study the Earth's ionosphere. The retrieval processes of ionospheric profiling from radio occultation observations usually assume spherical symmetry of electron density distribution at the locality of occultation and use the Abel integral transform to invert the measured total electron content (TEC) values. This pa-per presents a set of ionospheric profiles obtained from SAC-C satellite with the Abel inversion technique. The effects of the ionosphere on the GPS signal during occultation, such as bending and scintillation, are examined. Electron density profiles are obtained using the Abel inversion technique. Ionospheric radio occultations are validated using vertical profiles of electron con-centration from inverted ionograms , obtained from ionosonde sounding in the vicinity of the occultation. Results indicate that the Abel transform works well in the mid-latitudes during the daytime, but is less accurate during the night-time.

Radial dependence of surface streamer-channel luminosity: experimental evidence of Gaussian radiative profiles in Ar and N2

International Nuclear Information System (INIS)

Šimek, M; Ambrico, P F

2012-01-01

Radial distributions of electronically excited species produced during surface streamer propagation were obtained by applying the Abel inverse transform to projected luminosities of single streamers. The streamers were generated in an argon and nitrogen surface coplanar dielectric barrier discharge at atmospheric pressure and their magnified microscopic images were registered with high time resolution. Selected regions of the projected luminosities were processed by the Abel inverse transform procedure based on the Hankel–Fourier method assuming cylindrical symmetry of the streamer channel. Projected as well as Abel-inverted profiles were fitted by Gaussian functions. It is shown that the projected profiles, in addition to the Abel-inverted ones, can be well approximated by the sum of two coaxial Gaussians with two different half-widths and weights. The sharper Gaussian component with higher weight characterizes the radial dependence of the primary cathode-directed streamer-channel luminosity. The second (broader) Gaussian component probably originates either from the pre-breakdown Townsend phase or from the second wave propagating towards the anode. (paper)

Interview with Pierre Deligne

DEFF Research Database (Denmark)

Raussen, Martin; Skau, Christian

2014-01-01

Pierre Deligne is the recipient of the 2013 Abel Prize of the Norwegian Academy of Science and Letters. This interview was conducted in May 2013 in conjunction with the Abel Prize celebration. The article originally appeared in the September 2013 issue of the Newsletter of the European Mathematical...

Weak lensing study of dark matter filaments and application to the binary cluster A 222 and A 223

NARCIS (Netherlands)

Dietrich, JP; Schneider, P; Clowe, D; Romano-Diaz, E; Kerp, J

We present a weak lensing analysis of the double cluster system Abell 222 and Abell 223. The lensing reconstruction shows evidence for a possible dark matter filament connecting both clusters. The case for a filamentary connection between A 222/223 is supported by an analysis of the galaxy density

Abel's legends and first dissemination of the premier mathematical research plan in Chinese journals%《科学世界》首次传入数学家阿贝尔事迹并发表我国第一份数学研究计划

Institute of Scientific and Technical Information of China (English)

亢小玉

2012-01-01

目的 对清光绪二十九年(1903)由上海仪器馆创办的自然科学期刊——《科学世界》所刊载的数学内容作特别梳理.方法 采用原始期刊文献调研和考证.结果 《科学世界》首次在中文期刊媒介上介绍了阿贝尔的传奇人生和近代数学研究分支,相对于当时落后的中国数学现状,为国人传递了国外最新的数学知识.结论 对阿贝尔及其经典代数的传播,反映了中国近代的科学家立足本土科技期刊平台、拉近与世界科技前沿距离的信心,而第一份数学研究计划则是中国近世数学发展史的一份珍贵史料.%Aim The mathematical contents in the nature science journal Science World are unscrambled in this paper, this journal was founded by Shanghai Instrument Museum in Qing Dynasty Guangxu twenty-nine years (1903 ). Methods To investigate and research the original journal references. Results It is Science World that introduced firstly Abel's legendary life and modern math research branch in Chinese journals. For the relatively un-progressive math research in china, it transmitted the newest foreign mathematical knowledge. Conclusion The dissemination of Abel and classical algebra reflects Chinese scientists' confidence to take hold local journals and shorten the distance between the advanced world science and us in modern times, and the publication of the premier mathematical research plan is the valuable material of the development of Chinese modern mathematics.

Health reform and technology--what does it mean for us?

Science.gov (United States)

Abele, J

1995-01-01

John Abele, Founder Chairman of Boston Scientific Corporation, spoke at AAMI's 30th Annual Meeting on 22 May in Anaheim, CA. His speech was part of AAMI's plenary session, "The Impact of a Reformed Health System on New Technology." After his speech, Abele joined three of AAMI's experts in a roundtable discussion on the topics he raised. See the BI&T Forum page 479 for their discussion. As a business entrepreneur and scientist, Abele is well versed in the topic of health reform and scientific advancements. He began his career with a degree in physics and philosophy, then moved into the health care field because of his fascination with medical devices and technologies. He has spent years working as an engineer, a salesperson, a general manager, and a partner in a research and development company. He was a cofounder of AAMI in 1965. Boston Scientific's roots trace back to 1969, when Abele joined with Itzhak Bentov to build a company around a steerable catheter. The associated technology became a platform for many types of tools that could be used as alternatives to surgery in most organs of the body. Today, with over 5,000 employees, 4,000 products, and a worldwide presence, the original objective of developing products and procedures that reduce risk, trauma, cost, and time still applies. Abele is the author of many papers and book chapters, and he has lectured extensively on the technology of various medical devices and technical, social, economic, and political trends affecting health care. His major interests are science education and the process by which new technology is invented, developed, and introduced to society. The following article is based on Abele's presentation.

THE GRISM LENS-AMPLIFIED SURVEY FROM SPACE (GLASS). IV. MASS RECONSTRUCTION OF THE LENSING CLUSTER ABELL 2744 FROM FRONTIER FIELD IMAGING AND GLASS SPECTROSCOPY

Energy Technology Data Exchange (ETDEWEB)

Wang, X.; Schmidt, K. B.; Jones, T. A. [Department of Physics, University of California, Santa Barbara, CA 93106-9530 (United States); Hoag, A.; Huang, K.-H.; Bradac, M. [Department of Physics, University of California, Davis, CA 95616 (United States); Treu, T. [Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095-1547 (United States); Brammer, G. B.; Ryan, R. E. Jr. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD, 21218 (United States); Vulcani, B. [Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study (UTIAS), the University of Tokyo, Kashiwa, 277-8582 (Japan); Amorín, R.; Castellano, M.; Fontana, A.; Merlin, E. [INAF—Osservatorio Astronomico di Roma Via Frascati 33, I-00040 Monte Porzio Catone (Italy); Trenti, M., E-mail: xinwang@physics.ucsb.edu [School of Physics, The University of Melbourne, VIC 3010 (Australia)

2015-09-20

We present a strong and weak lensing reconstruction of the massive cluster Abell 2744, the first cluster for which deep Hubble Frontier Fields (HFF) images and spectroscopy from the Grism Lens-Amplified Survey from Space (GLASS) are available. By performing a targeted search for emission lines in multiply imaged sources using the GLASS spectra, we obtain five high-confidence spectroscopic redshifts and two tentative ones. We confirm one strongly lensed system by detecting the same emission lines in all three multiple images. We also search for additional line emitters blindly and use the full GLASS spectroscopic catalog to test reliability of photometric redshifts for faint line emitters. We see a reasonable agreement between our photometric and spectroscopic redshift measurements, when including nebular emission in photometric redshift estimations. We introduce a stringent procedure to identify only secure multiple image sets based on colors, morphology, and spectroscopy. By combining 7 multiple image systems with secure spectroscopic redshifts (at 5 distinct redshift planes) with 18 multiple image systems with secure photometric redshifts, we reconstruct the gravitational potential of the cluster pixellated on an adaptive grid, using a total of 72 images. The resulting mass map is compared with a stellar mass map obtained from the deep Spitzer Frontier Fields data to study the relative distribution of stars and dark matter in the cluster. We find that the stellar to total mass ratio varies substantially across the cluster field, suggesting that stars do not trace exactly the total mass in this interacting system. The maps of convergence, shear, and magnification are made available in the standard HFF format.

The Grism Lens-amplified Survey from Space (GLASS). IV. Mass Reconstruction of the Lensing Cluster Abell 2744 from Frontier Field Imaging and GLASS Spectroscopy

Science.gov (United States)

Wang, X.; Hoag, A.; Huang, K.-H.; Treu, T.; Bradač, M.; Schmidt, K. B.; Brammer, G. B.; Vulcani, B.; Jones, T. A.; Ryan, R. E., Jr.; Amorín, R.; Castellano, M.; Fontana, A.; Merlin, E.; Trenti, M.

2015-09-01

We present a strong and weak lensing reconstruction of the massive cluster Abell 2744, the first cluster for which deep Hubble Frontier Fields (HFF) images and spectroscopy from the Grism Lens-Amplified Survey from Space (GLASS) are available. By performing a targeted search for emission lines in multiply imaged sources using the GLASS spectra, we obtain five high-confidence spectroscopic redshifts and two tentative ones. We confirm one strongly lensed system by detecting the same emission lines in all three multiple images. We also search for additional line emitters blindly and use the full GLASS spectroscopic catalog to test reliability of photometric redshifts for faint line emitters. We see a reasonable agreement between our photometric and spectroscopic redshift measurements, when including nebular emission in photometric redshift estimations. We introduce a stringent procedure to identify only secure multiple image sets based on colors, morphology, and spectroscopy. By combining 7 multiple image systems with secure spectroscopic redshifts (at 5 distinct redshift planes) with 18 multiple image systems with secure photometric redshifts, we reconstruct the gravitational potential of the cluster pixellated on an adaptive grid, using a total of 72 images. The resulting mass map is compared with a stellar mass map obtained from the deep Spitzer Frontier Fields data to study the relative distribution of stars and dark matter in the cluster. We find that the stellar to total mass ratio varies substantially across the cluster field, suggesting that stars do not trace exactly the total mass in this interacting system. The maps of convergence, shear, and magnification are made available in the standard HFF format.

Journal of Biosciences | Indian Academy of Sciences

Indian Academy of Sciences (India)

Instituto de Biologia Molecular e Celular, Universidade do Porto, Rua do Campo Alegre 823, 4150-180 Porto, Portugal; Instituto de Ciências Biomédicas de Abel Salazar, Universidade do Porto, Largo Prof Abel Salazar 2, 4099-003 Porto, Portugal; Instituto de Patologia e Imunologia Molecular, Universidade do Porto, Rua ...

The ASTRODEEP Frontier Fields catalogues. I. Multiwavelength photometry of Abell-2744 and MACS-J0416

Science.gov (United States)

Merlin, E.; Amorín, R.; Castellano, M.; Fontana, A.; Buitrago, F.; Dunlop, J. S.; Elbaz, D.; Boucaud, A.; Bourne, N.; Boutsia, K.; Brammer, G.; Bruce, V. A.; Capak, P.; Cappelluti, N.; Ciesla, L.; Comastri, A.; Cullen, F.; Derriere, S.; Faber, S. M.; Ferguson, H. C.; Giallongo, E.; Grazian, A.; Lotz, J.; Michałowski, M. J.; Paris, D.; Pentericci, L.; Pilo, S.; Santini, P.; Schreiber, C.; Shu, X.; Wang, T.

2016-05-01

Context. The Frontier Fields survey is a pioneering observational program aimed at collecting photometric data, both from space (Hubble Space Telescope and Spitzer Space Telescope) and from ground-based facilities (VLT Hawk-I), for six deep fields pointing at clusters of galaxies and six nearby deep parallel fields, in a wide range of passbands. The analysis of these data is a natural outcome of the Astrodeep project, an EU collaboration aimed at developing methods and tools for extragalactic photometry and creating valuable public photometric catalogues. Aims: We produce multiwavelength photometric catalogues (from B to 4.5 μm) for the first two of the Frontier Fields, Abell-2744 and MACS-J0416 (plus their parallel fields). Methods: To detect faint sources even in the central regions of the clusters, we develop a robust and repeatable procedure that uses the public codes Galapagos and Galfit to model and remove most of the light contribution from both the brightest cluster members, and the intra-cluster light. We perform the detection on the processed HST H160 image to obtain a pure H-selected sample, which is the primary catalogue that we publish. We also add a sample of sources which are undetected in the H160 image but appear on a stacked infrared image. Photometry on the other HST bands is obtained using SExtractor, again on processed images after the procedure for foreground light removal. Photometry on the Hawk-I and IRAC bands is obtained using our PSF-matching deconfusion code t-phot. A similar procedure, but without the need for the foreground light removal, is adopted for the Parallel fields. Results: The procedure of foreground light subtraction allows for the detection and the photometric measurements of ~2500 sources per field. We deliver and release complete photometric H-detected catalogues, with the addition of the complementary sample of infrared-detected sources. All objects have multiwavelength coverage including B to H HST bands, plus K

The Mathematics of Mikhael Gromov

DEFF Research Database (Denmark)

Hansen, Vagn Lundsgaard

2009-01-01

Laudatio for the Abel Prize winner Mikhael Gromov in Oslo, Norway, March 26, 2009. The lecture is recorded at htttp://media01.smartcom.no/ Microsite/webcast.aspx?eventid=4117......Laudatio for the Abel Prize winner Mikhael Gromov in Oslo, Norway, March 26, 2009. The lecture is recorded at htttp://media01.smartcom.no/ Microsite/webcast.aspx?eventid=4117...

The ASTRODEEP Frontier Fields catalogues. II. Photometric redshifts and rest frame properties in Abell-2744 and MACS-J0416

Science.gov (United States)

Castellano, M.; Amorín, R.; Merlin, E.; Fontana, A.; McLure, R. J.; Mármol-Queraltó, E.; Mortlock, A.; Parsa, S.; Dunlop, J. S.; Elbaz, D.; Balestra, I.; Boucaud, A.; Bourne, N.; Boutsia, K.; Brammer, G.; Bruce, V. A.; Buitrago, F.; Capak, P.; Cappelluti, N.; Ciesla, L.; Comastri, A.; Cullen, F.; Derriere, S.; Faber, S. M.; Giallongo, E.; Grazian, A.; Grillo, C.; Mercurio, A.; Michałowski, M. J.; Nonino, M.; Paris, D.; Pentericci, L.; Pilo, S.; Rosati, P.; Santini, P.; Schreiber, C.; Shu, X.; Wang, T.

2016-05-01

Aims: We present the first public release of photometric redshifts, galaxy rest frame properties and associated magnification values in the cluster and parallel pointings of the first two Frontier Fields, Abell-2744 and MACS-J0416. The released catalogues aim to provide a reference for future investigations of extragalactic populations in these legacy fields: from lensed high-redshift galaxies to cluster members themselves. Methods: We exploit a multiwavelength catalogue, ranging from Hubble Space Telescope (HST) to ground-based K and Spitzer IRAC, which is specifically designed to enable detection and measurement of accurate fluxes in crowded cluster regions. The multiband information is used to derive photometric redshifts and physical properties of sources detected either in the H-band image alone, or from a stack of four WFC3 bands. To minimize systematics, median photometric redshifts are assembled from six different approaches to photo-z estimates. Their reliability is assessed through a comparison with available spectroscopic samples. State-of-the-art lensing models are used to derive magnification values on an object-by-object basis by taking into account sources positions and redshifts. Results: We show that photometric redshifts reach a remarkable ~3-5% accuracy. After accounting for magnification, the H-band number counts are found to be in agreement at bright magnitudes with number counts from the CANDELS fields, while extending the presently available samples to galaxies that, intrinsically, are as faint as H ~ 32-33, thanks to strong gravitational lensing. The Frontier Fields allow the galaxy stellar mass distribution to be probed, depending on magnification, at 0.5-1.5 dex lower masses with respect to extragalactic wide fields, including sources at Mstar ~ 107-108 M⊙ at z > 5. Similarly, they allow the detection of objects with intrinsic star formation rates (SFRs) >1 dex lower than in the CANDELS fields reaching 0.1-1 M⊙/yr at z ~ 6-10. The

Connection between Seyfert galaxies and clusters

International Nuclear Information System (INIS)

Petrosyan, A.R.

1988-01-01

To identify Seyfert galaxies that are members of clusters, the sample of known Seyfert galaxies (464 objects) is tested against the Zwicky, Abell, and southern clusters. On the basis of the criteria adopted in the paper, 67 Seyfert galaxies are selected as probable members of Zwicky clusters, 15 as members of Abell clusters, and 18 as members of southern clusters. Lists of these objects are given

Feasibility of High Energy Lasers for Interdiction Activities

Science.gov (United States)

2017-12-01

NAVAL POSTGRADUATE SCHOOL MONTEREY, CALIFORNIA THESIS FEASIBILITY OF HIGH ENERGY LASERS FOR INTERDICTION ACTIVITIES by Carlos Abel Javier Romero... ENERGY LASERS FOR INTERDICTION ACTIVITIES 5. FUNDING NUMBERS 6. AUTHOR(S) Carlos Abel Javier Romero Chero 7. PERFORMING ORGANIZATION NAME(S) AND...the people or cargo. High Energy Laser (HEL) weapons are an effective way to deliver energy precisely from a relative long range. This thesis studies

Interview with John Milnor

DEFF Research Database (Denmark)

Raussen, Martin; Skau, Christian

2012-01-01

This interview was given by Professor John Milnor in connection to the Abel Prize 2011 ceremony. Originally the interview appeared in the September issue of the Newsletter of the European Mathematical Society......This interview was given by Professor John Milnor in connection to the Abel Prize 2011 ceremony. Originally the interview appeared in the September issue of the Newsletter of the European Mathematical Society...

Interview with Srinivasa Varadhan

DEFF Research Database (Denmark)

Raussen, Martin; Skau, Christian

2008-01-01

S. R. S. Varadhan is the recipient of the 2007 Abel Prize of the Norwegian Academy of Science and Letters. On May 21, 2007, prior to the Abel Prize celebration in Oslo, Varadhan was interviewed by Martin Raussen of Aalborg University and Christian Skau of the Norwegian University of Science...... and Technology. This interview originally appeared in the September 2007 issue of the European Mathematical Society Newsletter....

MUSE sneaks a peek at extreme ram-pressure events. III. Tomography of UGC 6697, a massive galaxy falling into Abell 1367

Science.gov (United States)

Consolandi, G.; Gavazzi, G.; Fossati, M.; Fumagalli, M.; Boselli, A.; Yagi, M.; Yoshida, M.

2017-10-01

We present the MUSE observations of UGC 6697, a giant (M∗ ≈ 1010M⊙) spiral galaxy infalling in the nearby cluster Abell 1367. During its high-velocity transit through the intracluster medium (ICM), the hydrodynamical interactions with the ICM produce a ≈ 100 kpc tail of ionized gas that we map with a mosaic of five MUSE pointings up to 60 kpc from the galaxy. CGCG 97087N, a small companion that lies at few arcminutes in projection from UGC 6697, is also showing signs of the hydrodynamic action of the ICM of the cluster. Along the whole extent of the tail, we detect diffuse Hα emission, and to a lesser extent, Hβ, [OIII]λ5007, and [OI]λ6300. By comparing the kinematics and distribution of gas and stars (as traced by the CaII triplet) for both galaxies, we separate the ionized gas, as traced by the Hα line, into a component that is still bound to the galaxy and a component that is stripped. We find that the bound component shows a low-velocity dispersion and line ratios consistent with photoionization by hot stars. The stripped gas is more turbulent, with velocity dispersions up to ≳100 km s-1, and is excited by shocks, as traced by high values of [OI]/Hα and [NII]/Hα ratio. In the tail of UGC 6697, we identify numerous bright compact knots with line ratios typical of HII regions. These are distributed along the only streams of stripped gas that retain low-velocity dispersions (≲35 km s-1). Despite being in the stripped gas, their physical properties are not different from normal HII regions in galactic disks. We find evidence of a past fast encounter between the two galaxies in the form of a double tail emerging from CGCG 97087N that connects with UGC 6697. This encounter might have increased the efficiency of the stripping process, leaving the stellar distribution and kinematics unaltered. The composite data cube is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http

Review: Petia Genkova & Andrea E. Abele (Eds. (2008. Lernen und Entwicklung im globalen Kontext. "Heimliche Lehrpläne" und Basiskompetenzen [Learning and Development in a Global Context. Hidden Curriculum and Base Competencies

Directory of Open Access Journals (Sweden)

Dörte Bernhard

2011-03-01

Full Text Available This anthology addresses globalization with regard to the world of work. How can women pursue their career and enjoy equal opportunities in the labor market? How can employees be supported during the process of company acquisition? How can the existential crises of young adults that were triggered through institutional work experiences be met and coped with? How can violence among children and adolescents be prevented? Seventeen contributions in Petia GENKOVA's and Andrea E. ABELE's anthology provide answers to these questions. There are four chapters focusing on: 1. female employees and their career, 2. patterns of socialization, 3. self-socialization as a means of gaining basic competencies, and 4. diversity and political culture. A short description of the meaning of a hidden curriculum in times of globalization follows an introduction to the contents of the book and information about the authors. All articles included are then commented upon. It should be noted that the anthology contains a variety of themes and aspects regarding globalization as well as innovative and interactive research methods, although the qualitative methods applied are limited to participative observation and expert interviews. The weakness of the anthology is that due to the complex and abstract linguistic usage, the concepts have not been made sufficiently accessible and straightforward. URN: http://nbn-resolving.de/urn:nbn:de:0114-fqs1102187

Une-Mati lood vene keeles

Index Scriptorium Estoniae

2004-01-01

Dagmar Normeti lasteraamatu "Une-Mati, Päris-Mati ja Tups" tõlget vene keelde (tõlkijad Irina Belobrovtseva ja Vitali Belobrovtsev; ill. Siima Shkop) esitletakse täna Kirjanike Liidu saalis; vt. ka Postimees, 19. märts, lk. 14

The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the intracluster medium out to R200 in Abell 2319

Science.gov (United States)

Ghirardini, V.; Ettori, S.; Eckert, D.; Molendi, S.; Gastaldello, F.; Pointecouteau, E.; Hurier, G.; Bourdin, H.

2018-06-01

Aims: We present the joint analysis of the X-ray and Sunyaev-Zel'dovich (SZ) signals in Abell 2319, the galaxy cluster with the highest signal-to-noise ratio in SZ Planck maps and that has been surveyed within our XMM-Newton Cluster Outskirts Project (X-COP), a very large program which aims to grasp the physical condition in 12 local (z 3 × 1014 M⊙) galaxy clusters out to R200 and beyond. Methods: We recover the profiles of the thermodynamic properties by the geometrical deprojection of the X-ray surface brightness, of the SZ Comptonization parameter, and accurate and robust spectroscopic measurements of the gas temperature out to 3.2 Mpc (1.6 R200), 4 Mpc (2 R200), and 1.6 Mpc (0.8 R200), respectively. We resolve the clumpiness of the gas density to be below 20% over the entire observed volume. We also demonstrate that most of this clumpiness originates from the ongoing merger and can be associated with large-scale inhomogeneities (the "residual" clumpiness). We estimate the total mass through the hydrostatic equilibrium equation. This analysis is done both in azimuthally averaged radial bins and in eight independent angular sectors, enabling us to study in detail the azimuthal variance of the recovered properties. Results: Given the exquisite quality of the X-ray and SZ datasets, their radial extension, and their complementarity, we constrain at R200 the total hydrostatic mass, modelled with a Navarro-Frenk-White profile at very high precision (M200 = 10.7 ± 0.5stat. ± 0.9syst. × 1014 M⊙). We identify the ongoing merger and how it is affecting differently the gas properties in the resolved azimuthal sectors. We have several indications that the merger has injected a high level of non-thermal pressure in this system: the clumping free density profile is above the average profile obtained by stacking Rosat/PSPC observations; the gas mass fraction recovered using our hydrostatic mass profile exceeds the expected cosmic gas fraction beyond R500; the pressure

A fractional derivative approach to full creep regions in salt rock

DEFF Research Database (Denmark)

Zhou, H. W.; Wang, C. P.; Mishnaevsky, Leon

2013-01-01

Based on the definition of the constant-viscosity Abel dashpot, a new creep element, referred to as the variable-viscosity Abel dashpot, is proposed to characterize damage growth in salt rock samples during creep tests. Ultrasonic testing is employed to determine a formula of the variable viscosity...... coefficient, indicating that the change of the variable viscosity coefficient with the time meets a negative exponent law. In addition, by replacing the Newtonian dashpot in the classical Nishihara model with the variable-viscosity Abel dashpot, a damage-mechanism-based creep constitutive model is proposed...... on the basis of time-based fractional derivative. The analytic solution for the fractional-derivative creep constitutive model is presented. The parameters of the fractional derivative creep model are determined by the Levenberg–Marquardt method on the basis of the experimental results of creep tests on salt...

Conditioning bounds for traveltime tomography in layered media

OpenAIRE

Baek, Hyoungsu; Demanet, Laurent

2011-01-01

This paper revisits the problem of recovering a smooth, isotropic, layered wave speed profile from surface traveltime information. While it is classic knowledge that the diving (refracted) rays classically determine the wave speed in a weakly well-posed fashion via the Abel transform, we show in this paper that traveltimes of reflected rays do not contain enough information to recover the medium in a well-posed manner, regardless of the discretization. The counterpart of the Abel transform in...

Mati Hindi juubeliseminer Tallinna Ülikoolis

Index Scriptorium Estoniae

2007-01-01

Täna kell 11 algab Tallinna Ülikoolis seminar, mis on pühendatud keeleteadlase ja Tallinna Ülikooli emeriitprofessori Mati Hindi hiljutisele 70 aasta juubelisünnipäevale, vaadata saab ka Mati Hindi elutööd tutvustavat näitust

Faraday rotation measurements on JET, and the change in the safety factor profile during a sawtooth collapse

International Nuclear Information System (INIS)

O'Rourke, J.; Lazzaro, E.

1990-01-01

Abel-inversion of Faraday rotation measurements on JET has shown that in the current flat-top of sawtoothing discharges the axial safety factor, q o , remains significantly below unity (0.75±0.15) throughout the sawtooth period. In this paper we address two limitations of the Abel-inversion technique, namely the dependence of the results on the assumed flux surface geometry (especially the elongation of the flux surfaces near the magnetic axis, κ o ) and their lack of sensitivity to small changes in the poloidal magnetic field. Assumptions about the flux surface geometry have been verified by comparing Faraday rotation measurements along nearly orthogonal chords, and by a self-consistent identification of the plasma equilibirum. The sensitivity to small changes in the poloidal field, such as those which occur during sawtooth instabilities, has been increased by Abel-inverting the changes in the Faraday rotation signals rather than the signals themselves. (author) 2 refs., 3 figs

Políticas públicas de mejoramiento barrial en los asentamientos informales barrios extensión Abel Amaya y extensión 30 de Octubre de Comodoro Rivadavia: efectos ambientales y comunitarios

Directory of Open Access Journals (Sweden)

Magali Elizabeth Chanampa

2015-04-01

Full Text Available En la ciudad de Comodoro Rivadavia, hace aproximadamente una década, se conformaron en base a diferentes lógicas, asentamientos informales, caracterizados por localizarse en la periferia y a un “costado” de barrios ya constituidos. Esta dimensión de informalidad urbana, les otorgó identidad local, conceptualizándolos en “extensiones” barriales. Estos nuevos espacios barriales, se encuentran determinados, principalmente, por la falta de planificación urbana e infraestructura básica. Las consecuencias de vivir en estas condiciones, crea territorios con problemas ambientales, de hábitat y calidad de vida degradada, conformando un paisaje de segregación urbana ambiental. Este trabajo, se basa en el plan de tesis para el Doctorado en Geografía, el cual, se centra en los barrios informales “Extensión 30 de Octubre” y “Extensión Abel Amaya”, localizados de forma contigua al sudoeste de la ciudad.Estos barrios han experimentado cambios dentro de la lógica de radicación y mejoramiento barrial, a través de políticas públicas de mejoramiento barrial. Estas intervenciones desarrolladas de forma discontinua y circunscrita, en ambos barrios, crea la necesidad de análisis sobre la lógica de intervención de dichos programas y sus posibles efectos, en organizaciones a nivel barrial-comunitario y en nuevas formas de segregación, como la urbana ambiental.

VizieR Online Data Catalog: Strong lensing mass modeling of 4 HFF clusters (Kawamata+, 2016)

Science.gov (United States)

Kawamata, R.; Oguri, M.; Ishigaki, M.; Shimasaku, K.; Ouchi, M.

2018-02-01

We use the public HFF data (http://www.stsci.edu/hst/campaigns/frontier-fields/) for our analysis. The HFF targets six massive clusters, Abell 2744 (z=0.308), MACS J0416.1-2403 (z=0.397), MACS J0717.5+3745 (z=0.545), MACS J1149.6+2223 (z=0.541), Abell S1063 (z=0.348), and Abell 370 (z=0.375), which have been chosen according to their lensing strength and also their accessibility from major ground-based telescopes. The cluster core and parallel field region of each cluster are observed deeply with the IR channel of Wide Field Camera 3 (WFC3/IR) and the Advanced Camera for Surveys (ACS). As of 2015 October, HST observations for the first four clusters, Abell 2744, MACS J0416.1-2403, MACS J0717.5+3745, and MACS J1149.6+2223, are completed. In this study, we use the Version 1.0 data products of drizzled images with a pixel scale of 0.03"/pixel provided by the Space Telescope Science Institute (STScI). The images for each cluster consist of F435W (B435), F606W (V606), and F814W (i814) images from ACS, and F105W (Y105), F125W (J125), F140W (JH140), and F160W (H160) images from WFC3/IR. (7 data files).

The ESO Nearby Abell Cluster Survey. VI. Spatial distribution and kinematics of early- and late-type galaxies

Science.gov (United States)

de Theije, P. A. M.; Katgert, P.

1999-01-01

Analysis of the data obtained in the ESO Nearby Abell Cluster Survey (ENACS) has shown that the space distribution and kinematics of galaxies with detectable emission lines in their spectra differ significantly from those of galaxies without emission lines. This result, and details of the kinematics, were considered as support for the idea that at least the spirals with emission lines are on orbits that are not isotropic. This might indicate that this subset of late-type galaxies either has `first approach'-orbits towards the dense core of their respective clusters, or has orbits that `avoid' the core. The galaxies with emission lines are essentially all late-type galaxies. On the other hand, the emission-line galaxies represent only about a third of the late-type galaxies, the majority of which do not show detectable emission lines. The galaxies without emission lines are therefore a mix of early- and late-type galaxies. In this paper we attempt to separate early- and late-type galaxies, and we study possible differences in distribution and kinematics of the two galaxy classes. For only about 10% of the galaxies in the ENACS, the morphology is known from imaging. Here, we describe our classification on the basis of the ENACS spectrum. The significant information in each spectrum is compressed into 15 Principal Components, which are used as input for an Artificial Neural Network. The latter is `trained' with 150 of the 270 galaxies for which a morphological type is available from Dressler, and subsequently used to classify each galaxy. This yields a classification for two-thirds of the ENACS galaxies. The Artificial Neural Network has two output classes: early-type (E+S0) and late-type (S+I) galaxies. We do not distinguish E and S0 galaxies, because these cannot be separated very robustly on the basis of the spectrum. The success rate of the classification is estimated from the sample of 120 galaxies with Dressler morphologies which were not used to train the ANN

Persistencia del conducto onfalomesenterico. Presentación de un caso

OpenAIRE

Sánchez Portela, Carlos A; Díaz Martínez, Jesús; Ampudia Lizano, Manuel; Sosa Hernández, Roberto; Rodríguez Ramos, William

2005-01-01

Se presentó el caso de un paciente de 42 años de edad, operado en el Hospital General Universitario «Abel Santamaría Cuadrado» de Pinar del Río, que presentaba una fístula entero cutánea, por persistencia del conducto onfalomesentérico. El tratamiento consistió en la resección intestinal y anastomosis terminoterminal. La evolución postoperatoria fue satisfactoria. A 42 year old male patient underwent an operation at "Abel Santamaria" University Hospital, Pinar del Rio. The patient presente...

Towards an understanding of dark matter: Precise gravitational lensing analysis complemented by robust photometric redshifts

Science.gov (United States)

Coe, Daniel Aaron

The goal of thesis is to help scientists resolve one of the great mysteries of our time: the nature of Dark Matter. Dark Matter is currently believed to make up over 80% of the material in our universe, yet we have so far inferred but a few of its basic properties. Here we study the Dark Matter surrounding a galaxy cluster, Abell 1689, via the most direct method currently available--gravitational lensing. Abell 1689 is a "strong" gravitational lens, meaning it produces multiple images of more distant galaxies. The observed positions of these images can be measured very precisely and act as a blueprint allowing us to reconstruct the Dark Matter distribution of the lens. Until now, such mass models of Abell 1689 have reproduced the observed multiple images well but with significant positional offsets. Using a new method we develop here, we obtain a new mass model which perfectly reproduces the observed positions of 168 knots identified within 135 multiple images of 42 galaxies. An important ingredient to our mass model is the accurate measurement of distances to the lensed galaxies via their photometric redshifts. Here we develop tools which improve the accuracy of these measurements based on our study of the Hubble Ultra Deep Field, the only image yet taken to comparable depth as the magnified regions of Abell 1689. We present results both for objects in the Hubble Ultra Deep Field and for galaxies gravitationally lensed by Abell 1689. As part of this thesis, we also provide reviews of Dark Matter and Gravitational Lensing, including a chapter devoted to the mass profiles of Dark Matter halos realized in simulations. The original work presented here was performed primarily by myself under the guidance of Narciso Benítez and Holland Ford as a member of the Advanced Camera for Surveys GTO Science Team at Johns Hopkins University and the Instituto de Astrofisica de Andalucfa. My advisors served on my thesis committee along with Rick White, Gabor Domokos, and Steve

Cette étrange matière

CERN Document Server

Kastler, Alfred

1976-01-01

La matière nous est connue et jusque dans sa structure intime : l'aspect qu'offre le monde industrialisé en est une preuve suffisante, la bombe atomique ou à hydrogène, un signe spectaculaire. Pourtant, selon Alfred Kastler, dont le témoignage en pareil domaine fait naturellement autorité, la matière mérite plus encore d'être appelée "étrange".

Kino-Mati näitab Rakveres kino / Tiit Tuumalu

Index Scriptorium Estoniae

Tuumalu, Tiit, 1971-

2001-01-01

Rakveres tuli lavale Toomas Raudami ja Peeter Simmi näidend Lõuna-Eesti kinomehaaniku Mati Parkja elust "Kino-Mati. Tema elutee ja juhtumised, mis seal ette tulid". Lavastas Peeter Simm, nimiosas Erik Ruus

KONSEPSI DAN APLIKASI PIDANA MATI DALAM PERADILAN DI INDONESIA

Directory of Open Access Journals (Sweden)

I Made Pasek Budiawan

2017-05-01

Full Text Available Imposition of the death penalty by the judge in the criminal justice process Indonesia still remains a debate among groups that agread with the group that oppose it. But in some laws for special crimes such as terrorism, corruption, narcotics, psychotropic substances, and a human rights capital punishment is still regulated, as well as of the criminal code and the concept of the criminal code by 2015 capital punishment is still based. The  existence of the group that did not agree with the conception and application of this dying, argued that human life bussiness, my God, not the man to lift the perspective of the scientific criminal law that a death penalty still exists in all criminal acts by perpetrators of crimes with widespread impact as well as detrimental to the wider community the research for criminal santions was important to examine the existence of the norms of law as a basic for corrector by maximum capital punishment in Indonesia. Penjatuhan pidana mati oleh hakim dalam proses peradilan pidana Indonesia masih tetap menjadi perdebatan antara kelompok yang setuju dengan kelompok yang menentangnya. Namun dalam beberapa undang-undang tindak pidana khusus seperti terorisme, korupsi, narkotika, psikotropika dan peradilan hak asasi manusia pidana mati masih diatur, begitu juga KUHP dan konsep KUHP tahun 2015 pidana mati masih tetap dicanangkan. Adanya kelompok yang tidak setuju dengan konsepsi dan aplikasi pidana  mati ini berdalih bahwa nyawa manusia menjadi urusan Tuhan, bukan menjadi kewenangan manusia untuk mencabutnya. Perspektif keilmuan hukum pidana bahwa pidana mati masih eksis untuk diberlakukan sepanjang tindak pidana yang dilakukan pelaku menyangkut kejahatan luar biasa dengan dampak luas serta merugikan masyarakat luas. Penelitian terhadap sanksi pidana mati penting dilakukan guna meneliti keberadaan norma hukum sebagai dasar pembenar dijatuhkannya pidana mati ini di Indonesia.

Hubble Space Telescope Observations of cD Galaxies and Their Globular Cluster Systems

Science.gov (United States)

Jordán, Andrés; Côté, Patrick; West, Michael J.; Marzke, Ronald O.; Minniti, Dante; Rejkuba, Marina

2004-01-01

We have used WFPC2 on the Hubble Space Telescope (HST) to obtain F450W and F814W images of four cD galaxies (NGC 541 in Abell 194, NGC 2832 in Abell 779, NGC 4839 in Abell 1656, and NGC 7768 in Abell 2666) in the range 5400 km s-1cluster (GC) systems reveals no anomalies in terms of specific frequencies, metallicity gradients, average metallicities, or the metallicity offset between the globular clusters and the host galaxy. We show that the latter offset appears roughly constant at Δ[Fe/H]~0.8 dex for early-type galaxies spanning a luminosity range of roughly 4 orders of magnitude. We combine the globular cluster metallicity distributions with an empirical technique described in a series of earlier papers to investigate the form of the protogalactic mass spectrum in these cD galaxies. We find that the observed GC metallicity distributions are consistent with those expected if cD galaxies form through the cannibalism of numerous galaxies and protogalactic fragments that formed their stars and globular clusters before capture and disruption. However, the properties of their GC systems suggest that dynamical friction is not the primary mechanism by which these galaxies are assembled. We argue that cD's instead form rapidly, via hierarchical merging, prior to cluster virialization. Based on observations with the NASA/ESA Hubble Space Telescope obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555 Based in part on observations obtained at the European Southern Observatory, for VLT program 68.D-0130(A).

Single-molecule dynamics in nanofabricated traps

Science.gov (United States)

Cohen, Adam

2009-03-01

The Anti-Brownian Electrokinetic trap (ABEL trap) provides a means to immobilize a single fluorescent molecule in solution, without surface attachment chemistry. The ABEL trap works by tracking the Brownian motion of a single molecule, and applying feedback electric fields to induce an electrokinetic motion that approximately cancels the Brownian motion. We present a new design for the ABEL trap that allows smaller molecules to be trapped and more information to be extracted from the dynamics of a single molecule than was previously possible. In particular, we present strategies for extracting dynamically fluctuating mobilities and diffusion coefficients, as a means to probe dynamic changes in molecular charge and shape. If one trapped molecule is good, many trapped molecules are better. An array of single molecules in solution, each immobilized without surface attachment chemistry, provides an ideal test-bed for single-molecule analyses of intramolecular dynamics and intermolecular interactions. We present a technology for creating such an array, using a fused silica plate with nanofabricated dimples and a removable cover for sealing single molecules within the dimples. With this device one can watch the shape fluctuations of single molecules of DNA or study cooperative interactions in weakly associating protein complexes.

Bäcklund transformations for the Jacobi system on an ellipsoid

Science.gov (United States)

Tsiganov, A. V.

2017-09-01

We consider analogues of auto- and hetero-Bäcklund transformations for the Jacobi system on a threeaxis ellipsoid. Using the results in a Weierstrass paper, where the change of times reduces integrating the equations of motion to inverting the Abel mapping, we construct the differential Abel equations and auto-Bäcklund transformations preserving the Poisson bracket with respect to which the equations of motion written in the Weierstrass form are Hamiltonian. Transforming this bracket to the canonical form, we can construct a new integrable system on the ellipsoid with a Hamiltonian of the natural form and with a fourth-degree integral of motion in momenta.

Holes in the distribution of rich clusters of galaxies

International Nuclear Information System (INIS)

Burns, J.O.

1988-01-01

The properties of voids in the distribution of Abell clusters of galaxies are described. Cluster voids, such as that in Bootes, serve as markers of large candidate voids of galaxies. The advantages and disadvantages of using rich clusters as tracers of large-scale structures are reviewed. One new 40/h Mpc diameter void of galaxies and clusters in Pisces-Cetus is described in detail. It is found that numerical simulations of models with Gaussian initial conditions do not reproduce the void or filament structures observed within the Abell cluster catalog. The implications of this discrepancy for future observations and models are discussed. 26 references

2001 Chemistry N abel Prize

Indian Academy of Sciences (India)

a biological process, led to his discovery of microbes, his resolu- tion of sodium ... (Nobel Laureates 1975, stereochemistry of enzymatic and or- ganic reactions), C J ... companies nowadays have to make sure that both enantiomers of a drug are ... Generally, chemical synthesis of asymmetric compounds results in racemic ...

Rakvere Teater mängib Kino-Mati lugu / Toomas Suuman

Index Scriptorium Estoniae

Suuman, Toomas

2002-01-01

Näitleja Erik Ruus Toomas Raudami poolt kirjapandud kinomehaanik Mati Parkja töödest-tegemistest jutustavas näidendis "Kino-Mati. Tema elutee ja juhtumised, mis seal ette tulid", lavastaja Peeter Simm

Research and Rhetoric on Teacher Certification

Directory of Open Access Journals (Sweden)

Linda Darling-Hammond

2002-09-01

Full Text Available In October, 2001, the Baltimore-based Abell Foundation issued a report purporting to prove that there is "no credible research that supports the use of teacher certification as a regulatory barrier to teaching" and urging the discontinuation of certification in Maryland. The report argued that large inequities in access to certified teachers for poor and minority students are not a problem because research linking teacher education to student achievement is flawed. In July, 2002, the U.S. Secretary of Education cited the Abell Foundation paper in his Annual Report on Teacher Quality as the sole source for concluding that teacher education does not contribute to teacher effectiveness. The Secretary's report then recommended that requirements for education coursework be eliminated from certification standards, and attendance at schools of education and student teaching be made optional. This article documents the many inaccuracies in the Abell Foundation paper and describes the actual findings of many of the studies it purports to review, as well as the findings of other studies it ignores. It details misrepresentations of a number of studies, including inaccurate statements about their methods and findings, false claims about their authors' views, and distortions of their data and conclusions. The article addresses methodological issues regarding the validity and interpretation of research. Finally, the article presents data challenging the Abell Foundation's unfounded claims that uncertified teachers are as effective as certified teachers, that teacher education makes no difference to teacher effectiveness, that verbal ability is the most important determinant of teaching effectiveness, that private schools staffed by uncertified teachers are more effective than public schools, and that untrained teachers are more qualified than prepared teachers. It concludes with a discussion of the policy issues that need to be addressed if all students are

Kaasaegne memento mori / Annika Toots

Index Scriptorium Estoniae

Toots, Annika

2015-01-01

Hispaania fotokunstnikust Tatiana Abellánist, kelle doktorantuuri uurimisteemaks Murcia ülikoolis oli surma kujutamine ja estetiseerimine kunstis. Tema huvist vanade fotode vastu, seeriast "Fuisteis yo"

TINJAUAN PSIKOLOGIS TERHADAP HUKUMAN MATI

Directory of Open Access Journals (Sweden)

Pujiastuti Handayani

2014-10-01

Full Text Available Abstrak Tindak pidana mutilasi merupakan kejahatan terhadap tubuh dalam bentuk pemotongan bagian-bagian tubuh tertentu dari korban. Persoalan terkait tindak pidana mutilasi yaitu penerapan sanksi pidana terhadap pelaku berupa hukuman mati. Tulisan ini akan menguraikan penerapan hukuman mati terhadap tindak pidana mutilasi yang ditinjau dari perspektif psikologis, hak asasi manusia, maupun agama. Abstract The criminal act of mutilation is a crime against the body in the form of cutting certain body parts of the victim. One of the issues related to mutilation as a crime is the application of death penalty to the perpetrators. This paper describes the application of the death penalty for the perpetrator of the crime of mutilation from a psychological, human rights, and religious perspectives.

Nende kõrgeaususte kirjad on avaldatud : [intervjuu] / Eva Aaver, Heli Laanekask ; üles kirjut. Juhani Püttsepp

Index Scriptorium Estoniae

Aaver, Eva, 1925-2008

1998-01-01

Riigi teaduspreemia humanitaarteaduste vallas said Eva Aaver, Heli Laanekask, Abel Nagelmaa ja Leo Anvelt (postuumselt) publikatsiooni 'Otto Wilhelm Masingu kirjad Johann Heinrich Rosenplänterile. 1814-1832'

Galaxy Clusters in the Swift/BAT era II: 10 more Clusters detected above 15 keV

Energy Technology Data Exchange (ETDEWEB)

Ajello, M.; /SLAC /KIPAC, Menlo Park; Rebusco, P.; /KIPAC, Menlo Park; Cappelluti, N.; /Garching, Max Planck Inst., MPE /Maryland U., Baltimore County; Reimer, O.; /SLAC /Palermo Observ.; Boehringer, H.; /Garching, Max Planck Inst., MPE; La Parola, V.; Cusumano, G.; /Palermo Observ.

2010-10-27

We report on the discovery of 10 additional galaxy clusters detected in the ongoing Swift/BAT all-sky survey. Among the newly BAT-discovered clusters there are: Bullet, Abell 85, Norma, and PKS 0745-19. Norma is the only cluster, among those presented here, which is resolved by BAT. For all the clusters we perform a detailed spectral analysis using XMM-Newton and Swift/BAT data to investigate the presence of a hard (non-thermal) X-ray excess. We find that in most cases the clusters emission in the 0.3-200 keV band can be explained by a multi-temperature thermal model confirming our previous results. For two clusters (Bullet and Abell 3667) we find evidence for the presence of a hard X-ray excess. In the case of the Bullet cluster, our analysis confirms the presence of a non-thermal, power-law like, component with a 20-100 keV flux of 3.4 x 10{sup -12} erg cm{sup -2} s{sup -1} as detected in previous studies. For Abell 3667 the excess emission can be successfully modeled as a hot component (kT = {approx}13 keV). We thus conclude that the hard X-ray emission from galaxy clusters (except the Bullet) has most likely thermal origin.

Computation of Collision-Induced Absorption by Simple Molecular Complexes, for Astrophysical Applications

Science.gov (United States)

Abel, Martin; Frommhold, Lothar; Li, Xiaoping; Hunt, Katharine L. C.

2012-06-01

The interaction-induced absorption by collisional pairs of H{_2} molecules is an important opacity source in the atmospheres of various types of planets and cool stars, such as late stars, low-mass stars, brown dwarfs, cool white dwarf stars, the ambers of the smaller, burnt out main sequence stars, exoplanets, etc., and therefore of special astronomical interest The emission spectra of cool white dwarf stars differ significantly in the infrared from the expected blackbody spectra of their cores, which is largely due to absorption by collisional H{_2}-H{_2}, H{_2}-He, and H{_2}-H complexes in the stellar atmospheres. Using quantum-chemical methods we compute the atmospheric absorption from hundreds to thousands of kelvin. Laboratory measurements of interaction-induced absorption spectra by H{_2} pairs exist only at room temperature and below. We show that our results reproduce these measurements closely, so that our computational data permit reliable modeling of stellar atmosphere opacities even for the higher temperatures. First results for H_2-He complexes have already been applied to astrophysical models have shown great improvements in these models. L. Frommhold, Collision-Induced Absorption in Gases, Cambridge University Press, Cambridge, New York, 1993 and 2006 X. Li, K. L. C. Hunt, F. Wang, M. Abel, and L. Frommhold, Collision-Induced Infrared Absorption by Molecular Hydrogen Pairs at Thousands of Kelvin, Int. J. of Spect., vol. 2010, Article ID 371201, 11 pages, 2010. doi: 10.1155/2010/371201 M. Abel, L. Frommhold, X. Li, and K. L. C. Hunt, Collision-induced absorption by H{_2} pairs: From hundreds to thousands of Kelvin, J. Phys. Chem. A, 115, 6805-6812, 2011} L. Frommhold, M. Abel, F. Wang, M. Gustafsson, X. Li, and K. L. C. Hunt, "Infrared atmospheric emission and absorption by simple molecular complexes, from first principles", Mol. Phys. 108, 2265, 2010 M. Abel, L. Frommhold, X. Li, and K. L. C. Hunt, Infrared absorption by collisional H_2-He complexes

Les paradoxes de la matière

CERN Document Server

2013-01-01

Si nous devons la multitude d’appareils numériques actuels à l’électronique, celle-ci atteint ses limites. Comment les dépasser ? En explorant les propriétés spectaculaires de la matière ! Et les candidats au remplacement de l’électronique sont nombreux : oxytronique, spintronique, plasmonique, magnonique, graphène... Nous réservant aussi bien d’autres surprises - tels les capes d’invisibilité, les plastiques conducteurs, les polymères autocicatrisants, les protections antisismiques, etc - les études sur la matière n’ont pas fini de nous étonner.

Mati Undi teater revisited / Luule Epner

Index Scriptorium Estoniae

Epner, Luule, 1953-

2009-01-01

Teatrilavastuste taastamisest üldisemalt. Pikemalt festivali UNT! programmis etendunud Mati Undi lavastustest "Majahoidja", "Vaimude tund Jannseni tänaval", "Helene, Marion ja Felix", originaali ja taastatud variandi võrdlus

[Mati Erelt. Estonian Language] / Katrin Hiietamm

Index Scriptorium Estoniae

Hiietamm, Katrin

2004-01-01

Arvustus: Estonian language / [Estonian Academy of Sciences] ; edited by Mati Erelt.Tallinn : Teaduste Akadeemia Kirjastus, 2003. 412, [1] lk. : ill., kaart. (Linguistica Uralica. Supplementary series, 0868-4731 ; vol. 1)

Fin de partida de Samuel Beckett: La soberanía del lenguaje y el juego metateatral

Directory of Open Access Journals (Sweden)

Carolina Brncic

2014-05-01

Full Text Available El artículo analiza Fin de partida de Samuel Beckett como obra metateatral. Para abordar el problema del género se examinan cuatro enfoques críticos relevantes: la teoría de Martin Esslin sobre el Teatro del Absurdo, la interpretación de Theodor Adorno como drama de la descomposición, la lectura de Christoph Menke como una tragedia de la representación y la propuesta de Lionel Abel sobre el metateatro. A partir de la definición señalada por Abel, se analiza la obra atendiendo a dos dimensiones paradigmáticas: la noción de juego representacional como drama autorreflexivo y la soberanía del lenguaje como soporte dramático.

Curare Alkaloids: Constituents of a Matis Dart Poison.

Science.gov (United States)

Malca Garcia, Gonzalo R; Hennig, Lothar; Shelukhina, Irina V; Kudryavtsev, Denis S; Bussmann, Rainer W; Tsetlin, Victor I; Giannis, Athanassios

2015-11-25

A phytochemical study of dart and arrow poison from the Matis tribe led to the identification of D-(-)-quinic acid, L-malic acid, ethyldimethylamine, magnoflorine, and five new bisbenzyltetrahydroisoquinoline alkaloids (BBIQAs), 1-5. D-Tubocurarine could not be identified among these products. BBIQA (3) contains a unique linkage at C-8 and C-11'. All structures were characterized by a combination of NMR and HRESIMS data. The effects of Matis poison and individual BBIQAs (1-3) on rat muscle nAChR expressed in Xenopus oocytes have been investigated using the two-electrode voltage clamp technique.

Mati Jostov jättis endast Virumaale sõna "jostovskije" / Tanel Mazur

Index Scriptorium Estoniae

Mazur, Tanel, 1971-

2008-01-01

Vt. ka Põhjarannik : Laupäev ; Severnoje Poberezhje : Subbota, Narva Postiljon 20. sept., lk. 2. Mati Jostovi sõbrad ja töökaaslased andsid Eesti Põlevkivi traagiliselt hukkunud juhi 50. sünniaastapäevaks välja mälestustekogumiku "Mati"

Kuwait summons more fire fighting teams

Energy Technology Data Exchange (ETDEWEB)

1991-08-05

Kuwait is calling in more muscle to help kill its wild wells. This paper reports on the latest action in Kuwait, the leasing of well control contracts to Abel Engineering/Well Control Inc., Houston, and China Petroleum Engineering Construction Co. (CPEC). Abel is the sixth North American well control company called to the scene, while CPEC is the first summoned from the East. In addition, the service responsible for combating well fires and blowouts in the U.S.S.R.'s Azerbaijan oil fields signed an agreement with Kuwait's government, apparently involving a contract valued at more than $100 million, to extinguish fires at 150 Kuwaiti wells, reported Eastern Bloc Energy, a publication of Eastern Bloc Research Ltd., Newton Kyme, U.K. More help likely is on the way.

Joaquín Monegro: el vano intento de liberar una pasión.

Directory of Open Access Journals (Sweden)

José Manuel Torres Torres

2007-01-01

Full Text Available ENGLISH:Freedom topic is examined from attitudes adopted by Joaquín Monegro, a character from Miguel de Unamuno novel Abel Sánchez. Those attitudes are held on throughout the novel plot. This character lives under an existencial anguish sign opprossed by a hateful passion which Joaquín Monegro can only be rid of in his agony and daeth. SPANISH: En el presente estudio se examina el tema de la libertad en la novela Abel Sánchez de Miguel de Unamuno, a partir de las actitudes que adopta en el desarrollo de la historia el personaje Joaquín Monegro, que vive bajo el signo de una angustia existencial, oprimido por una odiosa pasión, posible de liberar recién en su agonía y muerte.

V roce 2013 získal Abelovu cenu Pierre Deligne za fundamentální práce svazující algebru a geometrii

Czech Academy of Sciences Publication Activity Database

Křížek, Michal; Markl, Martin; Somer, L.

2013-01-01

Roč. 58, č. 4 (2013), s. 265-273 ISSN 0032-2423 Institutional support: RVO:67985840 Keywords : Abel prize * algebra and geomtery Subject RIV: BA - General Mathematics http://www.dml.cz/handle/10338.dmlcz/143720

Steps that count! A feasibility study of a pedometer-based, health ...

African Journals Online (AJOL)

a large gap between the development of effective pedometer-based interventions and their ... [13] Using more cost-effective intervention strategies, such as ..... Abel M, Hannon J, Mullineaux D, Beighle A. Determination of step rate thresholds.

Mehelikkuse kriis / Margit Tõnson

Index Scriptorium Estoniae

Tõnson, Margit, 1978-

2009-01-01

Eesti uuemaid lühimängufilme : Sutharsan Bala "Krantsid" (operaator Meelis Veermets, produtsent Marianne Ostrat, osades Jekaterina Novosjolova, Paulo Kulešov ja Mihkel Ulki "Pihv" (stsenarist Triin Sinissaar, osades Mari Abel, Andres Mähar)

Unduski näidend soome keeles

Index Scriptorium Estoniae

2007-01-01

Jaan Unduski näidend "Good-bye, Vienna" tõlgiti soome keelde ja loeti ette festivalil "Baltic Circle". Samal üritusel loeti ette ka lätlase Inga Abele ja leedulase Marius Ivashkevichiuse näidendeid

The National Representation Beauty Contest / Karolina Łabowicz-Dymanus

Index Scriptorium Estoniae

Łabowicz-Dymanus, Karolina

2011-01-01

Näitus "The Art of Estonia - Adapting Modernity / Provocations and Confrontations" Szczecini Rahvusmuuseumis kuni 27.veebr. 2011 ja Varssavi Rahvusmuuseumis kuni 04. juulini 2011. Kumu Kunstimuuseumi korraldatud näituse kuraatorid Tiina Abel ja Eha Komissarov

Mati Muru toetuseks / Ere Raag

Index Scriptorium Estoniae

Raag, Ere

2007-01-01

Maaraamatukogude imago on alati olnud kõrgem raamatukogude üldisest mainest. Vastukaja artiklitele: Einasto, Olga. Mida lugeja tegelikult raamatukogult ootab? // Raamatukogu (2006) nr. 6, lk. 9-14. Petrina, Marlena. Lugeja tehnoloogia varjus // Raamatukogu (2007) nr. 2, lk. 24-27. Muru, Mati. Kes me siis lõppude lõpuks ikka oleme? // Raamatukogu (2007) nr. 4, lk. 36-38

Meeldis. Mõjus. Mis edasi? / Mati Unt

Index Scriptorium Estoniae

Unt, Mati, 1944-2005

2004-01-01

Artiklis räägitakse peamiselt Evald Hermaküla lavastusest "Tuul Olümposelt tuhka tõi" (Eesti Draamateater, 1986), mis pakkus Mati Undile toona viimase aja suurima teatrielamuse, aga ka sellest, et teatrisemiootikud pole senini saavutanud üksmeelt, mis on ikkagi etenduse segment

Eesti Rahvuskultuuri Fond / Raul Pettai

Index Scriptorium Estoniae

Pettai, Raul, 1928-

2009-01-01

allfonde on loodud ka väliseestlaste poolt: Abel-Mirka fond majandusteaduse üliõpilaste koolituse toetamiseks USA-s ja Edmund Valtmani fond Eesti Kunstiakadeemia üliõpilase toetamiseks või akadeemia vilistlasele parima graafilise teose eest

Igavene juuli : näitleja ja lavastaja suvedialoog / Mati Unt ja Andrus Vaarik

Index Scriptorium Estoniae

Unt, Mati, 1944-2005

2004-01-01

Mati Unt ja Andrus Vaariku vestlus näitleja ja lavastaja omavahelisest koostööst. Näitleja kui dirigent Andrus Vaariku arvates. Dialoogi vahel on avaldatud katkendid Elias Canetti "Mass ja võim" ("Masse und Macht") Mati Sirkeli tõlkes

Pan African Medical Journal - Vol 10, No 1 (2011)

African Journals Online (AJOL)

Gervais Ondobo Andze, Abel Namsenmo, Benoit Kebella Illunga, Ditu Kazambu, Dieula Delissaint, Christopher Kuaban, Francois-Xavier Mbopi-Kéou, Wilfred Gabsa, Leopold Mulumba, Jean Pierre ... Raymond Tweheyo, Christine Nalwadda, Nicholas Ayebazibwe, David Mukanga, Elizeus Rutebemberwa, William Bazeyo ...

Soft X-ray Focusing Telescope Aboard AstroSat: Design ...

Indian Academy of Sciences (India)

K. P. Singh

2017-06-19

Jun 19, 2017 ... by the Indian Space Research Organisation (ISRO) on .... paper which will also include a detailed discussion of ..... SXT image of Abell 1795 cluster of galaxies after a slight smoothing using a Gaussian function, sigma = 40.

Untitled

Indian Academy of Sciences (India)

A number of studies have been reported on the wetting ... been used to analyse the experimental results obtained for these materials is identical to that developed for electrical conduction in granular metal films or cermets (Abeles et al. 1976).

Lateral mobility of plasma membrane lipids in Xenopus eggs: Regional differences related to animal/vegetal polarity

NARCIS (Netherlands)

Laat, S.W. de; Bluemink, J.G.; Dictus, W.J.A.G.; Zoelen, E.J.J. van; Tetteroo, P.A.T.; Tertoolen, L.G.J.

1984-01-01

Regional differences in the lateral mobility properties of plasma membrane lipids were studied in unfertilized and fertilized Xenopus eggs by fluorescence photobleaching recovery (FPR) measurements. Out of a variety of commonly used lipid probes only the aminofluorescein- -1abelled fatty

Architects of symmetry in finite nonabelian groups

Czech Academy of Sciences Publication Activity Database

Křížek, Michal; Somer, L.

2010-01-01

Roč. 21, č. 4 (2010), s. 307-319 ISSN 0865-4824 R&D Projects: GA AV ČR(CZ) IAA100190803 Institutional research plan: CEZ:AV0Z10190503 Keywords : Abel Prize * sporadic groups * monster Subject RIV: BA - General Mathematics

Isolation and characterization of an Aux/IAA gene (LaIAA2) from Larix

African Journals Online (AJOL)

微软用户

... an F-box protein, TIR1, which is a component of the SCFTIR1 ubiquitin ligase ... protein-protein interactions (Ulmasov et al., 1997b; Tiwari et al., 2003). In plant .... Statistical analysis .... main classes in the family (Abel and Theologis, 1995;.

Kolm Armastust ja Anarhiat. Nekrofiil, drellimõrvar ja John Woo Tallinnas / Jaan Ruus

Index Scriptorium Estoniae

Ruus, Jaan, 1938-2017

2009-01-01

Helsingi filmifestivali "Armastus ja Anarhia" mitme seansi toimumisest Eestis 1993.a. septembris : Abel Ferrara "Drellimõrvar" ("Driller Killer", 1979), sakslase Jörg Buttgereiti "Nekromantik" (1987) ja "Nekromantik 2" (1991), John Woo "Hard Boiled" (1993). Buttgereit ja Woo olid ka ise kohal

Neoimpressionismi klassikud Kumus / Ragne Nukk

Index Scriptorium Estoniae

Nukk, Ragne, 1984-

2010-01-01

Näitus "Neoimpressionismi jälgedes. Mägi ja Finch" Kumu Kunstimuuseumis 12. septembrini 2010. Kuraator Tiina Abel, kujundaja Inga Heamägi. Eksponeeritakse Soome muuseumide kogudesse kuuluvaid prantsuse maalikunstnike töid ja eesti kunstnike teoseid. Lühidalt neoimpressionismist

El mundo del libro : agosto de 1968

Directory of Open Access Journals (Sweden)

Agustín Rodríguez Garavito

1968-08-01

Full Text Available Se presentan reseñas de los siguientes autores y obras: -Arciniegas, Germán. Isaacs, genio y figura -Naranjo Villegas, Abel. Sociología de la familia -Morales Benítez, Otto. Raíces Humanas.

Mati Hindi põlvkonnapõhine meeleheiteraamat / Urmi Reinde

Index Scriptorium Estoniae

Reinde, Urmi, 1953-

2007-01-01

Mati Hindi raamatu "Minu vaade maale ja merele" Tallinn : TEA, 2007 esitlus toimus 7. juunil Pärnu Uue Kunsti Muuseumis. Mälestusteraamat pojast Madis Hindist (1970-2001) on raamat nelja sugupõlve Hintidest

URGENSI PENYUSUNAN MODEL BIMBINGAN KESEHATAN MENTAL (MENTAL HYGIENE SELAMA MENUNGGU EKSEKUSI MATI

Directory of Open Access Journals (Sweden)

Amir Hasan Ramli, Wiwik Utami

2012-06-01

Full Text Available Penelitian ini bertujuan mendiskripsikan urgensi penyusunan model pembimbingan kesehatan mental terpidana mati.   Penelitian ini merupakan penelitian hukum-empiris dengan pendekatan yuridis-psikologis. Berdasarkan hasil penelitian, materi dan metode pembimbingan kesehatan mental terpidana mati dilakukan berdasarkan interpretasi masing-masing petugas pemasyarakatan, sepanjang tidak melanggar ketentuan hukum yang berlaku.     Hal ini semata-mata dilakukan agar terpidana mati tidak melakukan perbuatan yang melanggar hukum di LAPAS/RUTAN, dan agar lebih siap dalam menghadapi eksekusi mati.   Pembimbing berasal dari dalam maupun luar LAPAS. Prosesnya diintegrasikan melalui kegiatan pembinaan bidang keagamaan dengan metode caramah secara massal dan konsultasi individual. Konseling individual merupakan langkah positif untuk membimbing terpidana mati sesuai dengan kebutuhannya. Sayangnya, pembimbingan tersebut belum didasarkan pada hasil pemeriksanaan psikologis, prosesnya juga belum menggunakan prinsip-prinsip konseling sehingga hasilnya belum optimal. Jika pedoman tersebut ada, petugas pemasyarakatan dapat menyusun langkah-langkah pembimbingan secara sah, efisien dan efektif dalam bimbingan dan konseling, sehingga terpidana mati siap dieksekusi. This research aims at describing the urgence of designing model of sentenced-death prisoner health mental supervision. This research is empiric-law research with psychological- juridical approaches. Based on research result, the supervision is conducted based on the interpretation of each officers as long as it does not violate the rule. The aim of this sort of supervision is that the sentenced-death prisoner does not violate the rule and prepare for the death sentence. Supervisors may come from inside or outside the prison. The process is integrated through religious supervision activity with massive sermon and individual consultation. Individual counceling is a positive step to supervise sentenced

models for prediction of global solar radiation on horizontal surface

African Journals Online (AJOL)

2016-10-12

Oct 12, 2016 ... Ogun State, Nigeria. Abel Giwa Usifo, Department of Physical and Earth Sciences, Crawford University, Igbesa, Ogun State, Nigeria. ... Cubic. The second approach uses two-dimensional. PCA to construct orthogonal-mutually uncorrelated principal components. The method employs centralization of the ...

Hudozhnik i jego dom

Index Scriptorium Estoniae

2004-01-01

Näituse "Kunstnik ja tema kodu. C. T. von Neffi kunstikogu Piira ja Muuga mõisast" raames Väliskunsti Muuseumis toimunud konverentsi "19. sajandi keskpaiga kunstiruum" ettekannetest. Esinesid Jevgenia Kiritshenko, Juri Gudõmenko, Ants Hein, Kadi Polli, Veronika Bogdan, Ingrida Raudsepa, Tiina Abel

Täna toimub Kadrioru lossis väliskunsti muuseumis...

Index Scriptorium Estoniae

2004-01-01

Näituse "Kunstnik ja tema kodu. C. T. von Neffi kunstikogu Piira ja Muuga mõisast" raames toimuva ettekannete päeva "19. sajandi keskpaiga kunstiruum" kava. Esinevad Jevgenia Kiritshenko, Juri Gudõmenko, Ants Hein, Kadi Polli, Veronika Bogdan, Ingrida Raudsepa, Tiina Abel

MIT professor wins major international math prize

CERN Multimedia

Allen, S

2004-01-01

Mathematicians Isadore Singer of MIT and Sir Michael Francis Atiyah of the University of Edinburgh will share an $875,000 award as winners of the second Abel Prize, which some hope will come to be seen as a Nobel Prize for math.

Generalization of boson-fermion equivalence and Fay's addition theorem

International Nuclear Information System (INIS)

Kato, Hideyuki; Saito, Satoru

1989-01-01

Generalizations of Fay's addition theorem for Abel functions are obtained by using generalized boson-fermion equivalence of off-shell string amplitudes. A simple example of such generalizations is presented explicitly which relates derivatives of a Riemann θ-function to its determinant. (orig.)

Veneetsia filmifestival ilmutas auhindu jagades tolerantsi / Margit Tõnson

Index Scriptorium Estoniae

Tõnson, Margit, 1978-

2005-01-01

62. Veneetsia filmifestivali auhinnasaajad. Parima filmi Kuldlõvi sai Ang Lee "Brokebacki mägi", žürii eripreemia Abel Ferrara (artiklis "Ferrera") "Mary", parimaks naisnäitlejaks tituleeriti Giovanna Mezzogiorno, Marcello Mastroianni nimelise noore näitleja preemia sai Menothy Cesar

Kui ma oleksin rahvas... / Jürgen Rooste

Index Scriptorium Estoniae

Rooste, Jürgen, 1979-

2007-01-01

Anders Härmi kuraatorinäitus "Poliitiline/Poeetiline" Tallinna IV graafikatriennaali raames Tallinna Kunstihoones kuni 25. XI. Abel Abidini, Michael Baersi, Johansoni ja Johansoni, Jakob Koldingu, Teemu Mäki, Dan Perjovschi, Hanno Soansi ning Aleksandr Breneri & Barbara Schurzi töödest

Optical identifications of IRAS point sources: the Fornax, Hydra I and Coma clusters

International Nuclear Information System (INIS)

Wang, G.; Leggett, S.K.; Savage, A.

1991-01-01

We present optical identifications for 66 IRAS point sources in the region of the Fornax cluster of galaxies, 106 IRAS point sources in the region of the Hydra I cluster of galaxies (Abell 1060) and 59 IRAS point sources in the region of the Coma cluster of galaxies (Abell 1656). Eight other sources in Hydra I do not have optical counterparts and are very probably due to infrared cirrus. Twenty-three (35 per cent) of the Fornax sources are associated with stars and 43 (65 per cent) with galaxies; 48 (42 per cent) of the Hydra I sources are associated with stars and 58 (51 per cent) with galaxies; 18 (31 per cent) of the Coma sources are associated with stars and 41 (69 per cent) with galaxies. The stellar and infrared cirrus surface density is consistent with the galactic latitude of each field. (author)

Isoperiodic classical systems and their quantum counterparts

International Nuclear Information System (INIS)

Asorey, M.; Carinena, J.F.; Marmo, G.; Perelomov, A.

2007-01-01

One-dimensional isoperiodic classical systems have been first analyzed by Abel. Abel's characterization can be extended for singular potentials and potentials which are not defined on the whole real line. The standard shear equivalence of isoperiodic potentials can also be extended by using reflection and inversion transformations. We provide a full characterization of isoperiodic rational potentials showing that they are connected by translations, reflections or Joukowski transformations. Upon quantization many of these isoperiodic systems fail to exhibit identical quantum energy spectra. This anomaly occurs at order O(h 2 ) because semiclassical corrections of energy levels of order O(h) are identical for all isoperiodic systems. We analyze families of systems where this quantum anomaly occurs and some special systems where the spectral identity is preserved by quantization. Conversely, we point out the existence of isospectral quantum systems which do not correspond to isoperiodic classical systems

IS THE DUST CLOUD AROUND LAMBDA ORIONIS A RING OR A SHELL, OR BOTH?

Energy Technology Data Exchange (ETDEWEB)

Lee, Dukhang; Seon, Kwang-Il; Jo, Young-Soo, E-mail: lee.dukhang@gmail.com [Korea Astronomy and Space Science Institute, Daejeon 305-348 (Korea, Republic of)

2015-06-20

The dust cloud around λ Orionis is observed to be circularly symmetric with a large angular extent (≈8°). However, whether the three-dimensional (3D) structure of the cloud is shell- or ring-like has not yet been fully resolved. We study the 3D structure using a new approach that combines a 3D Monte Carlo radiative transfer model for ultraviolet (UV) scattered light and an inverse Abel transform, which gives a detailed 3D radial density profile from a two-dimensional column density map of a spherically symmetric cloud. By comparing the radiative transfer models for a spherical shell cloud and that for a ring cloud, we find that only the shell model can reproduce the radial profile of the scattered UV light, observed using the S2/68 UV observation, suggesting a dust shell structure. However, the inverse Abel transform applied to the column density data from the Pan-STARRS1 dust reddening map results in negative values at a certain radius range of the density profile, indicating the existence of additional, non-spherical clouds near the nebular boundary. The additional cloud component is assumed to be of toroidal ring shape; we subtracted from the column density to obtain a positive, radial density profile using the inverse Abel transform. The resulting density structure, composed of a toroidal ring and a spherical shell, is also found to give a good fit to the UV scattered light profile. We therefore conclude that the cloud around λ Ori is composed of both ring and shell structures.

Collision-Induced Infrared Absorption by Collisional Complexes in Dense Hydrogen-Helium Gas Mixtures at Thousands of Kelvin

Science.gov (United States)

Abel, Martin; Frommhold, Lothar; Li, Xiaoping; Hunt, Katharine L. C.

2011-06-01

The interaction-induced absorption by collisional pairs of H{_2} molecules is an important opacity source in the atmospheres of the outer planets and cool stars. The emission spectra of cool white dwarf stars differ significantly in the infrared from the expected blackbody spectra of their cores, which is largely due to absorption by collisional H{_2}-H{_2}, H{_2}-He, and H{_2}-H complexes in the stellar atmospheres. Using quantum-chemical methods we compute the atmospheric absorption from hundreds to thousands of kelvin. Laboratory measurements of interaction-induced absorption spectra by H{_2} pairs exist only at room temperature and below. We show that our results reproduce these measurements closely, so that our computational data permit reliable modeling of stellar atmosphere opacities even for the higher temperatures. L. Frommhold, Collision-Induced Absorption in Gases, Cambridge University Press, Cambridge, New York, 1993 and 2006 Xiaoping Li, Katharine L. C. Hunt, Fei Wang, Martin Abel, and Lothar Frommhold, "Collision-Induced Infrared Absorption by Molecular Hydrogen Pairs at Thousands of Kelvin", International Journal of Spectroscopy, vol. 2010, Article ID 371201, 11 pages, 2010. doi: 10.1155/2010/371201 M. Abel, L. Frommhold, X. Li, and K. L. C. Hunt, "Collision-induced absorption by H{_2} pairs: From hundreds to thousands of Kelvin," J. Phys. Chem. A, published online, DOI: 10.1021/jp109441f L. Frommhold, M. Abel, F. Wang, M. Gustafsson, X. Li, and K. L. C. Hunt, "Infrared atmospheric emission and absorption by simple molecular complexes, from first principles", Mol. Phys. 108, 2265, 2010

Kuidas tõlkida Kumu-hoonet kunsti keelde ehk kunstiehitus versus kunst = How to translate the Kumu building into the language of art or artistic architecture versus art / Liina Siib

Index Scriptorium Estoniae

Siib, Liina

2006-01-01

Kumu näitusekujundaja tähelepanekuid maja ja ekspositsiooni vahelistest seostest. Kumu põhiekspositsioonide kujundajad: Liina Siib (Eesti kunst 18. sajandist kuni 1944. aastani, kuraator Tiina Abel) ning Terje Kallast ja Urmas Luure (Eesti kunst 1945-1991, kuraatorid Eha Komissarov ja Kädi Talvoja)

Gericault, Monet ja Dufy Kumus / Harry Liivrand

Index Scriptorium Estoniae

Liivrand, Harry, 1961-

2009-01-01

Prantsusmaalt Lille'i Kunstimuuseumi kogudest pärinev 19. sajandi ja 20. sajandi I poole maastikumaali väljapanek "Normandia maalijad" Kumu Kunstimuuseumis 16. oktoobrist 10. jaanuarini 2010. Näituse koostaja Alain Tapié ja kuraator Tiina Abel. Nimetatud eksponeeritavate tööde autoreid

Analogues of Euler and Poisson Summation Formulae

Indian Academy of Sciences (India)

... f ( n ) have been obtained in a unified manner, where (()) is a periodic complex sequence; () is the divisor function and () is a sufficiently smooth function on [, ]. We also state a generalised Abel's summation formula, generalised Euler's summation formula and Euler's summation formula in several variables.

Book Review COMPOSITE WARFARE: THE CONDUCT OF ...

African Journals Online (AJOL)

COMPOSITE WARFARE: THE CONDUCT OF. SUCCESSFUL GROUND FORCE. OPERATIONS IN AFRICA. Eeben Barlow. Abel Esterhuyse, PhD. Stellenbosch University. Pinetown: 30 Degrees South Publishers. 2015, 576 pages. ISBN 9781928211761. Africa is still one of the most conflict-ridden places on earth – from ...

R-ES-ONAN--CE

Indian Academy of Sciences (India)

in some way lies 'behind' the proof in 1993/4 of FL T by Andrew Wiles: Pythagoras, Euclid,. Archimedes, Diophantus, Fibonacci, Pacioli,. Tartaglia, Cardano, Descartes, Pascal, Fermat. (of course!), Euler, Lagrange, Galois, Abel,. Cauchy, Fourier, Gauss, Dirichlet, Dedekind,. Kummer, Cantor, Riemann, Lobachevsky,. Bolyai ...

Fonoloogiast piiblitõlkeni. Mati Hindi juubelikogumik / Reili Argus

Index Scriptorium Estoniae

Argus, Reili, 1967-

2012-01-01

Tutvustus: Pühendusteos emeriitprofessor Mati Hindi 75. sünnipäevaks / koostanud ja toimetanud Reili Argus, Annika Hussar ja Tiina Rüütmaa. Tallinn : Tallinna Ülikool, 2012. (Tallinna Ülikooli eesti keele ja kultuuri instituudi toimetised ; 14)

STAR TREK elab ja õilmitseb / Scott Abel

Index Scriptorium Estoniae

Abel, Scott

2009-01-01

Artikli autor käis Bonnis "Star Treki" (USA, 1966-1969) fännide iga-aastasel kokkutulekul. Artiklis sellest, kuidas kulttussari on mõjutanud inimesi, kultuuri, meediat. Meenutavad näitleja Nichelle Nichols ja teismelisena sarja looja Gene Roddenberry juures vabatahtliku abilisena töötanud Richard Arnold. Sarja algusest, järgprojektidest ("Star Trek : The Next Generation", "Deep Space Nine" jt.) kuni J. J. Abramsi filmini, mis esilinastus 8. mail

Tagasi looduse ja inimese juurde / Tiina Abel

Index Scriptorium Estoniae

Abel, Tiina, 1951-

2010-01-01

Kunstipoliitika ja ametlik kunst. Heroiline alastuse motiiv. 1937. aasta Pariisi maailmanäitus. Väitlused kunsti rahvuslikkuse ja eesti stiili üle. Kunstikool ja kunstiühing Pallas. Prantsuse orientatsiooni süvenemine. Kaks Prantsuse kunstikultuuri manifestatsiooni

Uus tehnoloogia vajab uut juhtimist / Derek Abell

Index Scriptorium Estoniae

Abell, Derek

2001-01-01

Lausanne'is asuva International Institut for Management Development'i juhtimisprofessor soovitab tippjuhtideks edutada juristide ja turundajate kõrval ka insenere. Tähtsaimad sammud tegevjuhtkonna jaoks

Mati Polli : metsameeste ikoon / Gert D. Hankewitz

Index Scriptorium Estoniae

Hankewitz, Gert D.

2008-01-01

Endise puidutööstuse Sylvester asutaja Mati Polli on metsameeste keskel kujunenud ikooniks ja elavaks legendiks. Vt. samas: Elulugu; Tasub teada; Maksuametil kaotuseid jätkub. Kommenteerivad: ASi Pärnu Mets juhataja Ants Kaljund, ehitusettevõtja Andres Koger, Arengufondi nõukogu esimees Indrek Neivelt ja EMTL juht Andres Talijärv

Proceedings (Mathematical Sciences) SUBJECT INDEX

Indian Academy of Sciences (India)

R. Narasimhan (Krishtel eMaging) 1461 1996 Oct 15 13:05:22

SUBJECT INDEX. Abel's summation formula. Analogues of Euler and Poisson summa- tion formulae. 213 ... theorems of Wiener and Lévy on absolutely convergent Fourier series. 179. Brownian motion. Probabilistic representations of solutions to the heat equation. 321. Cesáro matrix. Necessary and sufficient conditions for.

"Ilutuli" mälestas näitlejat, õnnitles luuletajat, austas kunstnikku / Vaike Rannu ; fotod: Vaike Rannu

Index Scriptorium Estoniae

Rannu, Vaike

2007-01-01

16. veebr. 2007 Tartu College'is toimunud õhtust, mis pühendati näitleja ja deklamaatori Kalle Viirese mälestusele ning samas tähistati ka ajakirjaniku ja luuletaja Eerik Purje 80. sünnipäeva ning tutvuti kunstnik Abel Lee graafikanäitusega

Untitled

African Journals Online (AJOL)

characteristic pattern of developmental function now strongly suggest that defects known as the fetal alcohol maternal alcohol consumption during syndrome (FAS) (Abel, 1982). This pregnancy can affect fetal brain structure syndrome is characterized by specific and function (Clarren et al., 1985). The facial features such as ...

La construction de la matière le modèle Standard

CERN Document Server

Léon, Jacques

2016-01-01

Qu'est-ce que la matière ? Voilà une question à laquelle il pourrait sembler facile de répondre car il n'est rien de plus concret que la matière. Et pourtant, la réponse qu'en donne la physique contemporaine est pour le moins déconcertante ! Le concept-même de particules, briques élémentaires de la matière, s'est volatilisé, dissout dans des objets mathématiques abstraits et abscons pour les non-initiés. Plus nos théories sont précises et plus l'image qu'elles nous renvoient est insaisissable. En un siècle, la représentation des particules s'est métamorphosée en nuages de probabilité portés par des champs quantiques régis par des symétries confinées dans des espaces abstraits. Mais dans un même temps, nous avons réussi le tour de force d'expliquer toute cette complexité avec seulement 16 particules… et une seule théorie, véritable construction de notre conception de la matière : le modèle standard. Ce livre tente de guider le lecteur dans le dédale de la physique des particu...

X-ray lines and self-interacting dark matter.

Science.gov (United States)

Mambrini, Yann; Toma, Takashi

We study the correlation between a monochromatic signal from annihilating dark matter and its self-interacting cross section. We apply our argument to a complex scalar dark sector, where the pseudo-scalar plays the role of a warm dark matter candidate while the scalar mediates its interaction with the Standard Model. We combine the recent observation of the cluster Abell 3827 for self-interacting dark matter and the constraints on the annihilation cross section for monochromatic X-ray lines. We also confront our model to a set of recent experimental analyses and find that such an extension can naturally produce a monochromatic keV signal corresponding to recent observations of Perseus or Andromeda, while in the meantime it predicts a self-interacting cross section of the order of [Formula: see text], as recently claimed in the observation of the cluster Abell 3827. We also propose a way to distinguish such models by future direct detection techniques.

A Moderate Redshift Supernova Search Program

Science.gov (United States)

Adams, M. T.; Wheeler, J. C.; Ward, M.; Wren, W. R.; Schmidt, B. P.

1995-12-01

We report on a recently initiated supernova (SN) search program using the McDonald Observatory 0.76m telescope and Prime Focus Camera (PFC). This SN search program takes advantage of the PFC's 42.6 x 42.6 arcmin FOV to survey moderate redshift Abell clusters in single Kron-Cousins R-band images. Our scientific goal is to discover and provide quality BVRI photometric follow-up, to R \\ +21, for a significant SNe sample at 0.03 group (Perlmutter et al 1995, ApJ, 440, L41), and the High Redshift SN Search Team (Schmidt et al 1995, Aiguiblava NATO ASI Proceedings). The McDonald SN search program includes a sample of the Abell clusters used by Lauer and Postman (1994, ApJ, 425, 418) to analyze Local Group motion. SNe discovered in these clusters contribute to the resolution of the Local Group motion controversy. We present an overview of the McDonald Observatory supernova search program, and discuss recent results.

Pro-Kontra Hukuman Mati (Presepsi Tokoh Agama Islam dan Praktisi Hukum di Kota Palembang

Directory of Open Access Journals (Sweden)

Qodariyah Barkah

2016-03-01

Full Text Available Penelitian ini merupakan hasil penelitian yang membahas tentang pro-kontra hukuman mati, dengan memfokuskan kajian kepada presepsi tokoh agama agama Islam dan praktisi hukum di kota Palembang. Penelitian ini menyimpulkan bahwa Hukuman mati dalam persfektif hukum pidana di Indoneia adalah tertuang dalam Kitab Undang-undang Hukum Pidana (KUHP dan perundang-undangan lainnya yang memuat tentang hukuman mati, antara lain didalam Pasal 10 dan Pasal 11 KUHP. Hukuman pidana mati penerapannya di Indonesia menurut perspektif Tokoh Agama Islam dan praktisi hukum di kota Palembang masih terjadi pro dan kontra. Baik dikalangan praktisi hukum sendiri terjadi pro dan kontra, apakah hukuman pidana mati masih diperlukan penerapannya begitu juga dengan kalangan Tokoh Agama Islam. This article discusses the pros and cons of the death penalty, with a focus on the study of the perception of Islam and religious leaders, legal practitioners in the city of Palembang. This study concluded that the death penalty in criminal law perspective at Indoneia is contained in the Code of Criminal Law (Penal Code and other legislation that contains about the death penalty, among others in Article 10 and Article 11 of the Criminal Code. Penalty death penalty application in Indonesia from the perspective of Islamic religious leaders and legal practitioners in the city of Palembang is still going on pros and cons. Both among legal practitioners itself there are pros and cons, whether the punishment of the death penalty is still necessary application as well as the Islamic Religious Leaders.

La matière noire, clé de l'univers ?

CERN Document Server

Combes, Françoise

2015-01-01

Si ces dernières années de nombreuses découvertes ont permis de mieux connaître notre Univers, 95 % de son contenu, constitué de matière et d énergie noires, nous est encore aujourd hui totalement inconnu. Quelle est la nature de cette matière noire, de ces particules exotiques, sans lesquelles ne pourraient se former les galaxies ? L ouvrage, rédigé par Françoise Combes astrophysicienne dont les travaux de recherche dans ce domaine sont unanimement reconnus fait le point sur l état actuel des connaissances, les découvertes les plus récentes et les prochains défis à relever.

76 FR 16531 - Country of Origin of Textile and Apparel Products; Correction

Science.gov (United States)

2011-03-24

... FURTHER INFORMATION CONTACT: Roberts Abels, Textile Operations, Office of International Trade, (202) 863...: (1) On page 14579, in the first column, remove the word ``Persian'' in the first bullet point and add in its place the word ``Turkish''; (2) On page 14581, in the second column, remove the parenthetical...

Proceedings (Mathematical Sciences) SUBJECT INDEX

Indian Academy of Sciences (India)

Large deviations: An introduction to 2007. Abel prize. 161. Open mapping. Closed graph and open mapping theorems for normed cones. 245. Optimal control. Low-cost control problems on perforated and non-perforated domains. 133. Optimal values. An optimal version of an inequality involv- ing the third symmetric means.

Prospects for SODART observations of nearby clusters of galaxies

DEFF Research Database (Denmark)

Pedersen, Kenneth; Westergaard, Niels Jørgen Stenfeldt

1998-01-01

Using the current best understanding of the SODART mirror system, the Bragg panel and of the LEPC/HEPC responses [1] we have studied the feasibility and prospects for SODART studies of nearby clusters of galaxies. From simulated HEPC data of the cluster Abell 2256, we demonstrate that SODART...

Binarity and the Abundance Discrepancy Problem in Planetary Nebulae

Science.gov (United States)

Corradi, Romano L. M.; García-Rojas, Jorge; Jones, David; Rodríguez-Gil, Pablo

2015-04-01

The discrepancy between abundances computed using optical recombination lines and collisionally excited lines is a major unresolved problem in nebular astrophysics. Here, we show that the largest abundance discrepancies are reached in planetary nebulae with close binary central stars. We illustrate this using deep spectroscopy of three nebulae with a post common-envelope (CE) binary star. Abell 46 and Ou 5 have O2+/H+ abundance discrepancy factors larger than 50, and as high as 300 in the inner regions of Abell 46. Abell 63 has a smaller discrepancy factor around 10, which is still above the typical values in ionized nebulae. Our spectroscopic analysis supports previous conclusions that, in addition to “standard” hot ({{T}e} ˜ 104 K) gas, there exists a colder ({{T}e} ˜ 103 K), ionized component that is highly enriched in heavy elements. These nebulae have low ionized masses, between 10-3 and 10-1 M⊙ depending on the adopted electron densities and temperatures. Since the much more massive red giant envelope is expected to be entirely ejected in the CE phase, the currently observed nebulae would be produced much later, during post-CE mass loss episodes when the envelope has already dispersed. These observations add constraints to the abundance discrepancy problem. We revise possible explanations. Some explanations are naturally linked to binarity such as, for instance, high-metallicity nova ejecta, but it is difficult at this stage to depict an evolutionary scenario consistent with all of the observed properties. We also introduce the hypothesis that these nebulae are the result of tidal destruction, accretion, and ejection of Jupiter-like planets.

The Frontier Fields: Survey Design and Initial Results

Energy Technology Data Exchange (ETDEWEB)

Lotz, J. M.; Koekemoer, A.; Grogin, N.; Mack, J.; Anderson, J.; Avila, R.; Barker, E. A.; Borncamp, D.; Durbin, M.; Gunning, H.; Hilbert, B.; Jenkner, H.; Khandrika, H.; Levay, Z.; Lucas, R. A.; MacKenty, J.; Ogaz, S. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Coe, D.; Capak, P.; Brammer, G., E-mail: lotz@stsci.edu [European Space Agency/Space Telescope Science Institute, 3700 Sam Martin Drive, Baltimore, MD 21218 (United States); and others

2017-03-01

What are the faintest distant galaxies we can see with the Hubble Space Telescope ( HST ) now, before the launch of the James Webb Space Telescope ? This is the challenge taken up by the Frontier Fields, a Director’s discretionary time campaign with HST and the Spitzer Space Telescope to see deeper into the universe than ever before. The Frontier Fields combines the power of HST and Spitzer with the natural gravitational telescopes of massive high-magnification clusters of galaxies to produce the deepest observations of clusters and their lensed galaxies ever obtained. Six clusters—Abell 2744, MACSJ0416.1-2403, MACSJ0717.5+3745, MACSJ1149.5+2223, Abell S1063, and Abell 370—have been targeted by the HST ACS/WFC and WFC3/IR cameras with coordinated parallel fields for over 840 HST orbits. The parallel fields are the second-deepest observations thus far by HST with 5 σ point-source depths of ∼29th ABmag. Galaxies behind the clusters experience typical magnification factors of a few, with small regions magnified by factors of 10–100. Therefore, the Frontier Field cluster HST images achieve intrinsic depths of ∼30–33 mag over very small volumes. Spitzer has obtained over 1000 hr of Director’s discretionary imaging of the Frontier Field cluster and parallels in IRAC 3.6 and 4.5 μ m bands to 5 σ point-source depths of ∼26.5, 26.0 ABmag. We demonstrate the exceptional sensitivity of the HST Frontier Field images to faint high-redshift galaxies, and review the initial results related to the primary science goals.

The first high resolution image of coronal gas in a starbursting cool core cluster

Science.gov (United States)

Johnson, Sean

2017-08-01

Galaxy clusters represent a unique laboratory for directly observing gas cooling and feedback due to their high masses and correspondingly high gas densities and temperatures. Cooling of X-ray gas observed in 1/3 of clusters, known as cool-core clusters, should fuel star formation at prodigious rates, but such high levels of star formation are rarely observed. Feedback from active galactic nuclei (AGN) is a leading explanation for the lack of star formation in most cool clusters, and AGN power is sufficient to offset gas cooling on average. Nevertheless, some cool core clusters exhibit massive starbursts indicating that our understanding of cooling and feedback is incomplete. Observations of 10^5 K coronal gas in cool core clusters through OVI emission offers a sensitive means of testing our understanding of cooling and feedback because OVI emission is a dominant coolant and sensitive tracer of shocked gas. Recently, Hayes et al. 2016 demonstrated that synthetic narrow-band imaging of OVI emission is possible through subtraction of long-pass filters with the ACS+SBC for targets at z=0.23-0.29. Here, we propose to use this exciting new technique to directly image coronal OVI emitting gas at high resolution in Abell 1835, a prototypical starbursting cool-core cluster at z=0.252. Abell 1835 hosts a strong cooling core, massive starburst, radio AGN, and at z=0.252, it offers a unique opportunity to directly image OVI at hi-res in the UV with ACS+SBC. With just 15 orbits of ACS+SBC imaging, the proposed observations will complete the existing rich multi-wavelength dataset available for Abell 1835 to provide new insights into cooling and feedback in clusters.

Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel'dovich measurements

Science.gov (United States)

Tchernin, C.; Bartelmann, M.; Huber, K.; Dekel, A.; Hurier, G.; Majer, C. L.; Meyer, S.; Zinger, E.; Eckert, D.; Meneghetti, M.; Merten, J.

2018-06-01

Context. The mass of galaxy clusters is not a direct observable, nonetheless it is commonly used to probe cosmological models. Based on the combination of all main cluster observables, that is, the X-ray emission, the thermal Sunyaev-Zel'dovich (SZ) signal, the velocity dispersion of the cluster galaxies, and gravitational lensing, the gravitational potential of galaxy clusters can be jointly reconstructed. Aims: We derive the two main ingredients required for this joint reconstruction: the potentials individually reconstructed from the observables and their covariance matrices, which act as a weight in the joint reconstruction. We show here the method to derive these quantities. The result of the joint reconstruction applied to a real cluster will be discussed in a forthcoming paper. Methods: We apply the Richardson-Lucy deprojection algorithm to data on a two-dimensional (2D) grid. We first test the 2D deprojection algorithm on a β-profile. Assuming hydrostatic equilibrium, we further reconstruct the gravitational potential of a simulated galaxy cluster based on synthetic SZ and X-ray data. We then reconstruct the projected gravitational potential of the massive and dynamically active cluster Abell 2142, based on the X-ray observations collected with XMM-Newton and the SZ observations from the Planck satellite. Finally, we compute the covariance matrix of the projected reconstructed potential of the cluster Abell 2142 based on the X-ray measurements collected with XMM-Newton. Results: The gravitational potentials of the simulated cluster recovered from synthetic X-ray and SZ data are consistent, even though the potential reconstructed from X-rays shows larger deviations from the true potential. Regarding Abell 2142, the projected gravitational cluster potentials recovered from SZ and X-ray data reproduce well the projected potential inferred from gravitational-lensing observations. We also observe that the covariance matrix of the potential for Abell 2142

Armastus ja anarhia / J[aan] R[uus

Index Scriptorium Estoniae

J. R.

1993-01-01

Helsingi filmifestivali "Armastus ja anarhia" mängufilmid "Nekromantik I" (1987) ja "Nekromantik II" (1991), režissöör Jörg Buttgereit ja "Trellimõrtsukas" (1979), režissöör Abel Ferrara, Tallinna kinos "Eha". Arvustavad Rainer Sarnet, Jaak Kilmi, Marko Raat ja J. R. (Jaan Ruus)

African American Men, Identity, and Participation in Adult Basic Education and Literacy Programs. Research Brief #6

Science.gov (United States)

Drayton, Brendaly; Prins, Esther

2011-01-01

Although the national graduation rate for African American males is only 47% (Schott Foundation for Public Education, 2010), few studies have explored their experiences in adult basic and literacy education (ABEL) programs. This study draws on prior research to explore the relationship between literacy and identity and its potential for…

Interaction of the WAT Source in A3395 with the Intracluster Medium

Indian Academy of Sciences (India)

2016-01-27

Jan 27, 2016 ... Using X-ray observations from Chandra and XMM-Newton and radio observations from the Australia Telescope Compact Array (ATCA), we have examined the merging environment of the bimodal cluster Abell 3395. From X-ray data we have produced thermodynamic maps of the cluster. The Wide Angle ...

Deep multi-frequency rotation measure tomography of the galaxy cluster A2255

NARCIS (Netherlands)

Pizzo, R. F.; de Bruyn, A. G.; Bernardi, G.; Brentjens, M. A.

Aims. By studying the polarimetric properties of the radio galaxies and the radio filaments belonging to the galaxy cluster Abell 2255, we aim to unveil their 3-dimensional location within the cluster. Methods. We performed WSRT observations of A2255 at 18, 21, 25, 85, and 200 cm. The polarization

Incorrigible advocates

NARCIS (Netherlands)

Doornbos, N.; de Groot-van Leeuwen, L.E.

2012-01-01

Inspired by the work of Richard Abel, the authors conduct a N=1 study into the career path and disciplinary records of a Dutch immigration advocate. Their aim is to offer explanations as to why some lawyers seem so impervious to discipline. The authors analyse the case from three different angles:

Understanding Cultural Differences in the Antecedents of Pro-Environmental Behavior: A Comparative Analysis of Business Students in the United States and Chile

Science.gov (United States)

Cordano, Mark; Welcomer, Stephanie; Scherer, Robert; Pradenas, Lorena; Parada, Victor

2010-01-01

We surveyed business students in the U. S. (n = 256) and Chile (n = 310). The survey included measures drawn from studies of pro-environmental behavior using Schwartz's norm activation theory (Schwartz, 1977), the theory of reasoned action (Ajzen & Fishbein, 1980), and a values-beliefs-norms model created by Stern, Dietz, Abel, Guagnano, and…

A Cross-Cultural Assessment of Three Theories of Pro-Environmental Behavior: A Comparison between Business Students of Chile and the United States

Science.gov (United States)

Cordano, Mark; Welcomer, Stephanie; Scherer, Robert F.; Pradenas, Lorena; Parada, Victor

2011-01-01

We surveyed business students in the United States (n = 256) and Chile (n = 310) to compare three theories of pro-environmental behavior.We examined Ajzen and Fishbein's theory of reasoned action, Schawartz's norm activation theory, and the values-beliefs-norms theory created by Stern, Dietz, Abel, Guagnano, and Kalof. We produced reliable…

The Olympic Games: Showcases of Internationalism and Modernity in Asia

Directory of Open Access Journals (Sweden)

Robin Kietlinski

2017-09-01

Full Text Available Stefan Huebner. Pan-Asian Sports and the Emergence of Modern Asia, 1913-1974. Singapore: National University of Singapore Press, 2016. 416 pp. $42 (paper. Jessamyn Abel. The International Minimum: Creativity and Contradiction in Japan's Global Engagement, 1933-1964. Honolulu: University of Hawai‘i Press, 2015. 344 pp. $54 (cloth.

3-D modelling of a bilayer heterojunction organic solar cell based on ...

African Journals Online (AJOL)

The thin film multilayer stacking theory is applied to the bilayer heterojunction organic solar cell, with the optical matrix of the Abeles theory leading to new expression of generation rate and density of exciton photogenerated in the organic photoactive layer of CuPc/C60. The excitons density is investigated considering the ...

Proceedings – Mathematical Sciences | Indian Academy of Sciences

Indian Academy of Sciences (India)

Home; Journals; Proceedings – Mathematical Sciences; Volume 118; Issue 2. Issue front cover thumbnail. Volume 118, Issue 2. May 2008, pages 159-320. pp 159-160. Note on Plagiarism · Gadadhar Misra N Mukunda · More Details Fulltext PDF. pp 161-182 Invited Article. Large Deviations: An Introduction to 2007 Abel ...

Examining EXPRESS with Simulation

Science.gov (United States)

2012-03-01

warfighter communities. iv AFIT-OR-MS-ENS-12-27 The God of the universe presents marvelous fingerprints of his glory throughout creation ( Isaiah 6:3...Redistribution Decision Support”, Air Force Journal of Logistics, 21(3):14–20, 25, 1997. [23] Cohen, Irv K., J. Abell, and Thomas F. Lippiatt. Coupling Logistics

Gaussian curvature on hyperelliptic Riemann surfaces

Indian Academy of Sciences (India)

Indian Acad. Sci. (Math. Sci.) Vol. 124, No. 2, May 2014, pp. 155–167. c Indian Academy of Sciences. Gaussian curvature on hyperelliptic Riemann surfaces. ABEL CASTORENA. Centro de Ciencias Matemáticas (Universidad Nacional Autónoma de México,. Campus Morelia) Apdo. Postal 61-3 Xangari, C.P. 58089 Morelia,.

The Intelligence Revolution: A Historical Perspective

Science.gov (United States)

1988-10-01

1979), is a useful survey. 7. Cf. Zara Steiner , The Foreign Office and Foreign Policy, 1898-1914 (Cambridge, 1969); and Lamar F. Cecil, The German...falsifying two identity of these people. You may recall that Rudolf Abel was arrested in New York in the 1950s. He was later exchanged, I believe, for

Perspectives on Early Childhood Education in Egypt and Kuwait.

Science.gov (United States)

El-Beblawi, Viola F.

Early childhood education is rooted in the Arab culture. Of particular importance for the implementation of early childhood education is the academic psycho-educational movement in the Arab world (initiated by Tsmail El Kabani and Dr. Abel Aziz El Koussy), which began in the 1920s. This movement, combined with rapid social change (including the…

Is the Age Problem Resolved? Ali Akbar Navabi & Nematollah Riazi

Indian Academy of Sciences (India)

R. Narasimhan (Krishtel eMaging) 1461 1996 Oct 15 13:05:22

uncertainties are comparatively studied in the present paper. We are ... the recent estimates of the age of globular clusters have led to the gradual ... Three main streams of research seem to have converged to consistent estimates of the ... ters on the basis of a wide set of observational data including the Abell-ACO cluster.

The HST/ACS Coma Cluster Survey : II. Data Description and Source Catalogs

NARCIS (Netherlands)

Hammer, Derek; Kleijn, Gijs Verdoes; Hoyos, Carlos; den Brok, Mark; Balcells, Marc; Ferguson, Henry C.; Goudfrooij, Paul; Carter, David; Guzman, Rafael; Peletier, Reynier F.; Smith, Russell J.; Graham, Alister W.; Trentham, Neil; Peng, Eric; Puzia, Thomas H.; Lucey, John R.; Jogee, Shardha; Aguerri, Alfonso L.; Batcheldor, Dan; Bridges, Terry J.; Chiboucas, Kristin; Davies, Jonathan I.; del Burgo, Carlos; Erwin, Peter; Hornschemeier, Ann; Hudson, Michael J.; Huxor, Avon; Jenkins, Leigh; Karick, Arna; Khosroshahi, Habib; Kourkchi, Ehsan; Komiyama, Yutaka; Lotz, Jennifer; Marzke, Ronald O.; Marinova, Irina; Matkovic, Ana; Merritt, David; Miller, Bryan W.; Miller, Neal A.; Mobasher, Bahram; Mouhcine, Mustapha; Okamura, Sadanori; Percival, Sue; Phillipps, Steven; Poggianti, Bianca M.; Price, James; Sharples, Ray M.; Tully, R. Brent; Valentijn, Edwin

The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imaging in the F475W and F814W passbands. Although our survey was interrupted by the ACS instrument failure in early 2007, the partially completed survey still covers ~50% of the core high-density region in

The Use of Lego Technologies in Elementary Teacher Preparation

NARCIS (Netherlands)

Hadjiachilleos, Stella; Avraamidou, Lucy; Papastavrou, Stavros

2013-01-01

The need to reform science teacher preparation programs has been pointed out in research (Bryan and Abell in J Res Sci Teach 36:121-140, 1999; Bryan and Atwater in Sci Educ 8(6):821-839, 2002; Harrington and Hathaway in J Teach Educ 46(4):275-284, 1995). Science teachers are charged with the

Status Pencemaran Lingkungan Sungai Badung dan Sungai Mati di Provinsi Bali Berdasarkan Bioindikator Phylum Annelida

Directory of Open Access Journals (Sweden)

Mawardi Labbaik

2017-11-01

Full Text Available Water pollution is the entry or inclusion of substances, energy and other components into the water by human activities, so that water quality decrease to a certain level. This study a timed to monitor the pollution of aquatic environment in the Badung River and Mati River by using Annelida phylum as bioindicator, the study was conducted from February to March 2017. The data obtained were analyzed by the structure of the community, and also used ABC (Abudance-Biomass Comparison method. The result of the research showed that the most abundance of Annelida and dominant from all stations of Badung River and Mati River was Lumbriculus variegatus. Is showed that it contamination status was categorized as mild contamination because it was dominant by facultative organism. The structure of the Annelida community in the Badung River and Mati River with the value of the diversity index was categorized as low Annelida (H '<1.0. The uniformity index was categorized as depressed Annelida community (0.00 Mati River was medium (0.50 < C < 0.75. The result of the water quality range as the supporting factor showed the average support for Annelida life i.e the current velocity 0.16 - 0.61 m/s, the temperature 25.5 - 31oC, DO 3-7.2 mg/l, pH 7.77 - 8.44 and BOD5 0.5 - 3.1 mg/l. The analysis environmental pollution condition of Badung River and Mati River with Annelida as bioindicator by using ABC method showed that were medium contaminated.

Itaalia kunstipärandinäitus Eestis

Index Scriptorium Estoniae

2004-01-01

21. IV-23. V Eesti Kunstimuuseumi Rüütelkonna hoones näitus "Itaalia majoolika kuldajastud. Meistriteoseid Rooma Riiklikust Antiikkunsti Galeriist". Näitusele esitatud majoolikanõud ja keraamilised plaadid on valminud XIII-XIX sajandil. Kuraator Marisa Zaccagnini, näituse ettevalmistamist EKM-s kureeris Tiina Abel. 8. ja 15. V tutvustab Inge Teder majoolikat, selle dekoori ja koolkondi

Modernismi ja rahvusluse vahel / Juta Kivimäe

Index Scriptorium Estoniae

Kivimäe, Juta, 1952-

1998-01-01

Kolme Balti riigi maailmasõdadevahelist kunstiajalugu käsitlev konverents "Modernity and Identity : Art 1918-1939" 22.-23. okt. Kaunases M. K. Chiurlionise kunstimuuseumis. Esinesid Jolita Muleviciute, Pille Väljataga, Eduards Klavinsh, Osvaldas Daugelis, Tiina Abel, Juta Kivimäe, Anne Lõugas, Sergei Fauchereau (möödunudkevadisest suurnäitusest 1930ndate Euroopa kunstist Pariisi Linna Kunstimuuseumis)

The Use of Lego Technologies in Elementary Teacher Preparation

Science.gov (United States)

Hadjiachilleos, Stella; Avraamidou, Lucy; Papastavrou, Stavros

2013-01-01

The need to reform science teacher preparation programs has been pointed out in research (Bryan and Abell in "J Res Sci Teach" 36:121-140, 1999; Bryan and Atwater in "Sci Educ" 8(6):821-839, 2002; Harrington and Hathaway in "J Teach Educ" 46(4):275-284, 1995). Science teachers are charged with the responsibility of…

Journal of Astrophysics and Astronomy | Indian Academy of Sciences

Indian Academy of Sciences (India)

2016-01-27

Jan 27, 2016 ... We present a statistical analysis of the rotation measure (RM) catalogue from the NVSS in search for a statistical excess of rotation measure through Abell clusters. After excluding the data known to be affected by the large-scale magnetic field of the Galaxy ( ≤ |30|), we consider RMs as a function of ...

The Intelligence Revolution: A Historical Perspective: Proceedings of the Military History Symposium (13th) Held in Colorado Springs, Colorado on 12-14 October 1988

Science.gov (United States)

1991-01-01

Diplomacy (Cambridge, Mass., 1970). 6. E. A. Whitcomb, Napoleon’s Diplomatic Service (Durham, N.C., 1979), is a useful survey. 7. Cf. Zara Steiner , The...And this goes so far as falsifying two identity of the ,e people. You may recall that Rudolf Abel was arrested in New York in the 1950s. He was later

Abel-grassmann's groupoids of modulo matrices

International Nuclear Information System (INIS)

Javaid, Q.; Awan, M.D.; Naqvi, S.H.A.

2016-01-01

The binary operation of usual addition is associative in all matrices over R. However, a binary operation of addition in matrices over Z/sub n/ of a nonassociative structures of AG-groupoids and AG-groups are defined and investigated here. It is shown that both these structures exist for every integer n >≥ 3. Various properties of these structures are explored like: (i) Every AG-groupoid of matrices over Z/sub n/ is transitively commutative AG-groupoid and is a cancellative AG-groupoid if n is prime. (ii) Every AG-groupoid of matrices over Z/sub n/ of Type-II is a T/sup 3/-AG-groupoid. (iii) An AG-groupoid of matrices over Z/sub n/ ; G /sub nAG/(t,u), is an AG-band, if t+u=1(mod n). (author)

Vtoroi plan vremeni / Tiina Abel ; interv. Nikolai Hrustaljov

Index Scriptorium Estoniae

Abel, Tiina, 1951-

2007-01-01

Näituse "Metafoor ja müüt. Kirjanduslikud ja ajaloolised motiivid 19. ja 20. sajandi vahetuse Poola kunstis" Kumu kunstimuuseumi kuraatori Tiina Abeliga näituse ettevalmistustööst, poola maalikunstist 19. sajandil, töödest näitusel

Mati Vanni firma Neoqi paneb USAs saunad püsti

Index Scriptorium Estoniae

2009-01-01

Ärimees Mati Vanni firma Neoqi saunakomplekse Cube paigaldatakse tänavu mitmesse USA firma KWC America salongi, seni on Neoqi lõõgastusseadmeid müüdud rohkem kui 50 riiki. USA firma Sybaritic hagist Neoqi vastu ja Neoqi avaldusest Sybariticu tegevuse kohta, saavutatud leppest

114-----------------------------~---------RE-SO-NANCEIDe-ce-mb-er

Indian Academy of Sciences (India)

Abel (7) 28 (GA). Adams J F (2) 8 (SA). Ageing (8) 67 (RN). Age-specific mortality rate (8) 67 (RN). Albert Einstein - The man behind the myths by. John Stachel (8) 76 (RF). Algebra (1) 8 (SA). Algebra in ancient and modern times by. V S Varadarajan (6) 80 (BR). Algebraic integers (7) 28 (GA). Algebraic number theory (7) 28 ...

PROBLEMATIKA PENERAPAN PIDANA MATI DALAM KONTEKS PENEGAKAN HUKUM DI INDONESIA

Directory of Open Access Journals (Sweden)

Slamet Tri Wahyudi

2012-07-01

Full Text Available Penegakan hukum yang tanpa arah dan tidak didasarkan pada tiga pilar hukum yakni keadilan, kepastian hukum dan kemanfaatan bagi masyarakat dapat melanggar hukum bahkan pula melanggar hak asasi manusia. Adapun salah satu kebijakan dari Pemerintah yang dianggap tidak mencerminkan nilai-nilai keadilan dan meresahkan bagi masyarakat, yakni kebijakan pemerintah yang melakukan pembiaran atau penundaan dalam penerapan pidana mati. Penelitian ini merupakan penelitian hukum normatif dengan menggunakan pendekatan yuridis normatif. Data yang dikumpulkan adalah data sekunder yang dianalisis dengan menggunakan metode analisis yuridis kualitatif. Berdasarkan hasil penelitian ini dapat ditarik kesimpulan bahwa di dalam penerapan pidana mati terdapat permasalahan hukum yang serius, hal ini dikarenakan kebijakan pemerintah yang melakukan pembiaran atau penundaan dalam eksekusi pidana mati merupakan pelanggaran terhadap hak asasi manusia sebagaimana yang diatur dalam Pasal 28 UUD 1945.   Law enforcement without direction and not based on the three pillars of the justice of the law, legal certainty and the benefits to society can break the law anyway even violate human rights. As one of the policies of the government that do not represent the values of justice and disturbing for the people, the government policy that acts of omission or delay in the application of the death penalty. This research is a normative legal normative juridical approach. The data collected is secondary data were analyzed using qualitative methods juridical analysis. Based on these results it can be concluded that in the application of the death penalty there are serious legal issues, this is due to government policies that commit omission or delay in the execution of the death penalty is a violation of human rights as stipulated in Article 28 of the 1945 Constitution.

Ed & Os : kahe Wilde näitemäng / Mati Unt

Index Scriptorium Estoniae

Unt, Mati, 1944-2005

1998-01-01

Mati Undi näidend Eduard Vilde ja Oscar Wilde'i kohtumisest. Illustratsiooniks Tiiu Kirsipuu Tartusse Wilde Irish Pubi ette loodava skulptuurigrupi kavand. Autori märkus : Tekst on kirjutatud Kahe Wilde Pubi avamiseks ja koostatud Wilde'i ja Vilde tekstidest.

Farm Shop : Augmenter l'accès aux matières premières agricoles au ...

International Development Research Centre (IDRC) Digital Library (Canada)

Farm Shop est un modèle de franchise social novateur qui permet d'obtenir des matières premières d'excellente qualité à des prix abordables grâce à des économies d'échelle. Il forme également des franchisés et des agriculteurs sur la façon d'utiliser les matières premières. Au cours de ses trois premières années ...

PERBINCANGAN MENGENAI HUKUMAN MATI TERKAIT KASUS BALI NINE DAN MARY JANE DALAM SITUS JEJARING SOSIAL TWITTER

Directory of Open Access Journals (Sweden)

Jimi Narotama Mahameruaji

2016-06-01

Full Text Available Twitter telah menjadi alat atau media komunikasi yang sangat populer diantara para pengguna Internet. Melalui Twitter, penggunanya dapat berbagi cerita hidup mereka sehari-hari, melakukan perbincangan dengan pengguna lain dan juga mengekspresikan pendapat mereka. Twitter juga dapat dilihat sebagai sebuah wadah untuk melakukan perbincangan politik dan isu-isu publik. Oleh karena itu, peran Twitter terkait partisipasi publik, kampanye, dan pembentukan opini publik kini semakin diperhitungkan (Jungherr, 2015. Fokus penelitian ini tentang perbincangan para pengguna Twitter di Indonesia mengenai peristiwa hukuman mati kasus narkoba Bali Nine dan Mary Jane. Penelitian ini bertujuan untuk mengetahui apa ragam perbincangan yang terjadi di antara para pengguna Twitter Indonesia terkait kasus hukuman mati tersebut, apa argumen yang muncul terkait penolakan maupun dukungan terhadap isu hukuman mati, dan juga siapa saja Twitter Influencer yang berperan dalam isu ini.   DOI: 10.24198/jkk.vol4n1.5

Matis and Korubo, Contact, and Isolated Indigenous Peoples: Native Narratives and Ethnography in the Brazilian Amazon

Directory of Open Access Journals (Sweden)

Barbara Maisonnave Arisi

2010-02-01

Full Text Available This article is about isolation, contact, and relations between two Amazonian indigenous peoples: the Matis and the Korubo. Both groups, of the Panoan linguistic family, live in the Vale do Javari Indigenous Land, in the state of Amazonas, Brazil. The Matis were contacted by the Funai (the Brazilian agency for indigenous affairs in 1976, and they worked as intermediaries helping the Brazilian government to make contact with the Korubo in 1996. Since then, the Matis have been the main translators and mediators between the Korubo and the rest of the world (indigenous and non-indigenous. Based on my investigation, I propose to classify “isolation” in different ways and to relate the Matis’ own narratives about their contact with their neighbors the Korubo in order to approximate a native conception of what “isolation” and “isolated peoples” mean—if they mean anything at all.

FIRST Bent-Double Radio Sources: Tracers of High-Redshift Clusters

International Nuclear Information System (INIS)

Blanton, E. L.; Gregg, M. D.; Helfand, D. J.; Becker, R. H.; White, R. L.

2000-01-01

Bent-double radio sources can act as tracers for clusters of galaxies. We present imaging and spectroscopic observations of the environments surrounding 10 of these sources (most of them wide-angle tails [WATs]) selected from the VLA FIRST survey. Our results reveal a previously unknown cluster associated with eight of the radio sources with redshifts in the range 0.33< z<0.85; furthermore, we cannot rule out that the other two bent doubles may be associated with clusters at higher redshift. Richness measurements indicate that these clusters are typical of the majority of those found in the Abell catalog, with a range of Abell richness classes from 0 to 2. The line-of-sight velocity dispersions are very different from cluster to cluster, ranging from approximately 300 to 1100 km s-1. At the upper end of these intervals, we may be sampling some of the highest redshift massive clusters known. Alternatively, the large velocity dispersions measured in some of the clusters may indicate that they are merging systems with significant substructure, consistent with recent ideas concerning WAT formation (Burns et al.). (c) 2000 The American Astronomical Society

Medusa spectroscopy of A400, A576, A1767, and A2124

International Nuclear Information System (INIS)

Hintzen, P.; Hill, J.M.; Lindley, D.; Scott, J.S.; Angel, J.R.P.

1982-01-01

Galaxy velocity data taken with the Steward Observatory multiple aperture fiber optic spectrograph are presented for four Abell clusters. The root-mean-square external errors in these velocities are about 100 km/s; accuracy which compares favorably with that obtained from single-object observations. We expect that the recent adoption of a CCD detector should decrease external errors to about 50 km/s. All four of the clusters observed are known x-ray sources and our data agree well with empirically derived velocity dispersion--x-ray luminosity relations for clusters of galaxies. Abell 400 is interesting in this regard, since both its x-ray luminosity and its velocity dispersion are quite small. Such objects are particularly important in determining the slope of the velocity dispersion--x-ray luminosity relation. The large microwave decrement observed in A576 was initially interpreted as due to Compton scattering of the microwave background by the x-ray-emitting intracluster gas. White and Silk have presented Einstein x-ray data which indicate that A576 contains too little gas to produce the observed microwave decrement by Compton scattering. Our velocity dispersion for 47 members of this cluster strengthens their conclusion

Medusa spectroscopy of A400, A576, A1767, and A2124

Science.gov (United States)

Hintzen, P.; Hill, J. M.; Lindley, D.; Scott, J. S.; Angel, J. R. P.

1982-01-01

Galaxy velocity data taken with the Steward Observatory multiple aperture fiber optic spectrograph are presented for four Abell clusters. The root-mean-square external errors in these velocities are about 100 km/s; accuracy which compares favorably with that obtained from single-object observations. It is expected that the recent adoption of a CCD detector should decrease external errors to about 50 km/s. All four of the clusters observed are known X-ray sources and the present data agree well with empirically derived velocity dispersion-X-ray luminosity relations for clusters of galaxies. Abell 400 is interesting in this regard, since both its X-ray luminosity and its velocity dispersion are quite small. Such objects are particularly important in determining the slope of the velocity dispersion-X-ray luminosity relation. The large microwave decrement observed in A576 was initially interpreted as due to Compton scattering of the microwave background by the X-ray-emitting intracluster gas. White and Silk have presented Einstein X-ray data which indicate that A576 contains too little gas to produce the observed microwave decrement by Compton scattering. The velocity dispersion obtained here for 47 members of this cluster strengthens their conclusion.

The principle of open access is an essential part of our profession

OpenAIRE

Editores Biblios

2012-01-01

Interview with Abel Laerte Packer (Brazil). Project coordinator of SciELO (Scientific Electronic Library Online) and Advisor to the da Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP). Master's degree in librarianship by Syracuse University, New York, has been director of the Latin American and Caribbean Center on Health Sciences Information (BIREME/PAHO/WHO).

Välis- ja kodueesti kunst kui tervik : sõnum Torontost / Mai Levin

Index Scriptorium Estoniae

Levin, Mai, 1942-

2003-01-01

30. X Tartu Kunstimajas Osvald Timmase näitusel kunstniku loomingule pühendatud õhtust, kus esinesid Mai Levin ja kunstniku vend Evald Timmas, näidati slaide ning Ain Habichti tehtud koduvideosid O. Timmasest ja Abel Leest. A. Lee ja O. Timmas on olnud 1952. a. Torontos loodud Colour and Form Society presidendid. Väliseesti kunsti tuleks käsitleda koos kodueesti kunstiga

Värvi triumf / Mai Levin

Index Scriptorium Estoniae

Levin, Mai, 1942-

2010-01-01

Näitus "Neoimpressionismi jälgedes. Mägi ja Finch" Kumu Kunstimuuseumis 12. septembrini 2010. Kuraator Tiina Abel, kuraatori abi Liisa Kaljula, kujundaja Inga Heamägi. Puäntillismi mõjust, Konrad Mäe pöördumisest täppiva laadi poole. Inglise päritolu belgia-soome kunstniku Alfred William Finchi avastamisest. Prantsuse ja eesti kunstnike töödest näitusel

An improved experimental scheme for simultaneous measurement of high-resolution zero electron kinetic energy (ZEKE) photoelectron and threshold photoion (MATI) spectra

Science.gov (United States)

Michels, François; Mazzoni, Federico; Becucci, Maurizio; Müller-Dethlefs, Klaus

2017-10-01

An improved detection scheme is presented for threshold ionization spectroscopy with simultaneous recording of the Zero Electron Kinetic Energy (ZEKE) and Mass Analysed Threshold Ionisation (MATI) signals. The objective is to obtain accurate dissociation energies for larger molecular clusters by simultaneously detecting the fragment and parent ion MATI signals with identical transmission. The scheme preserves an optimal ZEKE spectral resolution together with excellent separation of the spontaneous ion and MATI signals in the time-of-flight mass spectrum. The resulting improvement in sensitivity will allow for the determination of dissociation energies in clusters with substantial mass difference between parent and daughter ions.

Observations of High Dispersion Clusters of Galaxies: Constraints on Cold Dark Matter

Science.gov (United States)

Oegerle, William R.; Hill, John M.; Fitchett, Michael J.

1995-07-01

We have studied the dynamics of several Abell clusters of galaxies, which were previously reported to have large velocity dispersions, and hence very large masses. In particular, we have investigated the assertion of Frenk et al. (1990) that clusters with intrinsic velocity dispersions ~> 1200 km s^-1^ are extremely rare in the universe, and that large observed dispersions are due to projection effects. We report redshifts for 303 galaxies in the fields of A1775, A2029, A2142, and A2319, obtained with the Nessie multifiber spectrograph at the Mayall 4 m telescope. A1775 appears to be two poor, interacting clusters, separated in velocity space by ~3075 km s^-1^ (in the cluster rest frame). A2029 has a velocity dispersion of 1436 km s^-1^, based on 85 cluster member redshifts. There is evidence that a group or poor cluster of galaxies of slightly different redshift is projected onto (or is merging with) the core of A2029. However, the combined kinematic and x-ray data for A2029 argue for an intrinsically large dispersion for this cluster. Based on redshifts for 103 members of A2142, we find a dispersion of 1280 km s^-1^, and evidence for subclustering. With 130 redshifts in the A2319 field, we have isolated a subcluster ~10' NW of the cD galaxy. After its removal, A2319 has a velocity dispersion of 1324 km s^-1^. The data obtained here have been combined with recent optical and X-ray data for other supposedly high-mass clusters to study the cluster velocity dispersion distribution in a sample of Abell clusters. We find that clusters with true velocity dispersions ~> 1200 km s^-1^ are not extremely rare, but account for ~5% of all Abell clusters with R >= 0. If these clusters are in virial equilibrium, then our results are inconsistent with a high-bias (b~>22), high-density CDM model.

Mati Hint - sünge keeleteadlane ja pessimistlik ühiskonnategelane / Mari Klein

Index Scriptorium Estoniae

Klein, Mari, 1979-

2007-01-01

11. septembril peeti Tallinna Ülikoolis seminari, mis oli pühendatud Mati Hindi 70. sünnipäevale. Ettekannetega esinesid ülikoolikaaslased, sõbrad ja kolleegid Rein Veidemann, Haldur Õim, Martin Ehala, Mats Traat, Tapani Lehtinen, Jaan Kaplinski

Redshifts of radio galaxies in Abell clusters of galaxies

International Nuclear Information System (INIS)

Owen, F.N.; White, R.A.; Thronson, H.A. Jr.

1988-01-01

The paper presents redshifts for 51 radio galaxies and companion systems which were obtained with the Steward 2.3-m and multiple mirror telescopes. The observations were performed over the course of six runs during 1980-1983. The sample includes eight multiple systems (or multiple nuclei) having internal velocity differences ranging from 150 to 2400 km/s. 17 references

The Baryonic and Dark Matter Distributions in Abell 401

Science.gov (United States)

Nevalainen, J.; Markevitch, M.; Forman, W.

1999-11-01

We combine spatially resolved ASCA temperature data with ROSAT imaging data to constrain the total mass distribution in the cluster A401, assuming that the cluster is in hydrostatic equilibrium, but without the assumption of gas isothermality. We obtain a total mass within the X-ray core (290 h-150 kpc) of 1.2+0.1-0.5×1014 h-150 Msolar at the 90% confidence level, 1.3 times larger than the isothermal estimate. The total mass within r500 (1.7 h-150 Mpc) is M500=0.9+0.3-0.2×1015 h-150 Msolar at 90% confidence, in agreement with the optical virial mass estimate, and 1.2 times smaller than the isothermal estimate. Our M500 value is 1.7 times smaller than that estimated using the mass-temperature scaling law predicted by simulations. The best-fit dark matter density profile scales as r-3.1 at large radii, which is consistent with the Navarro, Frenk & White (NFW) ``universal profile'' as well as the King profile of the galaxy density in A401. From the imaging data, the gas density profile is shallower than the dark matter profile, scaling as r-2.1 at large radii, leading to a monotonically increasing gas mass fraction with radius. Within r500 the gas mass fraction reaches a value of fgas=0.21+0.06-0.05 h-3/250 (90% confidence errors). Assuming that fgas (plus an estimate of the stellar mass) is the universal value of the baryon fraction, we estimate the 90% confidence upper limit of the cosmological matter density to be ΩmEinstein-deSitter universe. Even though the NFW dark matter density profile is statistically consistent with the temperature data, its central temperature cusp would lead to convective instability at the center, because the gas density does not have a corresponding peak. One way to reconcile a cusp-shaped total mass profile with the observed gas density profile, regardless of the temperature data, is to introduce a significant nonthermal pressure in the center. Such a pressure must satisfy the hydrostatic equilibrium condition without inducing turbulence. Alternately, significant mass drop-out from the cooling flow would make the temperature less peaked and the NFW profile acceptable. However, the quality of data is not adequate to test this possibility.

Pierre Deligne Wins Abel Prize 2013 Information and Announcements

Indian Academy of Sciences (India)

IAS Admin

which won him the Fields Medal in 1978. The novel methods he introduced not only revolutionized algebraic geometry and number theory and led to their synthesis, they have continued to drive most of contemporary research in arithmetic and geometry. Many mathematical tools introduced by him have become so standard ...

Teatriõpilane ja -uuendaja Mati Unt Vanemuises (1966 - 1972) / Ülo Tonts

Index Scriptorium Estoniae

Tonts, Ülo, 1931-2016

2008-01-01

Teatriloolisi meeldetuletusi ja ääremärkusi. Vaatluse all on Mati Undi tööd ja tegemised Vanemuise perioodil. Tööst lavastaja assistendi, instseneerija ja tõlkijana. Koostööst Kaarel Irdi ja Evald Hermakülaga. Algus eelmises TMKs

Lateral mobility of plasma membrane lipids in Xenopus eggs: Regional differences related to animal/vegetal polarity

OpenAIRE

Laat, S.W. de; Bluemink, J.G.; Dictus, W.J.A.G.; Zoelen, E.J.J. van; Tetteroo, P.A.T.; Tertoolen, L.G.J.

1984-01-01

Regional differences in the lateral mobility properties of plasma membrane lipids were studied in unfertilized and fertilized Xenopus eggs by fluorescence photobleaching recovery (FPR) measurements. Out of a variety of commonly used lipid probes only the aminofluorescein- -1abelled fatty acids HEDAF (5-(N-hexadecanoyl)- aminofluorescein) and TEDAF (5-(N-tetradecanoyl)-aminofluorescein) appear to distribute itself in the plasma membrane. Under all experimental conditions used these molecules s...

A Spatiotemporal Clustering Approach to Maritime Domain Awareness

Science.gov (United States)

2013-09-01

reveal two clusters , -step two are shown in Figure 12 o, colored green and cyan and l ically clustered , ed. c1 and c2 , . In abeled c1...development,” Center for Development Research , University of Bonn, Bonn, Germany, Working Paper Nr. 17, 2006. 104 THIS PAGE INTENTIONALLY LEFT... CLUSTERING APPROACH TO MARITIME DOMAIN AWARENESS by Kristofer A. Tester September 2013 Thesis Advisor: Jim Scrofani Thesis Co-Advisor

Primer registro de Plica plica (Linnaeus, 1758 para el departamento de La Paz, Bolivia. Comentarios sobre la extensión de la distribución geográfica para Plica umbra (Linnaeus 1758, (Squamata: Tropiduridae

Directory of Open Access Journals (Sweden)

Aguilar-Kirigin, Alvaro J.

2011-12-01

Full Text Available Siete ejemplares de la especie Plica plica y tres de Plica umbra fueron colectados en la República de Bolivia y depositados en la Colección Boliviana de Fauna (CBF, La Paz, Bolivia. Todos los registros se realizaron en el Departamento de La Paz, Provincia Abel Iturralde, Capital de Provincia Ixiamas, Sección Primera, Municipio Ixiamas, Cantón Ixiamas, Capital de Cantón Tahua.

Kõnelused Tartus / Anne Untera

Index Scriptorium Estoniae

Untera, Anne, 1951-

2007-01-01

8.-10. V Tartus toimunud eesti, läti ja saksa kunstiteadlaste ühisseminarist. Alexander Knorre rääkis Karl August Senffi, Ilona Audere Friedrich Ludwig von Maydelli, Mai Levin Karl Alexander von Winkleri, Kristiana Abele Johann Walter-Kurau (1869-1932), Anne Untera Konstantin ja Sally von Kügelgeni, Epp Preem Julie Hagen-Schwartzi, Friedrich Gross Eduard von Gebhardti ja Katharina Hadding Ida Kerkoviuse (1879-1970) loomingust

Laboratory Performance of the Single-Sided E-A-R (registered trademark) Combat Arms Hearing Protective Earplug

Science.gov (United States)

2010-01-01

Research article / Article de recherche LABORATORY PERFORMANCE OF THE SINGLE-SIDED EAR® COMBAT ARMS HEARING PROTECTIVE EARPLUG Sharon M. Abel and...external microphones for enhanced L:. -communication-? ;‘ V SOMMAIRE. Le but de cet article est de comparer 1 effet du port de bouchons conventionnels a...MA. Bekesy audiometry and loudness balance testing. In: Katz, J, editor. Handbook of clinical audiology . 3rd ed. Williams & Wilkins: Baltimore; 1985

De wondere wereld van Alex van Warmerdam: absurdisme in de eigentijdse Nederlandse film

Directory of Open Access Journals (Sweden)

L. Nas

1999-04-01

After situating both Abel and De noorderlingen within the context of contemporary Dutch cinema and television, as well as within the filmmaker’s cinematic oeuvre, the article will introduce Alex van Warmerdam's background and closely analyse both films. Finally it will be argued that Van Warmerdam's films force Dutch audiences to take an ironic, critical look at themselves, a new take in Dutch cinema that has also found approval abroad.

Põlvkondade triloogia Von Krahli teatris / Hedi-Liis Toome

Index Scriptorium Estoniae

Toome, Hedi-Liis

2010-01-01

Von Krahli teatri lavastustest: William Shakespeare "Kuningas Lear", mängib Viljandi Kultuuriakadeemia 8. lend, lavastaja Peeter Jalakas (esietendus 30. jaan. 2010); "The End" - autorid, lavastajad ja näitlejad: Mari Abel, Tiina Tauraite, Riina Maidre, Erki Laur, Taavi Eelmaa, Juhan Ulfsak (esietendus 19. märts 2010); "Mehed lumes" Peter Freucheni jutustuse "Olavi lugu" ainetel lavastanud Mart Koldits ja Kristjan Sarv, kes ka ise mängivad (17. aprill 2010)

A new algorithm to determine the total radiated power at ASDEX upgrade

Energy Technology Data Exchange (ETDEWEB)

Gloeggler, Stephan; Bernert, Matthias; Eich, Thomas [Max Planck Institute for Plasma Physics, Boltzmannstr. 2, 85748 Garching (Germany); Collaboration: The ASDEX Upgrade Team

2016-07-01

Radiation is an essential part of the power balance in a fusion plasma. In future fusion devices about 90% of the power will have to be dissipated, mainly by radiation. For the development of an appropriate operational scenario, information about the absolute level of plasma radiation (P{sub rad,tot}) is crucial. Bolometers are used to measure the radiated power, however, an algorithm is required to derive the absolute power out of many line-integrated measurements. The currently used algorithm (BPD) was developed for the main chamber radiation. It underestimates the divertor radiation as its basic assumptions are not satisfied in this region. Therefore, a new P{sub rad,tot} algorithm is presented. It applies an Abel inversion on the main chamber and uses empirically based assumptions for poloidal asymmetries and the divertor radiation. To benchmark the new algorithm, synthetic emissivity profiles are used. On average, the new Abel inversion based algorithm deviates by only 10% from the nominal synthetic value while BPD is about 25% too low. With both codes time traces of ASDEX Upgrade discharges are calculated. The analysis of these time traces shows that the underestimation of the divertor radiation can have significant consequences on the accuracy of BPD while the new algorithm is shown to be stable.

Discovery of intergalactic radio emission in the Coma-A1367 supercluster

International Nuclear Information System (INIS)

Kim, K.T.; Kronberg, P.P.; Venturi, T.

1989-01-01

The Coma cluster is a rich cluster of galaxies nested in an even larger super cluster of galaxies. The plane of the supercluster seems to be defined by the Coma cluster itself and another galaxy cluster, Abell 1367, which lies ∼ 40 Mpc farther west. The largest structures known are the giant voids and superclusters which are as large as 70h 75 -1 Mpc (refs 3-5). The Coma cluster of galaxies seems to be located on the rim of a giant void in the three-dimensional distribution of galaxies. Here we describe the detection of faint, supercluster-scale radio emission at 326 MHz that extends between the Coma cluster of galaxies and the Abell 1367 cluster and which is apparently not associated with any individual galaxy system in the complex. The radiation's synchrotron origin implies the existence of a large-scale intercluster magnetic field with an estimated strength of 0.3-0.6 μG, which is remarkably strong. The synchrotron-emitting relativistic electrons cannot be older than a few times 10 8 yr, but we speculate that the magnetic field is the fossil of a pre-galactic primaeval field, which was amplified in the course of the formation of intergalactic voids and superclusters. (author)

DYNAMIC DEFORMATION THE VISCOELASTIC TWOCOMPONENT MEDIUM

Directory of Open Access Journals (Sweden)

V. S. Polenov

2015-01-01

Full Text Available Summary. In the article are scope harmonious warping of the two-component medium, one component which are represent viscoelastic medium, hereditary properties which are described by the kernel aftereffect Abel integral-differential ratio BoltzmannVolterr, while second – compressible liquid. Do a study one-dimensional case. Use motion equation of two-component medium at movement. Look determination system these equalization in the form of damped wave. Introduce dimensionless coefficient. Combined equations happen to homogeneous system with complex factor relatively waves amplitude in viscoelastic component and in fluid. As a result opening system determinant receive biquadratic equation. Elastic operator express through kernel aftereffect Abel for space Fourier. With the help transformation and symbol series biquadratic equation reduce to quadratic equation. Come to the conclusion that in two-component viscoelastic medium exist two mode sonic waves. As a result solution of quadratic equation be found description advance of waves sonic in viscoelastic two-component medium, which physical-mechanical properties represent complex parameter. Velocity determination advance of sonic waves, attenuation coefficient, mechanical loss tangent, depending on characteristic porous medium and circular frequency formulas receive. Graph dependences of description advance of waves sonic from the temperature logarithm and with the fractional parameter γ are constructed.

Investigation of the sensitivity of visible continuum Zeff(0) to edge radiation

International Nuclear Information System (INIS)

Telesca, G.; Oost, G. Van; Ongena, J.; Leys, C.; Schoon, N.

1992-01-01

The determination of Z eff from visible continuum radiation is based on the assumption that the line-integrated continuum signal is mostly composed of bremsstrahlung radiation. In practice a wavelength window relatively free of spectral lines is selected, and the line-integrated continuum signal along different chords from the edge up to the central plasma is measured. The local emissivity ε(r) is then calculated using an Abel inversion procedure, and the Z eff profile can be obtained. Although theory and techniques are well established, in any experimental device there remains an uncertainty in the calculated value of Z eff due to the non-bremsstrahlung radiation from the cooler edge plasma (e.g. emission from recombination and molecular bands). As a consequence, the local bremsstrahlung emissivity in the outer region of the plasma cannot be determined and the signal measured along every chord through the plasma contains a spurious contribution. In this paper the error in the value of the central plasma emissivity (and Z eff ) due to edge radiation has been investigated. Qualitative analytical considerations have been complemented by a qualitative analysis, consisting of the comparison of test emissivity profiles with Abel-inverted profiles obtained from the integrals along central chords only. (author) 5 refs., 5 figs

Reviews of recent publications

Directory of Open Access Journals (Sweden)

2010-01-01

Full Text Available Esperança Bielsa. The Latin American Urban Crónica: Between Literature and Mass Culture by Miguel González-Abellás Gene H. Bell-Villada, ed. Gabriel García Márquez’s One Hundred Years of Solitude: A Casebook by Miguel González-Abellás Albert Memmi. Decolonization and the Decolonized . Trans. Robert Bononno by Christa Jones Erin Graff Zivin. The Wandering Signifier: Rhetoric of Jewishness in the Latin American Imaginary by Naomi Lindstrom Dawn Fulton. Signs of Dissent: Maryse Condé and Postcolonial Crticism by Jane E. Evans Anne Lambright. Creating the Hybrid Intellectual: Subject, Space and the Feminine in the Narrative of José María Arguedas by Arturio Arias Andrew Sobanet. Jail Sentences: Representing Prison in Twentieth-Century French Fiction by Elisabeth-Christine Muelsch Olga López-Valero Colbert. The Gaze on the Past: Popular Culture and History in Antonio Muñoz Molina’s Novels by Jorge Pérez Warren Motte. Fiction Now: The French Novel in the Twenty-First Century by Martine Fernandes Hélène Cixous. Hyperdream . Trans. Beverley Bie Brahic. by Amy Baram Reid Jean-Michel Rabaté. 1913: The Cradle of Modernism by Safoi Babana-Hampton

Liquid-film stripper for high-intensity heavy-ion beams

International Nuclear Information System (INIS)

Leemann, B.T.; Merrill, P.; Syversrud, H.K.; Wada, R.; Yourd, R.B.

1981-03-01

Electron strippers are widely used in heavy ion accelerators such as tandem Van de Graaff generators and heavy ion linacs. The SuperHILAC at Lawrence Berkeley Laboratory, employs a fluorocarbon oil vapor stripper at 113 keV/A for its high intensity injector ABEL, while after acceleration to 1.199 MeV/A a 35 μg/cm 2 carbon foil stripper is used. At present, the lifetime of these foils is about 1 hour for an 40 Ar beam of approx. 1 μA average particle current. With higher intensity high mass (100 less than or equal to A less than or equal to 238) beams available from ABEL injector the lifetime is expected to drop drastically and might be as low as one minute. A different approach to solve the stripper foil lifetime problem uses a thin free standing oil film spun from the edge of a sharp-edged rotating disc touching the surface of an oil reservoir. Areas of about 10 cm 2 with areal densities down to 20 μg/cm 2 have been reported. The work described here is based on the same concept, and produces a constantly regenerated, stable, free standing oil film of appropriate thickness for use at the SuperHILAC

Organismes de politiques et recherche en matière de santé

International Development Research Centre (IDRC) Digital Library (Canada)

gprudhomme

17 mars 2014 ... en renforçant les politiques nationales et l'équité dans les systèmes de santé. ...... matière de leadership stratégique, d'administration de programmes et de gestion ... Décrire les plans de recrutement adoptés pour combler les ...

VLA Discovers Giant Rings Around Galaxy Cluster

Science.gov (United States)

2006-11-01

Astronomers using the National Science Foundation's Very Large Array (VLA) radio telescope have discovered giant, ring-like structures around a cluster of galaxies. The discovery provides tantalizing new information about how such galaxy clusters are assembled, about magnetic fields in the vast spaces between galaxy clusters, and possibly about the origin of cosmic rays. Radio-Optical Image of Cluster Galaxy Cluster Abell 3376 (Radio/Optical) CREDIT: Joydeep Bagchi, IUCAA, NRAO/AUI/NSF Above, a combined radio/optical image shows the galaxy cluster Abell 3376 in visible light (blue) and radio (red) images. The giant radio arcs surrounding the cluster were discovered using the Very Large Array. The visible-light image is from the Digitized Sky survey. Below, an X-ray image of Abell 3376 made using the European Space Agency's XMM-Newton telescope shows a spectacular, bullet-shaped region of X-rays coming from gas heated to 60 million degrees Kelvin. The bullet shape results from the supersonic collision of a smaller smaller galaxy subcluster with the main body of the larger cluster. Click on images for larger version. X-Ray Image of Cluster Galaxy Cluster Abell 3376 (X-Ray) CREDIT: Joydeep Bagchi, IUCAA, ESA "These giant, radio-emitting rings probably are the result of shock waves caused by violent collisions of smaller groups of galaxies within the cluster," said Joydeep Bagchi, of the Inter-University Centre for Astronomy and Astrophysics in Pune, India, who led an international research team. The scientists reported their findings in the November 3 edition of the journal Science. The newly-discovered ring segments, some 6 million light-years across, surround a galaxy cluster called Abell 3376, more than 600 million light-years from Earth. They were revealed because fast-moving electrons emitted radio waves as they spiraled around magnetic field lines in intergalactic space. "Even from this large distance, the feeble radio waves were easily picked up by the VLA

Resonantly-enhanced two-photon ionization and mass-analyzed threshold ionization (MATI) spectroscopy of 2-hydroxypyridine

CERN Document Server

Lee, D H; Choi, K W; Choi, Y S; Kim, S K

2002-01-01

Mass-analyzed threshold ionization (MATI) spectra of 2-hydroxypyridines existing as lactims (2-pyridionl) in a molecular beam are obtained via (1+1') two-photon process to give accurate ionization energies of 8.9344 +- 0.0005 and 8.9284 +- 0.0005 eV for 2-pyridinol (2Py-OH) and its deuterated analogue (2Py-OD), respectively. Resonantly-enhanced two-photon ionization spectra of these compounds are also presented to give vibrational structures of their S sub 1 states. Vibrational frequencies of 2Py-OH and 2Py-OD in ionic ground states are accurately determined from MATI spectra taken via various S sub 1 intermediate states, and associated vibrational modes are assigned with the aid of ab initio calculations.

The Benefit of Supplementary Text for the Resolution of Auditory Overload

Science.gov (United States)

2015-05-01

of corrective glasses. Glasses have been shown to interfere with the fit of muff- style devices of the type that would be used in the study (Abel et al...the test language (van Wijngaarden et al., 2002). Only those whose native language was English or those who had learned English before the age of 12...Drullman R, Bronkhorst AW: Speech perception and talker segregation: effects of level, pitch, and tactile support with multiple simultaneous talkers

Cosmic abundances: The impact of stellar duplicity

OpenAIRE

Jorissen, A.; Van Eck, S.

2004-01-01

The mass-transfer scenario links chemical peculiarities with stellar duplicity for an increasing number of stellar classes (classical and dwarf barium stars, subgiant and giant CH stars, S stars without technetium, yellow symbiotic stars, WIRRING stars, Abell-35-like nuclei of planetary nebulae...). Despite these successes, the mass-transfer scenario still faces several problems: What is the mass-transfer mode? Why orbital elements of dwarf barium stars do not fully match those of the classic...

Ensuring a Strong U.S. Defense for the Future: The National Defense Panel Review of the 2014 Quadrennial Defense Review

Science.gov (United States)

2014-07-31

territorial disputes with China. We note recent moves to station U.S. forces in Darwin , the plan to station a number of Littoral Combat Ships in Singapore...Under Secretary of Defense, Comptroller (C) Charles “Chuck” Hagel Secretary of Defense Mara Karlin Principal Director for Strategy, Policy (P...Support Staff to the Panel Charles Arnold George Sinks U.S. Government Liaison Officers Lori Abele Chief of Staff, Deputy Under Secretary of Defense

Quantitative measurements in laser induced plasmas using optical probing. Progress report, October 1, 1977--April 30, 1978

International Nuclear Information System (INIS)

Sweeney, D.W.

1978-06-01

Optical probing of laser induced plasmas can be used to quantitatively reconstruct electron number densities and magnetic fields. Numerical techniques for extracting quantitative information from the experimental data are described and four Abel inversion codes are provided. A computer simulation of optical probing is used to determine the quantitative information that can be reasonably extracted from real experimental systems. Examples of reconstructed electron number densities from interferograms of laser plasmas show steepened electron distributions

Microfoundations and the birth of a firm's identity: How entrepreneurs deal with routines to entrench their start-up in an ecosystem

OpenAIRE

Kokshagina , Olga; Hooge , Sophie; Canet , Emilie

2016-01-01

International audience; How to shape successful ventures; ensure that an entrepreneur’s journey will lead to create viable businesses over time? It is argued that organizations are built on habits and routines in place that are defined as dispositions to follow certain behavioral tendencies motivated by appropriate contexts and environments (Abell et al., 2007; Becker, 2012; Cohen, 2012; Nelson & Sidney, 1982). Prior work stressed that the individual identity, founders’ habits influence the e...

Auditory Pattern Memory

Science.gov (United States)

1990-10-31

Creelman , 1962; Getty, 1975; Divenyi and Danner, kin et aL (1982) jitter-detection paradigm. An advantage of 1977; Divenyi and Sachs, 1978; and Allen...discrimination of tonal se- Creelman . C. D. (1962). "’Human discrimination ofauditory duration." 3. quences.’" J. Acoust. Soc. Am. 82.1218-1226. Acoust...single marked intervals (Abel, 1972a,b; Creelman , 1962; Getty, 1975; Divenyi and Danner, 1977; Divenyi and Sachs, 1978; Espinoza-Varas and Jamieson

Regards sur la matière des quantas et des choses

CERN Document Server

Espagnat, Bernard d'

1993-01-01

La physique quantique n'est pas seulement à la base de nombreuses inventions de pointe. Elle constitue aussi une révolution conceptuelle de grande ampleur.Bien que ses implications pratiques comme ses conséquences philosophiques soient immenses, la physique quantique est encore mal connue des non-spécialistes, en partie à cause des difficultés qu'il y a à exposer ses fondements.Or c'est justement la gageure réussie de cet ouvrage. En un style clair, enjoué et dépourvu d'équations, Etienne Klein nous guide dans les profondeurs de la matière. Nous découvrons avec lui des expériences aussi étranges que celle des fentes de Young ", qui montre que la matière est à la fois onde et corpuscule et que ses caractéristiques sont en partie liées... à notre propre existence en tant qu'observateur humain! Après avoir pris connaissance de paradoxes surprenants comme celui du chat de Schrödinger _ un chat à la fois mort et vivant! _ nous abordons la mystérieuse question de la " non-séparabilité ", s...

Orphan Stars Found in Long Galaxy Tail

Science.gov (United States)

2007-09-01

Astronomers have found evidence that stars have been forming in a long tail of gas that extends well outside its parent galaxy. This discovery suggests that such "orphan" stars may be much more prevalent than previously thought. The comet-like tail was observed in X-ray light with NASA's Chandra X-ray Observatory and in optical light with the Southern Astrophysical Research (SOAR) telescope in Chile. The feature extends for more than 200,000 light years and was created as gas was stripped from a galaxy called ESO 137-001 that is plunging toward the center of Abell 3627, a giant cluster of galaxies. "This is one of the longest tails like this we have ever seen," said Ming Sun of Michigan State University, who led the study. "And, it turns out that this is a giant wake of creation, not of destruction." Chandra X-ray Image of ESO 137-001 and Tail in Abell 3627 Chandra X-ray Image of ESO 137-001 and Tail in Abell 3627 The observations indicate that the gas in the tail has formed millions of stars. Because the large amounts of gas and dust needed to form stars are typically found only within galaxies, astronomers have previously thought it unlikely that large numbers of stars would form outside a galaxy. "This isn't the first time that stars have been seen to form between galaxies," said team member Megan Donahue, also of MSU. "But the number of stars forming here is unprecedented." The evidence for star formation in this tail includes 29 regions of ionized hydrogen glowing in optical light, thought to be from newly formed stars. These regions are all downstream of the galaxy, located in or near the tail. Two Chandra X-ray sources are near these regions, another indication of star formation activity. The researchers believe the orphan stars formed within the last 10 million years or so. The stars in the tail of this fast-moving galaxy, which is some 220 million light years away, would be much more isolated than the vast majority of stars in galaxies. H-alpha Image of

Tallinnas Narva mnt. 7 asuva kohviku Zebra sisekujundus / Tiiu Truus, Tiiu Prisko, Mati Veermets...[jt.

Index Scriptorium Estoniae

2006-01-01

põhiplaan, 11 värv. vaadet; fotod: Kalle Veesaar; laes olevate dekoratiivsete lippude graafiline kujundus on Tiiu Priskolt ja Mati Veermetsalt, tualettruumi looduskivist valamu ja põrandavaasi autor on Kaido Kivi

Leadership municipal intersectoriel en matière de santé en ...

International Development Research Centre (IDRC) Digital Library (Canada)

Ce projet vise à consolider le leadership en matière d'écosanté à l'échelle municipale en Colombie et au Vénézuela afin d'aborder les priorités en santé, notamment les maladies à transmission vectorielle et les interventions sur les systèmes d'alimentation en vue de prévenir les maladies non transmissibles. Dengue et ...

Renforcer le leadership en matière de politiques parmi les ...

International Development Research Centre (IDRC) Digital Library (Canada)

Les travailleurs de la santé doivent posséder le leadership et les capacités en matière de recherche et d'élaboration de politiques requis pour concevoir des programmes efficaces de lutte contre la pandémie de VIH/sida. Cette collaboration novatrice multipays visait à renforcer les programmes de santé axés sur le VIH/sida ...

Gestionnaire Services en gestion et innovation en matière d ...

International Development Research Centre (IDRC) Digital Library (Canada)

Plus particulièrement, il cerne les besoins des clients en matière d'information, administre les services de recherche destinés aux utilisateurs finaux, s'assure que les clients internes connaissent la façon d'accéder l'information emmagasinée dans les différents répertoires du Centre, conçoit et met sur pied une architecture ...

The Self-Powered Detector Simulation `MATiSSe' Toolbox applied to SPNDs for severe accident monitoring in PWRs

Science.gov (United States)

Barbot, Loïc; Villard, Jean-François; Fourrez, Stéphane; Pichon, Laurent; Makil, Hamid

2018-01-01

In the framework of the French National Research Agency program on nuclear safety and radioprotection, the `DIstributed Sensing for COrium Monitoring and Safety' project aims at developing innovative instrumentation for corium monitoring in case of severe accident in a Pressurized Water nuclear Reactor. Among others, a new under-vessel instrumentation based on Self-Powered Neutron Detectors is developed using a numerical simulation toolbox, named `MATiSSe'. The CEA Instrumentation Sensors and Dosimetry Lab developed MATiSSe since 2010 for Self-Powered Neutron Detectors material selection and geometry design, as well as for their respective partial neutron and gamma sensitivity calculations. MATiSSe is based on a comprehensive model of neutron and gamma interactions which take place in Selfpowered neutron detector components using the MCNP6 Monte Carlo code. As member of the project consortium, the THERMOCOAX SAS Company is currently manufacturing some instrumented pole prototypes to be tested in 2017. The full severe accident monitoring equipment, including the standalone low current acquisition system, will be tested during a joined CEA-THERMOCOAX experimental campaign in some realistic irradiation conditions, in the Slovenian TRIGA Mark II research reactor.

Vers une politique nationale en matière de sciences et de ...

International Development Research Centre (IDRC) Digital Library (Canada)

Le Consejo Nicaragüense de Ciencia y Tecnologia (CONICYT) a pour mandat de coordonner les différents acteurs du système d'innovation national du Nicaragua. Cette subvention permettra au CONICYT de concevoir une stratégie nationale en matière de sciences, de technologies et d'innovation (STI). Les extrants ...

One-photon mass-analyzed threshold ionization (MATI) spectroscopy of pyridine: Determination of accurate ionization energy and cationic structure

Energy Technology Data Exchange (ETDEWEB)

Lee, Yu Ran; Kang, Do Won; Kim, Hong Lae, E-mail: chkwon@kangwon.ac.kr, E-mail: hlkim@kangwon.ac.kr; Kwon, Chan Ho, E-mail: chkwon@kangwon.ac.kr, E-mail: hlkim@kangwon.ac.kr [Department of Chemistry and Institute for Molecular Science and Fusion Technology, College of Natural Sciences, Kangwon National University, Chuncheon 200-701 (Korea, Republic of)

2014-11-07

Ionization energies and cationic structures of pyridine were intensively investigated utilizing one-photon mass-analyzed threshold ionization (MATI) spectroscopy with vacuum ultraviolet radiation generated by four-wave difference frequency mixing in Kr. The present one-photon high-resolution MATI spectrum of pyridine demonstrated a much finer and richer vibrational structure than that of the previously reported two-photon MATI spectrum. From the MATI spectrum and photoionization efficiency curve, the accurate ionization energy of the ionic ground state of pyridine was confidently determined to be 73 570 ± 6 cm{sup −1} (9.1215 ± 0.0007 eV). The observed spectrum was almost completely assigned by utilizing Franck-Condon factors and vibrational frequencies calculated through adjustments of the geometrical parameters of cationic pyridine at the B3LYP/cc-pVTZ level. A unique feature unveiled through rigorous analysis was the prominent progression of the 10 vibrational mode, which corresponds to in-plane ring bending, and the combination of other totally symmetric fundamentals with the ring bending overtones, which contribute to the geometrical change upon ionization. Notably, the remaining peaks originate from the upper electronic state ({sup 2}A{sub 2}), as predicted by high-resolution photoelectron spectroscopy studies and symmetry-adapted cluster configuration interaction calculations. Based on the quantitatively good agreement between the experimental and calculated results, it was concluded that upon ionization the pyridine cation in the ground electronic state should have a planar structure of C{sub 2v} symmetry through the C-N axis.

Conveying Environmental Issues with and through Art

Science.gov (United States)

Abeles, K. V.

2016-12-01

Art has the ability to convey serious environmental issues, inspiring people to respond personally Kim Abeles is an artist who crosses disciplines and media to explore and map urban and global environments. She has exhibited with a unique range of collaborators including smog control agencies, science and natural history museums, and educational and healthcare professionals. Her work has been exhibited across the world. Since 1985, her art projects have explored topics including air and water pollution, refuse and recycling, and consumption. This presentation will discuss three unconventional art projects from inspiration to impact including results. Most can be replicated in any educational or community setting to increase understanding of environmental issues. Abeles's Smog Collector series makes images from polluted air, helping viewers to see the air they breathe in an accessible, engaging, and visceral way. In addition to exhibitions of this work in art museums and galleries, it has been displayed in vehicle emissions testing booths to increase awareness and behavior change, and the process has been taught as curriculum in schools. Abeles sees consumption as a primary problem that leads to environmental decay. Her Paper Person was made from the California Science Center's paper trash that was generated on a single day by their visitors (Earth Day 2009). The 40' x 48' sculpture is in the permanent collection of the CSC, and the text accompanying the artwork prompts visitors to consider bringing their lunches next time instead of buying fast food. Similarly, Paper Person (Harvard Westlake School) is a figurative sculpture made of one week of students' paper trash. Exhibited in the school's gallery, students were able to identify their own scraps, and to see how their consumption and trash adds up. When the artwork was exhibited, the school decided to change the way they handled their lunch preparation, bottled water, and trash. gallery-of-solutions was a recent

Metafüüsika magma pinnapealsuse shlaki all / Mati Sirkel ; interv. Kalev Kesküla

Index Scriptorium Estoniae

Sirkel, Mati

2004-01-01

Tõlkija Mati Sirkel oma raamatust "Orva-aastad". Ka tööst Eesti Kirjanike Liidu esimehena ning kirjaniku kohast ühiskonnas. Vastukaja: Vaher, Berk. Kas kirjanik vajab komissari? // Eesti Ekspress (2004) 5. aug., lk. B9

Solving polynomial differential equations by transforming them to linear functional-differential equations

OpenAIRE

Nahay, John Michael

2008-01-01

We present a new approach to solving polynomial ordinary differential equations by transforming them to linear functional equations and then solving the linear functional equations. We will focus most of our attention upon the first-order Abel differential equation with two nonlinear terms in order to demonstrate in as much detail as possible the computations necessary for a complete solution. We mention in our section on further developments that the basic transformation idea can be generali...

The Effect of Material and Side Walls on Hull Deflection during a Blast Event

Science.gov (United States)

2017-12-13

ARL-CR-0822 ● DEC 2017 US Army Research Laboratory The Effect of Material and Side Walls on Hull Deflection during a Blast Event...Army Research Laboratory The Effect of Material and Side Walls on Hull Deflection during a Blast Event prepared by Danielle Abell SURVICE...Walls on Hull Deflection during a Blast Event 5a. CONTRACT NUMBER W911QX-16-D-0014 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S

High-redshift supernova rates measured with the gravitational telescope A 1689

OpenAIRE

Petrushevska, T.; Amanullah, R.; Goobar, A.; Fabbro, S.; Johansson, J.; Kjellsson, T.; Lidman, C.; Paech, K.; Richard, J.; Dahle, Håkon; Ferretti, R.; Kneib, J.-P.; Limousin, M.; Nordin, J.; Stanishev, V.

2016-01-01

Aims. We present a ground-based, near-infrared search for lensed supernovae behind the massive cluster Abell 1689 at z = 0.18, which is one of the most powerful gravitational telescopes that nature provides. Methods. Our survey was based on multi-epoch J-band observations with the HAWK-I instrument on VLT, with supporting optical data from the Nordic Optical Telescope. Results. Our search resulted in the discovery of five photometrically classified, core-collapse supernovae with high re...

Browse Author Index

African Journals Online (AJOL)

Items 1 - 50 of 4028 ... Abdel-Gawad, E.I · Abdou, M · Abdul Rahim, R · Abdulla, NR · Abdullah, A.Y · Abdullah, AY · Abdullah, M · Abdulrazak, SA · Abed, F · Abegaz, S · Abegaz, S. Abel, S. Abin, S · Abiola, S.S · Aboagye, GS · Aboagye, S · Abou-Elewa, E · Abouheif, M A · Abouheif, M.A. · Abouheif, MA · Abrams, L · Absalan, M

Marketing Analysis and Strategy for a Small Business in the Beekeeping Industry.

Science.gov (United States)

1980-08-18

segment has opportunities associated with it that may be profitably 2Philip Kotler , " Marketing Management: Analysis, Planning, and Control," Prentice...I I I162 I I BIBLIOGRAPHY IB Abel, Derek and John Hammond. Strategic Market Planning. Englewood Cliffs, N.J.: Prentice- Hall, Inc., 1979. Kotler ...11I’ISTATIOY I I I I MARKETING ANALYSIS AND STRATEGY FOR A SMALL IBUSINESS IN THE BEEKEEPING INDUSTRY I III APPROVED: Acoession For DDC TABUn mounced or

Voyage dans le noir. Trous noirs, matière noire, énergie noire et antimatière

CERN Multimedia

CERN. Geneva; Alvarez-Gaume, Luis; Grojean, Christophe

2009-01-01

Et si nous faisions avec les physiciens un voyage dans le noir ? De l'astrophysique à la physique des particules les trois noirs, la matière noire, l'énergie noire ou l’antimatière intriguent et fascinent. Que sont ces objets qui bousculent nos idées et qui véhiculent parfois des craintes irraisonnées? Luis Alvarez-Gaume, Michael Doser et Christophe Grojean, physiciens du CERN vous invitent à mettre en lumière (!) les constituants de base de la matière et à explorer les mystères de la physique contemporaine. Une soirée lumineuse pour éclairer des concepts et ne plus avoir peur du noir.

Origin of amphibole-rich beach sands from Tila-Mati, Karwar, central-west coast of India

Digital Repository Service at National Institute of Oceanography (India)

Mislankar, P.G.; Iyer, S.D.

The pocket beach at Tila-Mati, Karwar, central west coast of India, is characterised by the occurrence of amphibole-rich (chiefly tremolite-actinolite) coarse sand in the zone of minimal impact of waves and currents. In the total sediment, grain...

On the distortion of properties of galaxy cluster

International Nuclear Information System (INIS)

Fesenko, B.I.

1979-01-01

The supposition is substantiated that most of Abell clusters with population of 50 and more members are false clusters. Some of them may contain, as peculiar nuclei, the real clusters with the number of members from ten to 25 within the range of apparent magnitudes from m 3 to m 3 +2, where m 3 is an apparent magnitude of the galaxy which is third in brightness. The rest members of false clusters are galaxies of front and rare backgrounds. The algorithm for galaxy cluster discrimination used by Abell is shown to promote selection of the real clusters with rho < approximately 25 in which region the number of the background galaxies is considerably increased as compared to other regions of the sky. A systematic and substantial underestimation of the role of such galaxies destorts the results of the cluster structures and dynamics analysis. False clusters are surprisingly well camouflaged as real clusters: when passing to more faint galaxies, the number of the seeming members grows faster than in the ambient field; the difference in angular diameters of false clusters distinctly reflects the difference in average distances of these galaxies; dispersion in velocity of false cluster members comparatively slightly depends on the average distance to an observer, and absolute magnitudes of the brightnesses of galaxies have small dispersion, as in real clusters

Inversion methods for analysis of neutron brightness measurements in tokamaks

International Nuclear Information System (INIS)

Gorini, G.; Gottardi, N.

1990-02-01

The problem of determining neutron emissivity from neutron brightness measurements in magnetic fusion plasmas is addressed. In the case of two-dimensional measurements with two orthogonal cameras, a complete, tomographic analysis of the data can in principle be performed. The results depend critically on the accuracy of the measurements and alternative solutions can be sought under the assumption of a known emissivity topology (Generalized Abel Inversion). In this work, neutron brightness data from the JET tokamak have been studied with both methods. We find that with the present experimental uncertainty (levels 10-20%) the Abel inversion method works best, while two-dimensional information cannot in general be deduced. This is confirmed by studies of the error propagation in the inversion using artificial data, which are also presented here. An important application of emissivity profile information is the determination of the plasma deuterium temperature profile, T D (R). Results are presented here from the analysis of JET data and the errors in T D (R) are discussed in some detail. It is found that, for typical JET plasma conditions, the dominant source of uncertainty arises from the high plasma impurity level and the fact that it is poorly known; these problems can be expected to be remedied and neutron brightness measurements would be expected to be very effective (especially in high density plasmas) as a T D (R) diagnostics. (author)

GASP. V. Ram-pressure stripping of a ring Hoag's-like galaxy in a massive cluster

Science.gov (United States)

Moretti, A.; Poggianti, B. M.; Gullieuszik, M.; Mapelli, M.; Jaffé, Y. L.; Fritz, J.; Biviano, A.; Fasano, G.; Bettoni, D.; Vulcani, B.; D'Onofrio, M.

2018-04-01

Through an ongoing MUSE program dedicated to study gas removal processes in galaxies (GAs Stripping Phenomena in galaxies with MUSE, GASP), we have obtained deep and wide integral field spectroscopy of the galaxy JO171. This galaxy resembles the Hoag's galaxy, one of the most spectacular examples of ring galaxies, characterized by a completely detached ring of young stars surrounding a central old spheroid. At odds with the isolated Hoag's galaxy, JO171 is part of a dense environment, the cluster Abell 3667, which is causing gas stripping along tentacles. Moreover, its ring counter-rotates with respect to the central spheroid. The joint analysis of the stellar populations and the gas/stellar kinematics shows that the origin of the ring was not due to an internal mechanism, but was related to a gas accretion event that happened in the distant past, prior to accretion on to Abell 3667, most probably within a filament. More recently, since infall in the cluster, the gas in the ring has been stripped by ram pressure, causing the quenching of star formation in the stripped half of the ring. This is the first observed case of ram-pressure stripping in action in a ring galaxy, and MUSE observations are able to reveal both of the events (accretion and stripping) that caused dramatic transformations in this galaxy.

Dynamical Friedel oscillations of a Fermi sea

Science.gov (United States)

Zhang, J. M.; Liu, Y.

2018-02-01

We study the scenario of quenching an interaction-free Fermi sea on a one-dimensional lattice ring by suddenly changing the potential of a site. From the point-of-view of the conventional Friedel oscillation, which is a static or equilibrium problem, it is of interest what temporal and spatial oscillations the local sudden quench will induce. Numerically, the primary observation is that for a generic site, the local particle density switches between two plateaus periodically in time. Making use of the proximity of the realistic model to an exactly solvable model and employing the Abel regularization to assign a definite value to a divergent series, we obtain an analytical formula for the heights of the plateaus, which turns out to be very accurate for sites not too close to the quench site. The unexpect relevance and the incredible accuracy of the Abel regularization are yet to be understood. Eventually, when the contribution of the defect mode is also taken into account, the plateaus for those sites close to or on the quench site can also be accurately predicted. We have also studied the infinite lattice case. In this case, ensuing the quench, the out-going wave fronts leave behind a stable density oscillation pattern. Because of some interesting single-particle property, this dynamically generated Friedel oscillation differs from its conventional static counterpart only by the defect mode.

Clusters of galaxies associated with quasars. I. 3C 206

International Nuclear Information System (INIS)

Ellingson, E.; Yee, H.K.C.; Green, R.F.; Kinman, T.D.

1989-01-01

Multislit spectroscopy and three-color CCD photometry of the galaxies in the cluster associated with the quasar 3C 206 (PKS 0837-12) at z = 0.198 are presented. This cluster is the richest environment of any low-redshift quasar observed in an Abell richness class 1 cluster. The cluster has a very flattened structure and a very concentrated core about the quasar. Most of the galaxies in this field have colors and luminosities consistent with normal galaxies at this redshift. The background-corrected blue fraction of galaxies is consistent with values for other rich clusters. The existence of several blue galaxies in the concentrated cluster core is an anomaly for a region of such high galaxy density, however, suggesting the absence of a substantial intracluster medium. This claim is supported by the Fanaroff-Riley (1974) class II morphology of the radio source. The velocity dispersion calculated from 11 spectroscopically confirmed cluster members is 500 + or - 110 km/s, which is slightly lower than the average for Abell class 1 clusters. A high frequency of interaction between the quasar host galaxy and cluster core members at low relative velocities, and a low intracluster gas pressure, may comprise a favorable environment for quasar activity. The properties of the cluster of galaxies associated with 3C 206 are consistent with this model. 59 refs

Criando Caim e Abel: pensando a prevenção da infração juvenil Raising Caim and Abel: thinking on juvenile delinquency prevention

Directory of Open Access Journals (Sweden)

Simone Gonçalves de Assis

1999-01-01

Full Text Available Este artigo é parte de uma pesquisa que envolveu adolescentes infratores e seus irmãos não infratores, realizada nas cidades do Rio de Janeiro e Recife. O principal objetivo foi o de conhecer os motivos que levam jovens a trilhar caminhos distintos, visando à prevenção da delinqüência juvenil. Foram incluídos casos de homicídio, assalto à mão armada, lesão corporal, estupro e atentado violento ao pudor e tráfico de drogas. A técnica de história de vida foi usada em entrevistas semi-estruturadas que foram aplicadas a 61 infratores e 31 não infratores. Nelas, buscou-se conhecer a sua realidade familiar, comunitária e social. A técnica de análise de conteúdo foi utilizada nas entrevistas. Foi feita ainda uma abordagem quantitativa dos dados (estudo de concordância e de associação de variáveis com o objetivo de identificar os fatores predisponentes à infração. No presente trabalho apresenta-se um modelo teórico explicativo da gênese da delinqüência juvenil e suas formas de prevenção; uma síntese dos achados qualitativos e quantitativos da pesquisa; e um ensaio de proposta para identificação dos fatores envolvidos na rede causal da infração cometida por adolescentes.This article is part of a research with juvenile delinquents and its siblings non delinquents. It was realized in the cities of Rio de Janeiro and Recife. It has the objective of studying the reasons that take young people to choose different roads, seeking the prevention of the juvenile delinquency. Cases of homicide, armed robbery, assault, rape and indecent act using force and drug traffic were included. The technique of life history was used in semi-structured interviews that were applied to 61 offenders and 31 non offenders. It stressed themes like family, community and social reality. The technique of content analysis was used in the interviews. It was still made a quantitative analysis of the data (agreement study and of association of variables with the objective of identifying the factors leading to the infraction. This article still presents an explanatory theoretical model of the genesis of juvenile delinquency and its prevention; a synthesis of the qualitative and quantitative results; and an attempt to identify which factors are involved in juvenile delinquency.

Number density measurements on analytical discharge systems: application of ''hook'' spectroscopy

Energy Technology Data Exchange (ETDEWEB)

Majidi, V.; Hsu, W.; Coleman, D.M.

1988-01-01

Various methods for determining atomic, ionic and electron number densities are reviewed. Time- and spatially-resolved number densities of sodium atoms in the post discharge environment of a high voltage spark are then quantitatively determined using the anomalous dispersion hook method. Number densities are calculated from hook separation near the Na D-lines. Lateral profiles are subsequently transformed to the radial domain using a derivative free Abel inversion process. Advantages, limitations, and practical ramification of the hook method are discussed.

Number density measurements on analytical discharge systems: application of ''hook'' spectroscopy

International Nuclear Information System (INIS)

Majidi, V.; Hsu, W.; Coleman, D.M.

1988-01-01

Various methods for determining atomic, ionic and electron number densities are reviewed. Time- and spatially-resolved number densities of sodium atoms in the post discharge environment of a high voltage spark are then quantitatively determined using the anomalous dispersion hook method. Number densities are calculated from hook separation near the Na D-lines. Lateral profiles are subsequently transformed to the radial domain using a derivative free Abel inversion process. Advantages, limitations, and practical ramification of the hook method are discussed. (author)

Supernovae in Low-Redshift Galaxy Clusters: Observations by the Wise Observatory Optical Transient Search (WOOTS)

OpenAIRE

Gal-Yam, Avishay; Maoz, Dan; Guhathakurta, Puragra; Filippenko, Alexei V.

2007-01-01

We describe the Wise Observatory Optical Transient Search (WOOTS), a survey for supernovae (SNe) and other variable and transient objects in the fields of redshift 0.06-0.2 Abell galaxy clusters. We present the survey design and data-analysis procedures, and our object detection and follow-up strategies. We have obtained follow-up spectroscopy for all viable SN candidates, and present the resulting SN sample here. Out of the 12 SNe we have discovered, seven are associated with our target clus...

Research on the penetration characteristic of supersonic molecule beam on the HL-1M tokamak

International Nuclear Information System (INIS)

Dong Jiafu; Luo Junling; Tang Nianyi; Li Wei; Zhong Yunze; Liu Yi; Fu Binzhong; Yao Lianghua; Feng Baibing; Qin Yunwen

2002-01-01

In the HL-1M plasma experiments, two refueling ways, the pellet injection and the gas puffing, are usually used. In recent years, a new refueling method, the supersonic molecular beam (SMB) injection, has been developed. In this paper, the penetration characteristics of SMB has been analyzed and researched. The SMB experiments were analyzed with H α emissivity measurement. The H α emissivity distribution in the plasma was calculated from multi-channel chord emission singles by means of the asymmetry Abel inversion method

Maorská kultura

OpenAIRE

Pirunčíková, Libuše

2008-01-01

This project is trying to get into Maori 's history, culture and conflicts of Maori's population. It describes inhabiting New Zealand by Moari, discovering these islands by Abel Janszoon Tasman and conflicts that came up during the conquering of New Zealand by European colonists, because of the diversity of both cultures. The important part of Maori's history includes war conflicts until mid 20's, when the renesaince of the falling culture started to happened. Since the end of the world war I...

Cuadernos de Antropología Social Nº 43

OpenAIRE

. .

2016-01-01

Cuerpo editorialEditores AsociadosCecilia Benedetti (coordinación editorial), Soledad Cutuli, María Guadalupe García, Mariana García Palacios, Julieta Infantino, Hernán Morel, Diego ZenobiCoordinación del DossierLena DavilaEvaluadores del NúmeroNacionalesLuis Abel Agüero, Universidad de Buenos AiresPatricia Arenas, Universidad Nacional de Tucumán Denis Baranger, Universidad Nacional de MisionesEmilio Crenzel, Universidad de Buenos AiresSergio Chamorro, Universidad Nacional de QuilmesMaría Eli...

Conference Digest - International Conference on Infrared and Millimeter Waves (13th) Held in Honolulu, Hawaii on 5-9 December 1988. Volume 1039.

Science.gov (United States)

1989-12-09

BY MICROSTRIP LINES - ERTIES OF GLASSES AND THE ENERGY TRANSFER TiROUGH S.T. Peng, NY Inst of Technology, Old Westbury, NY 11568; R.T. WINDOWS - R...Power is available from a Varian gyrotron oscillator design is an all-copper machined grating. The polarization in the TEo2 mode in 6.35-cm-diam...dielectric waveguide necessary. The Abel-inverted profile is shown in of *59 mm (Pyrex glass ). The laser beam is divided Fig.3(b). The measured density profile

Incidence des politiques en matière de publicité, de taxes et d ...

International Development Research Centre (IDRC) Digital Library (Canada)

Incidence des politiques en matière de publicité, de taxes et d'établissement des prix sur la consommation d'alcool (Argentine, Bolivie, Chili, Pérou). La consommation d'alcool ... Corruption in Latin America. This project will study private sector efforts to promote better compliance with anticorruption laws in Latin America.

La promotion du leadership en matière d'élaboration de politiques ...

International Development Research Centre (IDRC) Digital Library (Canada)

La promotion du leadership en matière d'élaboration de politiques économiques dans les États fragiles et dans les États d'après-conflit en Afrique. Ce projet fournit un financement de trois ans au Consortium pour la recherche économique en Afrique (AERC) afin de renforcer la capacité de recherche et d'analyse des ...

Innovation en matière de biocarburants sous le signe de l'inclusion ...

International Development Research Centre (IDRC) Digital Library (Canada)

Ce projet favorisera une innovation en matière de biocarburants qui prend en compte tous les acteurs pertinents, dont les femmes vivant en milieu rural. Les chercheurs ... Des chercheurs appuyés par le CRDI parlent de leurs expériences au Comité sur les ONG lors du forum de la Commission de la condition de la femme.

Mesures en matière de taxation des produits du tabac en Afrique de ...

International Development Research Centre (IDRC) Digital Library (Canada)

Mesures en matière de taxation des produits du tabac en Afrique de l'Ouest. En décembre 2007, le programme Recherche pour la lutte mondiale contre le tabac (RMCT) a entrepris une initiative afin de comprendre les facteurs cruciaux qui peuvent déterminer le succès de la lutte antitabac en Afrique subsaharienne.

Daimón: Jednota a protikladnost světa Lopeho de Aguirre

OpenAIRE

Janoušková, Petra

2011-01-01

The present work is focused on interpretation of the novel Daimón, written by Argentinian writer Abel Posse. It indicates the context of the "Latin America's new historical novel", comments the historical background of the story, touches the concept of time in the novel. Then the work analyses in detail the composition of the novel which is structured as a Tarot cards reading, explains the importance of the Tarot not only for interpretation of the Daimón novel, but also for understanding the ...

Deep multi-frequency rotation measure tomography of the galaxy cluster A2255

OpenAIRE

Pizzo, R. F.; de Bruyn, A. G.; Bernardi, G.; Brentjens, M. A.

2010-01-01

We aim to unveil their 3-dimensional geometry of Abell 2255 through WSRT observations at 18, 21, 25, 85, and 200 cm. The polarization images of the cluster were processed through rotation measure (RM) synthesis, producing three final RM cubes. The radio galaxies and the filaments at the edges of the halo are detected in the high-frequency RM cube, obtained by combining the data at 18, 21, and 25 cm. Their Faraday spectra show different levels of complexity. The radio galaxies lying near by th...

On the morphology of superclusters

International Nuclear Information System (INIS)

West, M.J.

1989-01-01

This paper explores the morphology of superclusters, focusing on the shapes and orientations of superclusters and possible alignments of the galaxy clusters which reside within them. A catalog of superclusters is generated using a simple procedure which uses available data on the three-dimensional distribution of Abell clusters. The results point toward a population of predominantly prolate superclusters with a moderate degree of flattening, with the galaxy clusters which reside within them exhibiting a clear tendency to be aligned over quite large distances. 99 refs

Partage des avantages découlant des améliorations en matière de ...

International Development Research Centre (IDRC) Digital Library (Canada)

Partage des avantages découlant des améliorations en matière de transport dans la grande sous-région du Mékong ... International Water Resources Association, in close collaboration with IDRC, is holding a webinar titled “Climate change and adaptive water management: Innovative solutions from the Global South”.

Certification of a second series of five hydrocarbon materials for the determination of equilibrium flashpoint (temperature ranges -10/sup 0/C to +5/sup 0/C and 80/sup 0/C to 135/sup 0/C)

Energy Technology Data Exchange (ETDEWEB)

Lewis, D J; Gonska, H; Karcher, W

1984-01-01

The closed cup flashpoints of five pure hydrocarbon materials (iso-octane, toluene, n-dodecane, n-tetradecane and n-hexadecane) have been determined by equilibrium methods in an interlaboratory exercise, involving twelve laboratories of the European Community member countries and one laboratory of the Commission of the European Communities. The methods used were based on IP303/74 (or ASTM D3278-73; Rapid Tester) and IP304/74 (Abel, Abel-Pensky, Pensky-Martens Cups) with extension to allow equilibrium conditions to be maintained outside the ranges of these methods. For each hydrocarbon material, the numbers of individual measurements accepted have been between 81 and 92. As a result, the closed cup flashpoints of these materials by an equilibrium method are certified at the following temperatures: CRM No. Hydrocarbon Equilibrium closed cup flashpoint 83 iso-octane -9.5 +- 0.5/sup 0/C 84 toluene +6.0 +- 0.5/sup 0/C 85 n-dodecane +81.0 +- 1.0/sup 0/C 86 n-tetradecane +108.0 +- 1.0/sup 0/C 87 n-hexadecane +133.5 +- 1.0/sup 0/C. This report describes the experimental details of the interlaboratory measurements and the certification procedure. The procedure required extensions to be made to methods IP303/74 and IP304/74 which are given in detail and recommendations are made for the improvement of these methods over the temperature range covered by the flashpoint reference materials.

HEAO A-1 observations of x ray emitting clusters of galaxies

International Nuclear Information System (INIS)

Johnson, M.W.

1990-01-01

Clusters of galaxies were known to be sources of x ray emission. Statistical analysis of how the x ray emission from clusters is related to other cluster properties was limited by the small number of clusters observed in the x ray region and the completeness of the x ray sample being considered. Both of these limitations are solved by producing a flux-limited catalog of x ray emitting Abell clusters of galaxies and using this catalog to investigate how the x ray emission correlates with other cluster properties. X ray data from the HEAO A-1 experiment were used to search for x ray emission from Abell clusters of galaxies. Selection criteria were chosen to ensure that the resulting catalog was complete and as free as possible from selection effects. The resulting identifications and x ray luminosities were used to check correlations with other cluster properties. Special consideration was given to observational selection effects and consistency checks. The data were consistent with all clusters of galaxies being x ray emitters beyond some limiting luminosity, which depends on cluster richness. Furthermore, the x ray luminosity of clusters is correlated with the richness of the cluster, its galaxy content, and the spacial distribution and galaxy content of galaxies within the cluster. It is concluded that the x ray emission from clusters of galaxies depends not only on the richness of the cluster but also the morphology of the cluster

Clusters of galaxies as tools in observational cosmology : results from x-ray analysis

International Nuclear Information System (INIS)

Weratschnig, J.M.

2009-01-01

Clusters of galaxies are the largest gravitationally bound structures in the universe. They can be used as ideal tools to study large scale structure formation (e.g. when studying merger clusters) and provide highly interesting environments to analyse several characteristic interaction processes (like ram pressure stripping of galaxies, magnetic fields). In this dissertation thesis, we have studied several clusters of galaxies using X-ray observations. To obtain scientific results, we have applied different data reduction and analysis methods. With a combination of morphological and spectral analysis, the merger cluster Abell 514 was studied in much detail. It has a highly interesting morphology and shows signs for an ongoing merger as well as a shock. using a new method to detect substructure, we have analysed several clusters to determine whether any substructure is present in the X-ray image. This hints towards a real structure in the distribution of the intra-cluster medium (ICM) and is evidence for ongoing mergers. The results from this analysis are extensively used with the cluster of galaxies Abell S1136. Here, we study the ICM distribution and compare its structure with the spatial distribution of star forming galaxies. Cluster magnetic fields are another important topic of my thesis. They can be studied in Radio observations, which can be put into relation with results from X-ray observations. using observational data from several clusters, we could support the theory that cluster magnetic fields are frozen into the ICM. (author)

Fascitis plantar

Directory of Open Access Journals (Sweden)

Dinorah Artidiello Bustio

2015-04-01

Full Text Available Introducción: la fascitis plantar es la inflamación del tejido denso que ocupa la parte anterior del tubérculo interno del calcáneo y constituye la causa más frecuente de dolor en la planta de los pies y dificulta en gran medida el desempeño laboral del individuo. Objetivo: caracterizar la fascitis plantar en pacientes asistidos en los servicios del Hospital General Docente "Abel Santamaría Cuadrado" en Pinar del Río. Material y método: estudio descriptivo, longitudinal y aplicado en el Departamento de Medicina Física y Rehabilitación del Hospital "Abel Santamaría Cuadrado", en el periodo comprendido desde abril del 2013 hasta abril del 2014, a los pacientes con diagnóstico de fascitis plantar. El universo coincidió con la muestra (60 pacientes. Resultados: de la muestra distribuida según ocupación laboral, 53 permanecen el mayor tiempo de pie, siendo el sexo femenino más predominante que el masculino y la edad promedio más afectada es de 40 a 49 años. El 70,0% de los pacientes mostraron dolor en las categorías de moderado a severo. Conclusiones: el sobrepeso y la obesidad crean un estrés adicional. Otro de los factores a considerar, son las neuropatías, el abuso del alcohol y el factor hereditario.

Subaru Weak Lensing Measurements of Four Strong Lensing Clusters: Are Lensing Clusters Over-Concentrated?

Energy Technology Data Exchange (ETDEWEB)

Oguri, Masamune; Hennawi, Joseph F.; Gladders, Michael D.; Dahle, Haakon; Natarajan, Priyamvada; Dalal, Neal; Koester, Benjamin P.; Sharon, Keren; Bayliss, Matthew

2009-01-29

We derive radial mass profiles of four strong lensing selected clusters which show prominent giant arcs (Abell 1703, SDSS J1446+3032, SDSS J1531+3414, and SDSS J2111-0115), by combining detailed strong lens modeling with weak lensing shear measured from deep Subaru Suprime-cam images. Weak lensing signals are detected at high significance for all four clusters, whose redshifts range from z = 0.28 to 0.64. We demonstrate that adding strong lensing information with known arc redshifts significantly improves constraints on the mass density profile, compared to those obtained from weak lensing alone. While the mass profiles are well fitted by the universal form predicted in N-body simulations of the {Lambda}-dominated cold dark matter model, all four clusters appear to be slightly more centrally concentrated (the concentration parameters c{sub vir} {approx} 8) than theoretical predictions, even after accounting for the bias toward higher concentrations inherent in lensing selected samples. Our results are consistent with previous studies which similarly detected a concentration excess, and increases the total number of clusters studied with the combined strong and weak lensing technique to ten. Combining our sample with previous work, we find that clusters with larger Einstein radii are more anomalously concentrated. We also present a detailed model of the lensing cluster Abell 1703 with constraints from multiple image families, and find the dark matter inner density profile to be cuspy with the slope consistent with -1, in agreement with expectations.

La face cachée de l’ancestralité. Masques et affinité chez les Matis d’Amazonie brésilienne

OpenAIRE

Erikson, Philippe

2009-01-01

La face cachée de l’ancestralité. Masques et affinité chez les Matis d’Amazonie brésilienne. Cet article montre en quoi les masques matis sont révélateurs des conceptions ouest amazoniennes de la temporalité et de la succession des générations. Après une discussion sur l’aspect cérémoniel des mascarades et sur les caractéristiques ontologiques imputées aux esprits mariwin, ce texte soutient que ces derniers, bien qu’associés aux morts du groupe et à des valeurs endogènes, représentent des aff...

Bilan des flux de matières particulaires et dissoutes du Sassandra à ...

African Journals Online (AJOL)

Ce travail a pour objectif l'estimation des apports du fleuve Sassandra. C'est dans ce cadre que les flux de matières particulaires et dissoutes ont été mesurés au cours de l'année 2003 sur le fleuve Sassandra, à la station hydrométrique de Gaoulou. La méthodologie adoptée a consisté à déterminer d'abord les ...

Imagen corporal en pacientes sometidos a cirug?a bari?trica

OpenAIRE

Vega Meza, Mar?a Paula

2017-01-01

La obesidad es un problema de salud que ha ido creciendo de manera considerable en los ?ltimos a?os, afectando a un alto porcentaje de la poblaci?n mundial (WHO, 2015). Uno de los tratamientos que m?s se emplea en la actualidad para tratar esta condici?n es la cirug?a bari?trica, la cual ha mostrado, hasta el momento, ser una de las t?cnicas m?s eficaces en cuanto a la p?rdida significativa del peso y el mantenimiento de los resultados (Abeles & Shikora, 2008). En ese orden, es pertinente ent...

Cuspidal discrete series for projective hyperbolic spaces

DEFF Research Database (Denmark)

Andersen, Nils Byrial; Flensted-Jensen, Mogens

2013-01-01

Abstract. We have in [1] proposed a definition of cusp forms on semisimple symmetric spaces G/H, involving the notion of a Radon transform and a related Abel transform. For the real non-Riemannian hyperbolic spaces, we showed that there exists an infinite number of cuspidal discrete series......, and at most finitely many non-cuspidal discrete series, including in particular the spherical discrete series. For the projective spaces, the spherical discrete series are the only non-cuspidal discrete series. Below, we extend these results to the other hyperbolic spaces, and we also study the question...

Radio observations of some clusters of galaxies at lambda=3.5 and 4 mm

International Nuclear Information System (INIS)

Efanov, V.A.; Zinchenko, I.I.; Kislyakov, A.G.; Krasil'nikov, A.A.; Kukina, E.P.; Moiseev, I.G.

1980-01-01

Millimeter radio observations with the 22-m Crimean antenna are reported for the central regions of the clusters of galaxies in Virgo, Hercules, and Coma Berenices, and from the cluster Abell 2199. In two of these, Coma and A2199, sources with a flux density of several jansky have been detected. The position of the source in A2199 matches that of the radio source 3C 338, but the object in the Coma cluster does not correspond to any known radio source. The nature of the emission from the new sources is discussed

[Calculation and analysis of arc temperature field of pulsed TIG welding based on Fowler-Milne method].

Science.gov (United States)

Xiao, Xiao; Hua, Xue-Ming; Wu, Yi-Xiong; Li, Fang

2012-09-01

Pulsed TIG welding is widely used in industry due to its superior properties, and the measurement of arc temperature is important to analysis of welding process. The relationship between particle densities of Ar and temperature was calculated based on the theory of spectrum, the relationship between emission coefficient of spectra line at 794.8 nm and temperature was calculated, arc image of spectra line at 794.8 nm was captured by high speed camera, and both the Abel inversion and Fowler-Milne method were used to calculate the temperature distribution of pulsed TIG welding.

Color-magnitude relations in nearby galaxy clusters

Science.gov (United States)

Rasheed, Mariwan A.; Mohammad, Khalid K.

2018-06-01

The rest-frame (g-r) /Mr color-magnitude relations of 12 Abell-type clusters are analyzed in the redshift range (0.02≲ z ≲ 0.10) and within a projected radius of 0.75 Mpc using photometric data from SDSS-DR9. We show that the color-magnitude relation parameters (slope, zero-point, and scatter) do not exhibit significant evolution within this low-redshift range. Thus, we can say that during the look-back time of z ˜ 0.1 all red sequence galaxies evolve passively, without any star formation activity.

Total-variation regularization with bound constraints

International Nuclear Information System (INIS)

Chartrand, Rick; Wohlberg, Brendt

2009-01-01

We present a new algorithm for bound-constrained total-variation (TV) regularization that in comparison with its predecessors is simple, fast, and flexible. We use a splitting approach to decouple TV minimization from enforcing the constraints. Consequently, existing TV solvers can be employed with minimal alteration. This also makes the approach straightforward to generalize to any situation where TV can be applied. We consider deblurring of images with Gaussian or salt-and-pepper noise, as well as Abel inversion of radiographs with Poisson noise. We incorporate previous iterative reweighting algorithms to solve the TV portion.

EK(b)P Keskkomitee VIII pleenumi stenogramm / tõlk. Mart Arold, tõlk. Jaan Isotamm

Index Scriptorium Estoniae

1999-01-01

EK(b)P Keskkomitee VIII pleenum, 21.-23. märts 1950. Sõnavõtud: N. Karotamm, P. Ponomarenko, I. Käbin, V. Kuusik, A. Jaanus, V. Hiznjakov, E. Ristimägi, I. Suija, H. Ajo, A. Meri, G. Abels, M. Assin, G. Latõshov, Rumjantsev, Müürisepp. Kommenteerinud Viktor Niitsoo. Algus: Akadeemia (1998) nr. 12, lk. 2655-2683 ; Järg nr.2;3;4;5;6;7;8;9;10 lk.415-446;639-670;863-894;1087-1118;1310-1342;1534-1566;1759-1790;2017-2048;2220-2256

A fast and accurate surface plasmon resonance system

Science.gov (United States)

Espinosa Sánchez, Y. M.; Luna Moreno, D.; Noé Arias, E.; Garnica Campos, G.

2012-10-01

In this work we propose a Surface Plasmon Resonance (SPR) system driven by Labview software which produces a fast, simple and accuracy measurements of samples. The system takes 2000 data in a range of 20 degrees in 20 seconds and 0.01 degrees of resolution. All the information is sent from the computer to the microcontroller as an array of bytes in hexadecimal format to be analyzed. Besides to using the system in SPR measurement is possible to make measurement of the critic angle, and Brewster angle using the Abeles method.

From nonlinear Schrödinger hierarchy to some (2+1)-dimensional nonlinear pseudodifferential equations

Science.gov (United States)

Yang, Xiao; Du, Dianlou

2010-08-01

The Poisson structure on CN×RN is introduced to give the Hamiltonian system associated with a spectral problem which yields the nonlinear Schrödinger (NLS) hierarchy. The Hamiltonian system is proven to be Liouville integrable. Some (2+1)-dimensional equations including NLS equation, Kadomtesev-Petviashvili I (KPI) equation, coupled KPI equation, and modified Kadomtesev-Petviashvili (mKP) equation, are decomposed into Hamilton flows via the NLS hierarchy. The algebraic curve, Abel-Jacobi coordinates, and Riemann-Jacobi inversion are used to obtain the algebrogeometric solutions of these equations.

From nonlinear Schroedinger hierarchy to some (2+1)-dimensional nonlinear pseudodifferential equations

International Nuclear Information System (INIS)

Yang Xiao; Du Dianlou

2010-01-01

The Poisson structure on C N xR N is introduced to give the Hamiltonian system associated with a spectral problem which yields the nonlinear Schroedinger (NLS) hierarchy. The Hamiltonian system is proven to be Liouville integrable. Some (2+1)-dimensional equations including NLS equation, Kadomtesev-Petviashvili I (KPI) equation, coupled KPI equation, and modified Kadomtesev-Petviashvili (mKP) equation, are decomposed into Hamilton flows via the NLS hierarchy. The algebraic curve, Abel-Jacobi coordinates, and Riemann-Jacobi inversion are used to obtain the algebrogeometric solutions of these equations.

Timothy Coombs: kriise tekib maailmas üha enam / intervjueerinud Kristel Abel

Index Scriptorium Estoniae

Coombs, Timothy

2013-01-01

Intervjuu riski- ja kriisikommunikatsiooni tippspetsialisti dr W. Timothy Coombsiga, kes räägib kriisikommunikatsiooni hetkeseisust ning jagab nõu, kuidas kriisikommunikatsiooniga toime tulla. Ta on välja arendanud situatsiooni kriisikommunikatsiooni teooria

Daamid poolpöördes : Paul Raua naisportreede taustast / Tiina Abel

Index Scriptorium Estoniae

Abel, Tiina

2008-01-01

Vendade Raudade loomingust sajandivahetusel ja nende erinevatest inspiratsiooniallikatest. Ka muutustest ühiskondlikus elus ja kultuuriteadvuses - pöördumine ühiskondlikult isiklikule ja psühholoogilisele, tegelikkuse ja indiviidi teadvuse ümbermõtestamine, ratsionaalse inimese asendumine tunnete ja instiktide inimesega - see ilmneb Paul Raua psühholoogilistes hingestatud naiseportreedes

EVALUASI RENCANA KINERJA KOLAM RETENSI (RETARDING BASIN DALAM UPAYA PENGENDALIAN BANJIR TUKAD MATI DI KOTA DENPASAR

Directory of Open Access Journals (Sweden)

I G. Suryadinata P

2013-03-01

Full Text Available Tukad Mati is one of the rivers in the province of Bali that unfolds and flows in Badung regency and Denpasar. Inundation due to flooding is a problem that often occurs in this region during the rainy season. In an effort to overcome problems of flooding have been many studies carried out so as to produce flood control alternatives such as normalization, diversion channels and retarding basins. Retarding basin is one of flood control alternative that has not been much studied. In this study conducted a simulation of flood prevention alternative with retarding basin at Tukad Mati, by the hydrology approach method and hydraulics using HEC-RAS 4.0 program applications. Simulations performed on the current river flow conditions (existing condition and to the existing conditions with the retarding basin, according to the detail design of retarding basin in the city of Denpasar and evaluate the effectiveness of the retarding basin in the river basin flood control of Tukad Mati. Flood control by retarding basin based on simulations with the 2 (two years flood return period, resulting in a reduction of water level by an average of 0.42 meters or an average of 12% of the maximum water level in the conditions without retarding basin, which occurred in along the grooves on the lower reaches of the retarding basin and inundation waters still occur in some places, particularly in the downstream of Umadui Dam. Economic analysis of both the analysis of Benefits/Cost produces a parameter of BCR, NPV and IRR are not meet the feasibility requirements. The effective retention of retarding basin based on simulation results are 282,630.00 m3 with the ability to flood accommodate for 3-4 hours. In terms of economic development retarding basin is not feasible in terms of comparative costs and benefits

EVALUASI RENCANA KINERJA KOLAM RETENSI (RETARDING BASIN DALAM UPAYA PENGENDALIAN BANJIR TUKAD MATI DI KOTA DENPASAR

Directory of Open Access Journals (Sweden)

I G. Suryadinata P

2013-01-01

Full Text Available Tukad Mati is one of the rivers in the province of Bali that unfolds and flows in Badung regency and Denpasar. Inundation due to flooding is a problem that often occurs in this region during the rainy season. In an effort to overcome problems of flooding have been many studies carried out so as to produce flood control alternatives such as normalization, diversion channels and retarding basins. Retarding basin is one of flood control alternative that has not been much studied. In this study conducted a simulation of flood prevention alternative with retarding basin at Tukad Mati, by the hydrology approach method and hydraulics using HEC-RAS 4.0 program applications. Simulations performed on the current river flow conditions (existing condition and to the existing conditions with the retarding basin, according to the detail design of retarding basin in the city of Denpasar and evaluate the effectiveness of the retarding basin in the river basin flood control of Tukad Mati. Flood control by retarding basin based on simulations with the 2 (two years flood return period, resulting in a reduction of water level by an average of 0.42 meters or an average of 12% of the maximum water level in the conditions without retarding basin, which occurred in along the grooves on the lower reaches of the retarding basin and inundation waters still occur in some places, particularly in the downstream of Umadui Dam. Economic analysis of both the analysis of Benefits/Cost produces a parameter of BCR, NPV and IRR are not meet the feasibility requirements. The effective retention of retarding basin based on simulation results are 282,630.00 m3 with the ability to flood accommodate for 3-4 hours. In terms of economic development retarding basin is not feasible in terms of comparative costs and benefits

Renforcement des capacités de réalisation d'essais en matière de ...

International Development Research Centre (IDRC) Digital Library (Canada)

Cette subvention soutiendra l'acquisition d'une expertise relativement aux essais en matière de prévention du VIH/sida au Botswana, en Tanzanie et en Zambie en mettant à profit des collaborations existant déjà entre des pays d'Afrique, le Canada et les États-Unis. Le Botswana-Tanzania-Zambia Capacity Building ...

L'harmonisation de la politique nationale en matière de S-T avec la ...

International Development Research Centre (IDRC) Digital Library (Canada)

Le Sri Lanka ne possède aucune politique officielle en matière de science et de technologie (S-T). Jusqu'à maintenant, les investissements en S-T ont été effectués de façon ponctuelle. Le gouvernement et les établissements de recherche et de développement (R-D) ont néanmoins reconnu que des investissements en S-T ...

Dynamique de transfert des matières organiques et inorganiques le long du continuum fluvial de la Garonne : impact de la retenue de Malause

OpenAIRE

Mamoudou, Mohamadou

2008-01-01

Les fleuves sont à l'origine des transferts de matières organiques et inorganiques des continents vers les océans. Ces matières peuvent être séparées par filtration (généralement à 0,45 ou 0,22µm) entre une phase particulaire et une phase dissoute. Le devenir des formes organiques va dépendre de leurs origines. Les formes labiles sont souvent rapidement minéralisées lors de leur transfert tandis que les formes réfractaires ont un comportement conservatif. Nous avons étudié la dynamique de tou...

Caracterización del comportamiento clínico-quirúrgico de la pancreatitis aguda en una unidad hospitalaria de Pinar del Río

Directory of Open Access Journals (Sweden)

Eduardo Rogelio García Noguera

2015-08-01

Full Text Available Introducción: la pancreatitis aguda es una enfermedad que produce diversos grados de inflamación en el órgano y puede llegar hasta la necrosis glandular. Objetivo: caracterizar el comportamiento clínico-quirúrgico en los pacientes con pancreatitis aguda en el Hospital General Docente "Abel Santamaría Cuadrado" de Pinar del Rio, en el periodo de 2009-2012. Material y método: se realizó una investigación observacional, descriptiva, longitudinal, retrospectiva, en pacientes con diagnóstico de pancreatitis aguda, ingresados en el Hospital General Docente "Abel Santamaría Cuadrado", de Pinar del Río, entre el 2009 y el 2012. Resultados: el 53,3% de los pacientes ingresó en el Servicio de Cirugía y el resto en la Unidad de Cuidados Intensivos. El 77,8% de los pacientes fueron intervenidos quirúrgicamente antes de transcurrir 48 horas desde el ingreso. Existió un predominio notable de enfermos complicados que ingresaron en las salas de cirugía, prevaleciendo en estos las complicaciones agudas o sistémicas. En los pacientes operados la mortalidad se elevó considerablemente un 42,1%. Conclusiones: para llevar a cabo una conducta adecuada en los pacientes ingresados con pancreatitis aguda, y de esta manera reducir las complicaciones y fallecimiento por esta causa, se deben ingresar desde el inicio en una sala de cuidados intensivos; además de incrementar el empleo de investigaciones como la TAC abdominal y disminuir los casos intervenidos quirúrgicamente.

RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey

Science.gov (United States)

Cerny, Catherine; Sharon, Keren; Andrade-Santos, Felipe; Avila, Roberto J.; Bradač, Maruša; Bradley, Larry D.; Carrasco, Daniela; Coe, Dan; Czakon, Nicole G.; Dawson, William A.; Frye, Brenda L.; Hoag, Austin; Huang, Kuang-Han; Johnson, Traci L.; Jones, Christine; Lam, Daniel; Lovisari, Lorenzo; Mainali, Ramesh; Oesch, Pascal A.; Ogaz, Sara; Past, Matthew; Paterno-Mahler, Rachel; Peterson, Avery; Riess, Adam G.; Rodney, Steven A.; Ryan, Russell E.; Salmon, Brett; Sendra-Server, Irene; Stark, Daniel P.; Strolger, Louis-Gregory; Trenti, Michele; Umetsu, Keiichi; Vulcani, Benedetta; Zitrin, Adi

2018-06-01

Strong gravitational lensing by galaxy clusters magnifies background galaxies, enhancing our ability to discover statistically significant samples of galaxies at {\\boldsymbol{z}}> 6, in order to constrain the high-redshift galaxy luminosity functions. Here, we present the first five lens models out of the Reionization Lensing Cluster Survey (RELICS) Hubble Treasury Program, based on new HST WFC3/IR and ACS imaging of the clusters RXC J0142.9+4438, Abell 2537, Abell 2163, RXC J2211.7–0349, and ACT-CLJ0102–49151. The derived lensing magnification is essential for estimating the intrinsic properties of high-redshift galaxy candidates, and properly accounting for the survey volume. We report on new spectroscopic redshifts of multiply imaged lensed galaxies behind these clusters, which are used as constraints, and detail our strategy to reduce systematic uncertainties due to lack of spectroscopic information. In addition, we quantify the uncertainty on the lensing magnification due to statistical and systematic errors related to the lens modeling process, and find that in all but one cluster, the magnification is constrained to better than 20% in at least 80% of the field of view, including statistical and systematic uncertainties. The five clusters presented in this paper span the range of masses and redshifts of the clusters in the RELICS program. We find that they exhibit similar strong lensing efficiencies to the clusters targeted by the Hubble Frontier Fields within the WFC3/IR field of view. Outputs of the lens models are made available to the community through the Mikulski Archive for Space Telescopes.

Initiatives canadiennes d'avant-garde en matière de systèmes de ...

International Development Research Centre (IDRC) Digital Library (Canada)

Initiatives canadiennes d'avant-garde en matière de systèmes de santé équitables et d'amélioration de la santé des mères et des enfants ... renforcement des systèmes de santé : d'une part, le recrutement des travailleurs de la santé, le maintien de cet effectif et, d'autre part, le rôle des systèmes d'information sur la santé.

Incidence des politiques en matière de publicité, de taxes et d ...

International Development Research Centre (IDRC) Digital Library (Canada)

Incidence des politiques en matière de publicité, de taxes et d'établissement des prix sur la consommation d'alcool (Argentine, Bolivie, Chili, Pérou). La consommation d'alcool dans les Amériques s'accompagne d'un coût considérable. En 2000, elle était à l'origine de 5 % des décès et de 9,7 % de la perte d'années de vie ...

Algebraic functions

CERN Document Server

Bliss, Gilbert Ames

1933-01-01

This book, immediately striking for its conciseness, is one of the most remarkable works ever produced on the subject of algebraic functions and their integrals. The distinguishing feature of the book is its third chapter, on rational functions, which gives an extremely brief and clear account of the theory of divisors.... A very readable account is given of the topology of Riemann surfaces and of the general properties of abelian integrals. Abel's theorem is presented, with some simple applications. The inversion problem is studied for the cases of genus zero and genus unity. The chapter on t

Correlación entre morfometría corneal y la ametropía en el LASEK

OpenAIRE

Rojas Álvarez, Eduardo; González Sotero, Janet

2014-01-01

Objetivo: establecer la correlación entre los cambios morfométricos corneales y la magnitud de la ametropía tratada hasta el año de cirugía corneal con láser de excímeros por la técnica LASEK. Métodos: se realizó una investigación observacional, descriptiva, longitudinal y prospectiva. La muestra quedó constituida por 56 pacientes (111 ojos) operados con LASEK en el Hospital «Abel Santamaría Cuadrado», en Pinar del Río, de noviembre de 2010 a junio de 2011. Se utilizó el microscopio confocal ...

Iguana iguana (Linnaeus 1758 (Squamata: Iguanidae

Directory of Open Access Journals (Sweden)

Aguilar-Kirigin, Alvaro

2011-05-01

Full Text Available Tres ejemplares fueron colectados en la República de Bolivia, y depositados en la Colección Boliviana de Fauna (CBF, La Paz, Bolivia. Los registros se realizaron en el Departamento de La Paz, Provincia Abel Iturralde, Sección Primera, Municipio Ixiamas. Localidad El Tigre, 11º58'15.7"S, 68º00'22.5"W; 162 msnm. Fecha de colecta: 11 julio 2010. Hora: 9:27 AM. Colectores: Alvaro J. Aguilar Kirigin y Wilson Bani Rivero. Colectado en bajíos herbáceos inundables, a orillas del río Madre de Dios.

Hydrodynamic aspects of selenium X-ray laser targets

Energy Technology Data Exchange (ETDEWEB)

Charatis, G; Busch, G E; Shepard, C L; Campbell, P M; Rosen, M D

1986-10-01

Recent experiments at KMS have been performed to investigate parameter variations of target component thickness, laser pulse duration and intensity, and one-sided vs two-sided irradiation in order to optimize the performance of the Livermore exploding foil selenium x-ray laser experiments. Preliminary experiments with selenium double foil targets were also conducted as a means of prolonging the duration and enlarging the spatial extent of the lasing conditions. Four-frame holographic interferometry was used in determining the time-dependence of density profiles obtained by Abel inversion of the interferometric fringe field and comparisons were made to LASNEX code calculations.

Lectures on Algebraic Geometry I

CERN Document Server

Harder, Gunter

2012-01-01

This book and the following second volume is an introduction into modern algebraic geometry. In the first volume the methods of homological algebra, theory of sheaves, and sheaf cohomology are developed. These methods are indispensable for modern algebraic geometry, but they are also fundamental for other branches of mathematics and of great interest in their own. In the last chapter of volume I these concepts are applied to the theory of compact Riemann surfaces. In this chapter the author makes clear how influential the ideas of Abel, Riemann and Jacobi were and that many of the modern metho

A uniform Tauberian theorem in dynamic games

Science.gov (United States)

Khlopin, D. V.

2018-01-01

Antagonistic dynamic games including games represented in normal form are considered. The asymptotic behaviour of value in these games is investigated as the game horizon tends to infinity (Cesàro mean) and as the discounting parameter tends to zero (Abel mean). The corresponding Abelian-Tauberian theorem is established: it is demonstrated that in both families the game value uniformly converges to the same limit, provided that at least one of the limits exists. Analogues of one-sided Tauberian theorems are obtained. An example shows that the requirements are essential even for control problems. Bibliography: 31 titles.

Clythrocerus carinatus Coelho, 1973 (Crustacea: Decapoda primer registro de una especie de la familia Tymolidae para el Caribe colombiano

Directory of Open Access Journals (Sweden)

Campos Néstor Hernando

1995-11-01

Full Text Available La subfamilia Tymolinae fue elevada recientemente a la categoría de familia, separándola de la Dorippidae, de acuerdo con lo expuesto por Wear & Batham (1975 y asumido por Bowman & Abele (1982 Y Williams (1984. La familia Tymolidae está constituida por un grupo de cangrejos, cercanos sistemáticamente a la familia Dromiacea, dentro de la que se destacan los del género Clythrocerus. A pesar de ser un grupo dedistribución tropical principalmente (Wear & Batam, 1975, no había sido registrada ninguna especie para el Caribe colombiano.

NMS Summer Student Programme at ISOLDE. LabVIEW readout of a gauge pressure meter for the VITO beam line. Atomic local studies in Graphene.

CERN Document Server

Valverde Mendez, Diana Sofia

2016-01-01

This document is a brief summary of my contributions to CERN during the NMS summer student program. My stay at CERN took place from the 27th of June until the 19th of August. During this time I collaborated in the Solid State Physics section of the nuclear research centre ISOLDE. I worked under the primary supervision of Dr. Torben Esmann Molholt and under Mr. Abel Da Silva Fenta as a second supervisor. Because of this I had two independent sets of tasks, so I will divide this report in two sections to address both collaborations individually.

A survey of high explosive-induced damage and spall in selected metals using proton radiography

International Nuclear Information System (INIS)

Holtkamp, D.B.; Clark, D.A.; Ferm, E.N.; Gallegos, R.A.; Hammon, D.; Hemsing, W.F.; Hogan, G.E.; Holmes, V.H.; King, N.S.P.; Lopez, R.P.; Merrill, F.E.; Morris, C.L.; Morley, K.B.; Murray, M.M.; Pazuchanics, P.D.; Prestridge, K.P.; Quintana, J.P.; Saunders, A.; Shinas, M.A.; Stacy, H.L.

2004-01-01

Multiple spall and damage layers can be created in metal when the free surface reflects a Taylor wave generated by high explosives. These phenomena have been explored in different thicknesses of several metals (tantalum, copper, 6061 T6-aluminum, and tin) using high-energy proton radiography. Multiple images (up to 21) can be produced of the dynamic evolution of damaged material on the microsecond time scale with a <50 ns 'shutter' time. Movies and multiframe still images of areal and (Abel inverted) volume densities are presented. An example of material that is likely melted on release (tin) is also presented

La reconstruction du passé anglo-écossais par les premiers historiens whigs de l’Union (1707)

OpenAIRE

Deschamps, Yannick

2018-01-01

À la différence des autres historiens de leur époque, Daniel Defoe (1660-1731), Abel Boyer (1667-1729) et Sir John Clerk of Penicuik (1676-1755) évoquent longuement les relations anglo-écossaises antérieures à l’Union de 1707. Whigs et unionistes, ces auteurs sont enclins à noircir le passé anglo-écossais préunioniste afin de mieux souligner la nécessité d’un rapprochement entre l’Angleterre et l’Écosse. S’ils tombent parfois dans les travers méthodologiques dénoncés par Herbert Butterfield, ...

An Assessment of Normalized Difference Skin Index Robustness in Aquatic Environments

Science.gov (United States)

2014-03-27

20 11 40 0. 56 0. 57 0. 58 0. 590 . 6 0. 61 0. 62 0. 63 W av el en gt h (n m ) Reflectance 0 m L 1. 07 m L 2. 14 m L 3. 21 m L 4. 28 m L 35 .7 1...thickness from water concentration profiles obtained with Raman spectroscopy”. Acta Dermato-Venereologica, 87(1):4–8, 2007. [10] Eismann, Michael T...confocal Raman spectroscopy”. Skin Research and Technology, 16(2):137–141, 2009. [35] Nunez, Abel S. “A physical model of human skin and its application

INDICIOS DEL PAPEL PREPONDERANTE DEL ÁLGEBRA EN LA EMERGENCIA DE LAS FUNCIONES ELÍPTICAS

Directory of Open Access Journals (Sweden)

LEONARDO SOLANILLA

2013-07-01

Full Text Available En el transcurso de un estudio sobre la emergencia del concepto de función elíptica en el siglo XIX hemos descubierto con sorpresa que el papel del Álgebra habría sido tanto, o quizás más importante, que el del mismo cálculo de las funciones complejas para el desenvolvimiento histórico de este campo de las Matemáticas. Para defender esta afirmación presentamos dos análisis. Uno de ellos se basa en las Recherches de Abel, el otro en los Fundamenta nova de Jacobi.

Some remarks on off-shell scattering in the eikonal approximation and applications to semi-inclusive reactions

International Nuclear Information System (INIS)

Rinat, A.S.; Taragin, M.F.

1997-01-01

Using the Abel inversion for the eikonal phase as function of the interaction we derive simple integral relations between half and on-shell eikonal phases. A frequently used short-range approximation for the half off-shell phase and profile appears supported by the above-mentioned relation. We work out some examples and also address the half off-shell eikonal phase pertinent to a diffractive amplitude. The latter is relevant for a calculation of selected transparencies T of nuclei for a proton, knocked-out in selected semi-inclusive A(e,e'p)X reactions. Some numerical results for T are given. (orig.)

Dark Matter Mystery Deepens in Cosmic "Train Wreck"

Science.gov (United States)

2007-08-01

Astronomers have discovered a chaotic scene unlike any witnessed before in a cosmic "train wreck" between giant galaxy clusters. NASA's Chandra X-ray Observatory and optical telescopes revealed a dark matter core that was mostly devoid of galaxies, which may pose problems for current theories of dark matter behavior. "These results challenge our understanding of the way clusters merge," said Dr. Andisheh Mahdavi of the University of Victoria, British Columbia. "Or, they possibly make us even reexamine the nature of dark matter itself." There are three main components to galaxy clusters: individual galaxies composed of billions of stars, hot gas in between the galaxies, and dark matter, a mysterious substance that dominates the cluster mass and can be detected only through its gravitational effects. Illustration of Abell 520 System Illustration of Abell 520 System Optical telescopes can observe the starlight from the individual galaxies, and can infer the location of dark matter by its subtle light-bending effects on distant galaxies. X-ray telescopes like Chandra detect the multimillion-degree gas. A popular theory of dark matter predicts that dark matter and galaxies should stay together, even during a violent collision, as observed in the case of the so-called Bullet Cluster. However, when the Chandra data of the galaxy cluster system known as Abell 520 was mapped along with the optical data from the Canada-France-Hawaii Telescope and Subaru Telescope atop Mauna Kea, HI, a puzzling picture emerged. A dark matter core was found, which also contained hot gas but no bright galaxies. "It blew us away that it looks like the galaxies are removed from the densest core of dark matter," said Dr. Hendrik Hoekstra, also of University of Victoria. "This would be the first time we've seen such a thing and could be a huge test of our knowledge of how dark matter behaves." Animation of Galaxy Cluster Animation of Galaxy Cluster In addition to the dark matter core, a

La politique criminelle en matière de violences conjugales : une évaluation des pratiques judiciaires et de leurs effets en termes de récidive

OpenAIRE

Vanneste, Charlotte

2016-01-01

La politique criminelle en matière de violences conjugales : une évaluation des pratiques judiciaires et de leurs effets en termes de récidive La recherche demandée par le Collège des Procureurs généraux visait à évaluer les pratiques judiciaires développées en matière de violences conjugales en application des directives de politique criminelle données par la circulaire COL 4/2006. Pour ce faire, les données statistiques relatives à l’ensemble des prévenus signalés au moins une fois aux ...

Genetic variability and heritability in cultivated okra [Abel moschus esculentus (L.) Moench

Energy Technology Data Exchange (ETDEWEB)

Nwangburuka, C. C.; Denton, O. A.; Khinde, O. B.; Ojo, D. K.; Popoola, A. R.

2012-11-01

Twenty-nine okra accessions from different agro-ecological regions in Nigeria were grown during the rainy and dry seasons, between 2006 and 2007 at Abeokuta (derived savanah) and Ilishan (rainforest) and assessed to determine their genetic variability, heritability and genetic advance from eight yield related characters. The experiment was laid out in a Randomized Complete Block Design with five replications. There was high genotypic coefficient of variability, % broad-sense heritability and genetic advance in traits such as plant height (26.2, 90.7, 51.5), fresh pod length (23.9, 98.5, 48.8), fresh pod width (23.9, 98.5, 48.8), mature pod length (28.6, 98.5, 52.3), branching per plant (29.3, 82.3, 54.8) and pod weight per plant (33.9, 90.0, 63.3), suggesting the effect of additive genes and reliability of selection based on phenotype of these traits for crop improvement. The positive and significant phenotypic and genotypic correlation between plant height at maturity, fresh pod width, seeds per pod and pods per plant, branches per plant with seed weight per plant and pod weight per plant, suggests that selection on the basis of the phenotype of these characters will lead to high seed and pod yield in okra. (Author) 26 refs.

VizieR Online Data Catalog: Spectra of Abell 2384 galaxies (Pranger+, 2014)

Science.gov (United States)

Pranger, F.; Bohm, A.; Ferrari, C.; Maurogordato, S.; Benoist, C.; Holler, H.; Schindler, S.

2014-09-01

The complementary EFOSC2 spectra and redshifts used are taken from the paper entitled "Merging history of three bimodal clusters" (authored by S. Maurogordato, J. L. Sauvageot, H. Bourdin, A. Cappi, C. Benoist, C. Ferrari, G. Mars and K. Houairi, published as A&A 525, A79 (2011A&A...525A..79M), DOI: 10.1051/0004-6361/201014415) and already available at CDS as Cat. J/A+A/525/A79 (2 data files).

Students with Disabilities Can Succeed! The Abell Report. Volume 26, No.7

Science.gov (United States)

Hettleman, Kalman R.

2013-01-01

The One Year Plus policy of Baltimore City Public Schools described in this Newsletter has the potential to breathe new life into "special education" for students with disabilities. In recent decades, many waves of K-12 education reform--including the No Child Left Behind Act, charter schools, alternative teacher recruitment paths,…

A GIANT RADIO HALO IN THE MASSIVE AND MERGING CLUSTER ABELL 1351

International Nuclear Information System (INIS)

Giacintucci, S.; Venturi, T.; Cassano, R.; Dallacasa, D.; Brunetti, G.

2009-01-01

We report on the detection of diffuse radio emission in the X-ray luminous and massive galaxy cluster A 1351 (z = 0.322) using archival Very Large Array data at 1.4 GHz. Given its central location, morphology, and Mpc-scale extent, we classify the diffuse source as a giant radio halo. X-ray and weak lensing studies show A 1351 to be a system undergoing a major merger. The halo is associated with the most massive substructure. The presence of this source is explained assuming that merger-driven turbulence may re-accelerate high-energy particles in the intracluster medium and generate diffuse radio emission on the cluster scale. The position of A 1351 in the log P 1.4GHz -log L X plane is consistent with that of all other radio-halo clusters known to date, supporting a causal connection between the unrelaxed dynamical state of massive (>10 15 M sun ) clusters and the presence of giant radio halos.

Fractal geometry of cosmic strings and correlations among galaxies and Abell clusters

International Nuclear Information System (INIS)

Pagels, H.R.

1987-01-01

In the context of the cosmic-string picture of galaxy and cluster formation we develop a model for the loop correlation function. Assuming that parent loops have dimension 1 and that the production of child loops cut off from the parent with a peculiar velocity v is described by a Brownian random walk we estimate for the fractal dimension of the correlations D = 1+3.28v 2 . For v≅0.24 this gives the observed fractal D≅1.2

Riiast kulda toomas ehk tähelepanekuid Balti kommunikatsiooniauhindade jagamisest / Kristel Abel

Index Scriptorium Estoniae

Abel, Kristel, 1974-

2017-01-01

Märtsi algul Riias peetud üritusel "Mi:t&Links Baltic Communication Awards 2017" jagati kommunikatsiooniauhindu. Võistlusel esile tõusnud projektidest. Strateegilisele mõtlemisele pühendatud konverentsist

The GenABEL Project for statistical genomics [version 1; referees: 2 approved

NARCIS (Netherlands)

L.C. Karssen (Lennart); C.M. van Duijn (Cornelia); Y.S. Aulchenko (Yurii)

2016-01-01

textabstractDevelopment of free/libre open source software is usually done by a community of people with an interest in the tool. For scientific software, however, this is less often the case. Most scientific software is written by only a few authors, often a student working on a thesis. Once the

Why Can't Johnny Read? The Abell Report. Volume 23, No.7

Science.gov (United States)

Jacobson, Joan

2010-01-01

Baltimore's school-based vision-screening program may be leaving thousands of children with uncorrected eyesight problems. Vision screening in public schools is essential for students to learn, especially when low-income children face a high rate of eyesight problems and have poor access to health care. Left undetected and uncorrected, vision…

Experimental evaluation of analyte excitation mechanisms in the inductively coupled plasma

International Nuclear Information System (INIS)

Lehn, Scott A.; Hieftje, Gary M.

2003-01-01

The inductively coupled plasma (ICP) is a justifiably popular source for atomic emission spectrometry. However, despite its popularity, the ICP is still only partially understood. Even the mechanisms of analyte excitation remain unclear; some energy levels are quite clearly populated by charge transfer while others might be populated by electron-ion recombination, by electron impact, or by Penning processes. Distinguishing among these alternatives is possible by means of a steady-state kinetics approach that examines correlations between the emission of a selected atom, ion, or level and the local number densities of species assumed to produce the excitation. In an earlier investigation, strong correlations were found between either calcium atom or ion emission and selected combinations of calcium atom or ion number densities and electron number densities in the plasma. However, all radially resolved data employed in the earlier study were produced from Abel inversion and from measurements that were crude by today's standards. Now, by means of tomographic imaging, laser-saturated atomic fluorescence, and Thomson and Rayleigh scattering, it is possible to measure the required radially resolved data without Abel inversion and with far greater fidelity. The correlations previously studied for calcium have been investigated with these more reliable data. Ion-electron recombination, either radiative or with argon as a third body, was determined to be the most likely excitation mechanism for calcium atom, while electron impact appeared to be the most important process to produce excite-state calcium ions. These results were consistent with the previous study. However, the present study suggests that collisional deactivation, rather than radiative decay, is the most likely mode of returning both calcium atoms and ions to the ground state

Sophus Lie une pensée audacieuse

CERN Document Server

Stubhaug, Arild

2006-01-01

Sophus Lie (1842-1899) compte parmi les plus grandes figures norvgiennes de la science. La notorit que lui valent ses travaux n'a rien envier celle de son illustre compatriote Niels Henrik Abel. Groupes et alg bres de Lie ont acquis droit de cit dans maints domaines. Dans cette biographie dtaille, l'crivain Arild Stubhaug, puisant dans la volumineuse correspondance de Lie, dcrit l'homme et la socit norvgienne dans la seconde moiti du XIXe si cle. Le lecteur peut ainsi suivre son enfance dans un presbyt re nich au fond d'un fjord, dcouvrir les rformes de l'enseignement, voyager en Europe, frque

Consommation d’alcool et culture masculine dans l’Europe de l’époque moderne

OpenAIRE

Tlusty, B. Ann

2018-01-01

Pourquoi les gens buvaient-ils à l’époque moderne ? Mathias von Abele, un juriste allemand du xviie siècle, relève au moins quarante-cinq bonnes raisons de le faire, au nombre desquelles on peut citer l’amitié, l’honneur, la vertu, la bravoure, la virilité, les affaires et le commerce, sans oublier le plaisir de la dégustation et une agréable compagnie ; la rancœur et la mauvaise humeur, l’envie, la défiance, l’ennui et l’oisiveté sont également des motifs tout aussi impérieux. Le vocabulaire...

Symposium Introduction: Papers on 'Modeling National Health Expenditures'.

Science.gov (United States)

Getzen, Thomas E; Okunade, Albert A

2017-07-01

Significant contributions have been made since the World Health Organization published Brian Abel-Smith's pioneering comparative study of national health expenditures more than 50 years ago. There have been major advances in theories, model specifications, methodological approaches, and data structures. This introductory essay provides a historical context for this line of work, highlights four newly published studies that move health economics research forward, and indicates several important areas of challenging but potentially fruitful research to strengthen future contributions to the literature and make empirical findings more useful for evaluating health policy decisions. Copyright © 2016 John Wiley & Sons, Ltd. Copyright © 2016 John Wiley & Sons, Ltd.

Análise cladística das abelhas do gênero Augochloropsis cockerell, 1897 (Hymenoptera:Apidae s.l.:Augochlorini)

OpenAIRE

Santos, Leandro Mattos

2014-01-01

Resumo: O gênero de abelhas Augochloropsis Cockerell, 1897 é o táxon mais diverso dentre os Augochlorini, com 146 espécies válidas, sendo a maioria descrita do ínicio até a metade do século vinte. Após este período pouco foi feito em referência à taxonomia e sistemática do gênero que nunca foi revisado e sua classificação é instável em relação aos subgêneros: Augochloropsis s.str., A. (Glyptobasia) Moure, 1941, A. (Glyptochlora) Moure, 1958 e A. (Paraugochloropsis) Schrottky, 1906. Estas abel...

The necessity of conflict resolving in the contemporary world

Directory of Open Access Journals (Sweden)

Krel Aleksandar

2015-01-01

Full Text Available Whether collective or among individuals, conflicts between people are their doom, their fate and represent their dark side. Many people are marked by this ill fate, in a similar way as Cain was imprinted by the seal for the murder of his own brother. This well-known story from the Old Testament of Cain and Abel tells us about the basic matrix of every human conflict: emerged out of jealousy and various other problems, a conflict situation arises between the two sides, whereas the parties involved are not able to overcome it, and in time, this situation grows into an open conflict ending up in a tragedy.

Exact Solutions for Certain Nonlinear Autonomous Ordinary Differential Equations of the Second Order and Families of Two-Dimensional Autonomous Systems

Directory of Open Access Journals (Sweden)

M. P. Markakis

2010-01-01

Full Text Available Certain nonlinear autonomous ordinary differential equations of the second order are reduced to Abel equations of the first kind ((Ab-1 equations. Based on the results of a previous work, concerning a closed-form solution of a general (Ab-1 equation, and introducing an arbitrary function, exact one-parameter families of solutions are derived for the original autonomous equations, for the most of which only first integrals (in closed or parametric form have been obtained so far. Two-dimensional autonomous systems of differential equations of the first order, equivalent to the considered herein autonomous forms, are constructed and solved by means of the developed analysis.

Axially symmetric reconstruction of plasma emission and absorption coefficients

International Nuclear Information System (INIS)

Yang Lixin; Jia Hui; Yang Jiankun; Li Xiujian; Chen Shaorong; Liu Xishun

2013-01-01

A layered structure imaging model is developed in order to reconstruct emission coefficients and absorption coefficients simultaneously, in laser fusion core plasma diagnostics. A novel axially symmetric reconstruction method that utilizes the LM (Levenberg-Marquardt) nonlinear least squares minimization algorithm is proposed based on the layered structure. Numerical simulation results demonstrate that the proposed method is sufficiently accurate to reconstruct emission coefficients and absorption coefficients, and when the standard deviation of noise is 0.01, the errors of emission coefficients and absorption coefficients are 0.17, 0.22, respectively. Furthermore, this method could perform much better on reconstruction effect compared with traditional inverse Abel transform algorithms. (authors)

Differential and complex geometry origins, abstractions and embeddings

CERN Document Server

Wells, Jr , Raymond O

2017-01-01

Differential and complex geometry are two central areas of mathematics with a long and intertwined history. This book, the first to provide a unified historical perspective of both subjects, explores their origins and developments from the sixteenth to the twentieth century. Providing a detailed examination of the seminal contributions to differential and complex geometry up to the twentieth century embedding theorems, this monograph includes valuable excerpts from the original documents, including works of Descartes, Fermat, Newton, Euler, Huygens, Gauss, Riemann, Abel, and Nash. Suitable for beginning graduate students interested in differential, algebraic or complex geometry, this book will also appeal to more experienced readers.

Radio investigations of clusters of galaxies

International Nuclear Information System (INIS)

Valentijn, E.A.

1978-01-01

This thesis contains a number of papers of the series entitled, A Westerbork Survey of Rich Clusters of Galaxies. The primary aim was to study the radio characteristics of cluster galaxies and especially the question whether their ''radio-activity'' is influenced by their location inside a cluster. It is enquired whether the presence of an intra-cluster medium (ICM), or the typical cluster evolution or cluster dynamical processes can give rise to radio-observable effects on the behaviour of cluster galaxies. 610 MHz WSRT observations of the Coma cluster (and radio observations of the Hercules supercluster) are presented. Extended radio sources in Abell clusters are then described. (Auth.)

The origin of cosmic gamma-ray bursts

International Nuclear Information System (INIS)

Van den Bergh, S.

1983-01-01

The positions of 46 γ-ray burst sources on the sky are used to show that the majority of these objects either originate in very distant regions with redshifts > or approx. 30 000 km s -1 or within < or approx. 0.5β of the Sun; where β is the scale-height of the parent population perpendicular to the galactic disc. An origin of the majority of γ-ray bursts in the more distant parts of the galactic disc, the galactic nuclear bulge, the Virgo supercluster, in galaxies with msub(pg) < 18 and rich in Abell clusters of distance classes 0 to 4 is excluded by the data. (orig.)

Primordial inhomogeneities in the expanding universe. I - Density and velocity distributions of galaxies in the vicinities of rich clusters

Science.gov (United States)

Silk, J.; Wilson, M. L.

1979-01-01

The density profiles and Hubble flow deviations in the vicinities of rich galaxy clusters are derived for a variety of models of initial density and velocity perturbations at the recombination epoch. The galaxy correlation function, measured with respect to the Abell clusters, is used to normalize the theoretical models. The angular scales of the required primordial inhomogeneities are calculated. It is found that the resulting density profiles around rich clusters are surprisingly insensitive to the shape of the initial perturbations and also to the cosmological density parameter, Omega. However, it is shown that the distribution of galaxy radial velocities can provide a possible means of deriving Omega.

éphémérides ou biographie sommaire de Savinien de Cyrano de Bergerac

Directory of Open Access Journals (Sweden)

Madeleine Alcover

2010-02-01

Full Text Available Biographie15519 avril : mariage, à Paris, des grands-parents paternels de l’écrivain, Savinien I de Cyrano et Anne Le Maire : celle-ci est la petite-fille d’Étienne Cardon, marchand parisien. À ce jour, l’origine du grand-père paternel n’est pas résolue (sarde ? descendant d’un marchand bourrelier de Sens ?.1555Le couple signe une donation entre vifs qui, en cas de décès, fait du survivant son légataire universel. Quatre enfants leur survivront : Abel, Samuel, Pierre et Anne.1555-1560Savinie...

Spécialiste de la sécurité en matière de TI (h/f) | CRDI - Centre de ...

International Development Research Centre (IDRC) Digital Library (Canada)

Pour ce faire, le spécialiste de la sécurité en matière de TI sera appelé de temps ... techniques dans les régions et des techniciens sous contrat) pour fournir des ... en oeuvre et à la maintenance des éléments d'infrastructure, en surveillant les ...

Recherche de marqueurs lipidiques aptes à montrer l’absence de tissus nerveux dans les matières premières des gélatines d’os

Directory of Open Access Journals (Sweden)

Combe Nicole

2002-09-01

Full Text Available La gélatine est fabriquée à partir de deux catégories de matières premières, dénommées « os lourds » et « os légers », obtenues après dégraissage, séchage, broyage, puis tamisage d’os frais de bœuf, à l’exclusion de matériaux à risques vis-à-vis de l’encéphalopathie spongiforme bovine (cerveaux, yeux, amygdales et moelle épinière. L’objectif de cette étude était d’identifier un ou plusieurs constituants lipidiques spécifiques des tissus nerveux, et principalement de la moelle épinière, permettant de vérifier l’absence de tissus nerveux dans les matières premières utilisées pour la fabrication de gélatine. Pour cela, la composition lipidique de la moelle épinière a été comparée à celle des matières premières de gélatine. La pertinence d’un paramètre (p, vis-à-vis d’une source donnée, a été évaluée par la valeur du facteur : F (p = [p]moelle épinière/[p] OS, qui est le rapport entre sa concentration dans les lipides de moelle épinière et celle dans la source osseuse considérée. Plus la valeur de F est élevée, plus le paramètre est pertinent. Trois paramètres ont été ciblés sur la base de leur caractère spécifique des tissus nerveux par rapport aux graisses d’os : (1 les phospholipides (PL; (2 les acides gras à très longues chaînes (AGTLC = 20:0 + 20:1 + 22:0 + 22:1 n-9 + 23:0 + 24:0 + 24:1 n-9 ; (3 les alcools gras, analysés sous la forme de dérivés diméthyl acétals (DMA. Eu égard aux matières premières servant à la fabrication de gélatine, la valeur de FPL varie de 8 à 15, celle de FAGTLC de 25 à 41. La valeur de FDMA est égale à 26 vis-à-vis des « os légers », elle est infiniment grande vis-à-vis des « os lourds » puisque, dans cette matière première, les DMA sont indétectables. Ainsi pour cette catégorie de matière première, le paramètre DMA s’avère le plus adapté pour détecter du matériel d’origine nerveuse (moelle épinière.

Paciente obstétrica críticamente enferma Critically-ill obstetric patient

Directory of Open Access Journals (Sweden)

Jorge M Balestena Sánchez

2004-04-01

Full Text Available Con la finalidad de identificar algunos factores que inciden en la morbilidad puerperal grave, se realizó una investigación retrospectiva, transversal y analítica en el Hospital Universitario "Abel Santamaría Cuadrado" durante el año 2002. El universo de nuestro estudio se conformó con todas las puérperas del período analizado, mientras que el grupo estudio estuvo formado por las puérperas que tuvieron una mortalidad grave; para la comparación se escogió otro grupo integrado por puérperas sin morbilidad de forma aleatoria simple. El análisis estadístico se realizó por el porciento, la media, la desviación estándar y la prueba de hipótesis de proporciones para dos muestras independientes con nivel de significación de p Aimed at identifying some factors which influence on severe puerperal morbidity a retrospective, cross-sectional and analytic research was carried out at Abel Santamaria Teaching General Hospital during year 2002. The universe of the study was constituted by all the puerperal during this period while the case control group was formed by puerperal having a severe morbidity, to the comparison a group formed by post _ puerperal without morbidity was chosen at random. The statistical analysis was conducted by the percentage mean, standard deviation and proportional hypothesis testing to two independent samples with the significance testing of p < 0.05. a positive relationship among the adolescence, old puerperal, multigravid, multipara, delayed delivery and cesarean section with severe puerperal morbidity was achieved. Sepsis was the most frequent morbidity, concluding that the variables analyzed above were the risk factors which lead to severe morbid process of puerperium.

Generalized Uncertainty Quantification for Linear Inverse Problems in X-ray Imaging

Energy Technology Data Exchange (ETDEWEB)

Fowler, Michael James [Clarkson Univ., Potsdam, NY (United States)

2014-04-25

In industrial and engineering applications, X-ray radiography has attained wide use as a data collection protocol for the assessment of material properties in cases where direct observation is not possible. The direct measurement of nuclear materials, particularly when they are under explosive or implosive loading, is not feasible, and radiography can serve as a useful tool for obtaining indirect measurements. In such experiments, high energy X-rays are pulsed through a scene containing material of interest, and a detector records a radiograph by measuring the radiation that is not attenuated in the scene. One approach to the analysis of these radiographs is to model the imaging system as an operator that acts upon the object being imaged to produce a radiograph. In this model, the goal is to solve an inverse problem to reconstruct the values of interest in the object, which are typically material properties such as density or areal density. The primary objective in this work is to provide quantitative solutions with uncertainty estimates for three separate applications in X-ray radiography: deconvolution, Abel inversion, and radiation spot shape reconstruction. For each problem, we introduce a new hierarchical Bayesian model for determining a posterior distribution on the unknowns and develop efficient Markov chain Monte Carlo (MCMC) methods for sampling from the posterior. A Poisson likelihood, based on a noise model for photon counts at the detector, is combined with a prior tailored to each application: an edge-localizing prior for deconvolution; a smoothing prior with non-negativity constraints for spot reconstruction; and a full covariance sampling prior based on a Wishart hyperprior for Abel inversion. After developing our methods in a general setting, we demonstrate each model on both synthetically generated datasets, including those from a well known radiation transport code, and real high energy radiographs taken at two U. S. Department of Energy

Presentación de un estudio en 680 pacientes operados de terceros molares retenidos

Directory of Open Access Journals (Sweden)

Felicia Morejón Álvarez

2000-08-01

Full Text Available Se realizó un estudio en 680 pacientes operados de terceros molares retenidos que fueron atendidos en el Servicio de Cirugía Maxilofacial del Hospital Docente Clinicoquirúrgico "Abel Santamaría" en el período comprendido entre el 6 de octubre de 1998 y el 6 de octubre de 1999, con el objetivo de determinar las complicaciones posoperatorias más frecuentes encontradas en los pacientes operados. Se plantean y analizan los resultados obtenidos y se establecen comparaciones con estudios anteriores. El procedimiento quirúrgico de los terceros molares retenidos constituye una de las actividades operatorias más frecuentes dentro del marco de la cirugía maxilofacial, y a partir de la cual pueden aparecer complicaciones que exigen su diagnóstico oportuno y tratamiento. Como complicaciones posoperatorias más frecuentes se encontraron la alveolitis en el 29,6 %, la celulitis facial posquirúrgica en el 22,7 %, la hemorragia en el 18,2 % y el trismo mandibular, en el 13,7 % de los casos.680 patients who were operated on of impacted third molars at the Maxillofacial Surgery Service of "Abel Santamaría" Clinical and Surgical Teaching Hospital, between October 6, 1998, and October 6, 1999, were studied aimed at determining the most frequent postoperative complications found in the operated on patients.The results obtained were analyzed and compared with those of previous studies. The surgical procedure of the impacted third molars is one of the commonest surgical activities within the framework of maxillofacial surgery. Complications needing a suitable diagnosis and treatment may appear. The most frequent postoperative complications are alveolitis in 29.6%, postsurgical facial cellulitis in 22.7%, hemorrhage in 18.2% and mandibular trismus in 13.7% of the cases.

The rates and time-delay distribution of multiply imaged supernovae behind lensing clusters

Science.gov (United States)

Li, Xue; Hjorth, Jens; Richard, Johan

2012-11-01

Time delays of gravitationally lensed sources can be used to constrain the mass model of a deflector and determine cosmological parameters. We here present an analysis of the time-delay distribution of multiply imaged sources behind 17 strong lensing galaxy clusters with well-calibrated mass models. We find that for time delays less than 1000 days, at z = 3.0, their logarithmic probability distribution functions are well represented by P(log Δt) = 5.3 × 10-4Δttilde beta/M2502tilde beta, with tilde beta = 0.77, where M250 is the projected cluster mass inside 250 kpc (in 1014M⊙), and tilde beta is the power-law slope of the distribution. The resultant probability distribution function enables us to estimate the time-delay distribution in a lensing cluster of known mass. For a cluster with M250 = 2 × 1014M⊙, the fraction of time delays less than 1000 days is approximately 3%. Taking Abell 1689 as an example, its dark halo and brightest galaxies, with central velocity dispersions σ>=500kms-1, mainly produce large time delays, while galaxy-scale mass clumps are responsible for generating smaller time delays. We estimate the probability of observing multiple images of a supernova in the known images of Abell 1689. A two-component model of estimating the supernova rate is applied in this work. For a magnitude threshold of mAB = 26.5, the yearly rate of Type Ia (core-collapse) supernovae with time delays less than 1000 days is 0.004±0.002 (0.029±0.001). If the magnitude threshold is lowered to mAB ~ 27.0, the rate of core-collapse supernovae suitable for time delay observation is 0.044±0.015 per year.

Efectividad de la acupuntura en la crisis aguda de asma bronquial

Directory of Open Access Journals (Sweden)

María Teresa Paz Rodríguez

2014-10-01

Full Text Available Introducción: el asma bronquial es una enfermedad respiratoria con significativa prevalencia y una de las principales causas de ingreso hospitalario y la acupuntura una forma terapéutica de la Medicina Tradicional y Natural con múltiples indicaciones, dentro de ellas esta afección. Objetivo: determinar la evolución de los pacientes asmáticos persistentes moderados de ambos sexos antes y después del tratamiento con acupuntura en el servicio de urgencia en el Hospital General Docente Abel Santamaría Cuadrado de Pinar del Río. Material y método: se realizó un estudio de intervención, prospectivo, longitudinal, utilizando la acupuntura como modalidad terapéutica de la Medicina Tradicional China en pacientes que acudieron al cuerpo de guardia de Medicina Interna del Hospital General Docente "Abel Santamaría Cuadrado" de Pinar del Rio, en el período comprendido entre octubre-diciembre del 2013. El universo lo integraron todos los pacientes que acudieron a la consulta con crisis aguda de asma bronquial (223 y la muestra, 83 pacientes clasificados como asmáticos persistentes moderados utilizándose acupuntura en los puntos pulmón 7, vaso concepción 17 y vejiga 13 al grupo de estudio (41 pacientes y 42 con tratamiento convencional. Resultados: al tratar estos pacientes se ha evidenciado que el 78,4% de ellos mejoró por la aplicación de este método milenario. Ninguno presentó complicaciones y sólo 11 pacientes no mejoraron. Conclusiones: los pacientes respondieron de igual forma al tratamiento sin distinción de edad y sexo, demostrando este método ser eficiente, de fácil aplicación con aparición de menos reacciones adversas y además, económico.

Infección nosocomial en la terapia intensiva neonatal. Factores de riesgo. Pinar del Río 2001-2003 Nosocomial infection in the neonatal intensive care unit. Risk factors, Pinar del Río

Directory of Open Access Journals (Sweden)

Ivón Aimé Sánchez Monterrey

2007-03-01

Full Text Available Con el objetivo de evaluar los factores de riesgo de las infecciones nosocomiales en la Unidad de Terapia Intensiva Neonatal del Hospital General Universitario "Abel Santamaría Cuadrado" de Pinar del Río, se realizó una investigación observacional, analítica, de tipo caso-control, para ello se estudiaron 170 niños ingresados en esta unidad en el período comprendido de abril de 2001 a diciembre de 2003. Se recogió en una planilla tipo y momento de adquisición de la infección, abordaje vascular, ventilación mecánica y gérmenes aislados, entre otros. Se elaboró una base de datos en Microsoft Excel-97, se aplicaron los Test de Chi cuadrado y test de Student, ambos con un intervalo de confianza de p With the purpose of evaluating risk factors of nosocomial infections in the Intensive Care Unit of the "Abel Santamaría Cuadrado" General Hospital in Pinar del Río, an observational, analytical and a case-control research was performed in 170 children admitted at this Unit from April 1st., 2001, to December 31st., 2003. The nosocomial infection and time of being infected were recorded in a form, as well as the vascular approach, artificial ventilation and isolated germs, among others. A data base using the Microsoft Excel 97 software was designed, and chi-square test was used, both of them with a confidence interval of p<0,05. It was observed that birth weight, sex, gestational age, stay at ICU, artificial ventilation and deep vascular approach were related significantly with the onset of the nosocomial infection versus a control group showing similar characteristics. E. Coli and negative coagulase were the most frequent isolated germs.

Indicadores en adolescentes con ingresos de recién nacidos en cuidados especiales neonatales Indicators of adolescent mothers having newborn infants admitted to Neonatal Intensive Care Unit

Directory of Open Access Journals (Sweden)

Nuvia Suárez Garcia

2013-02-01

Full Text Available Introducción: el embarazo en adolescentes constituye un indicador negativo de salud ocasionando serias consecuencias materno- infantiles. Objetivo: evaluar indicadores materno-perinatales y neonatales en adolescentes atendidos en el Hospital "Abel Santamaría Cuadrado" durante el 2010. Métodos: se realizó una investigación aplicada, observacional, analítica, retrospectiva tipo caso-control, cuyo universo englobó 5363 nacimientos vivos en el período, asignándose como casos(n=59: aquellos neonatos que ingresaron en cuidados especiales neonatales (CEN hijos de madres adolescentes (Introduction: pregnancy in adolescence constitutes a negative health indicator that provokes serious maternal-child consequences. Objective: to evaluate maternal-perinatal and neonatal indicators in adolescent mothers admitted at "Abel Santamaria Cuadrado" University General Hospital during 2010. Material and method: an applied, observational, analytical, retrospective, case-control type study which target group comprised 5363 live-born babies during the period, assigning as cases (n=59: newborn infants who were admitted to Neonatal Intensive Care Unit (NICU, newborn infants of adolescent mothers ( Results: the majority of the adolescents whose newborn infants were admitted to NICU were primigravida (69.49% (OR=5.63; CI 95%: 2.7-11.8; 45, 6% suffered from some affection (OR=2.27; CI 95%: 1.12-4.59, prevailing Premature Rupture of Membranes (18.64% and pregnancy-induced hypertension (11.86%, 49,15% of newborn infants were premature (OR=3.11; CI 95 %: 1.53-6.38, 52.54% were low-birth-weight infants (OR=3.4; CI 95%: 1.67-3.95 and 59,32% got the Apgar score of Conclusions: adolescence had a negative influence on perinatal and neonatal indicators increasing the risks of diseases associated with pregnancy: prematurity, low-weight and depression at birth.

Uso correcto de la vía inhalatoria en el tratamiento del asma bronquial

Directory of Open Access Journals (Sweden)

Annery Luis Martínez

2001-10-01

Full Text Available Se realizó un estudio descriptivo, transversal en 100 pacientes asmáticos adultos atendidos en el Policlínico Docente "Mario Muñoz Monroy", residentes en el reparto Abel Santamaría, con el objetivo de comprobar si conocen la forma adecuada de usar los inhaladores y si son instruidos en esta técnica. Se conoció que el 72 % de los pacientes recibieron instrucción, pero solo a un 23 % se le evaluó la técnica inhalatoria. En menos de la mitad de los enfermos se consideró que usaban una técnica buena, y se identificaron como errores más frecuentes no llevar la cabeza hacia atrás, accionar más de una vez el inhalador en una misma inspiración y no mantener una apnea. Resultó evidente la necesidad de educar al paciente asmático en el uso correcto de la vía inhalatoriaA crosswise descriptive study of 100 asthmatic adults, who live in the "Abel Santa María" residential zone and are seen at "Mario Muñoz Monroy" teaching polyclinics, was conducted to find out if they knew how to use correctly the aerosol inhalers and if they were instructed in managing that technique. It was known that 72% of the patients was taught how to use it but the inhalation technique had only been evaluated in 23% of the patients. It was considered that less than half of them followed a good technique. The more frequent mistakes were to push down the inhaler more than once in the same breathing, not to move the head backwards and not to keep the apnea. It was evident that the asthmatic patient needs to be instructed about the correct use of the inhalation administration

Tentativa de suicidio y apgar familiar modificado

Directory of Open Access Journals (Sweden)

Bárbara de la C Santos Céspedes

1997-08-01

Full Text Available Se estudian 50 pacientes con tentativa de suicidio durante 1993 en el área de salud del Policlínico "Josué País García" del Centro Urbano "Abel Santamaría" de Santiago de Cuba, mediante el Apgar familiar modificado, instrumento que mide el grado de funcionamiento familiar, adaptado después de estudios pilotos en la misma población. Las categorías adaptación, relación, desarrollo, efecto y convivencia, así como el resultado general del Apgar, demostraron que la dinámica familiar de las personas investigadas fue significativamente desfavorable, hallazgos que se validaron por las técnicas estadísticas convencionales. Este trabajo propone la investigación del fenómeno del suicidio con la perspectiva del enfoque sistémico de la familia y el individuo, modelo que se escapa a la tradición médica, el cual se considera importante como instrumento para los médicos de la familia.50 patients who attempted suicide in 1993 at the health area of the "Josué País García" Polyclinic from the "Abel Santamaría" Urban Center, in Santiago de Cuba, were studied by using the modified family Apgar, a tool that measures the family functioning degree, adaptation, relation, development, effect, and living together categories, as well as the Apgar's general result, showed that the family dynamics of the persons investigated was significantly unfavourable. These findings were validated by the conventional statistical techniques. This paper recommends the investigation of the sucide phenomenon with the perspective of the systemic approach of the family and the individual, a model hat escapes as an important tool for family physicians.

BD-22deg3467, a DAO-type Star Exciting the Nebula Abell 35

Science.gov (United States)

Ziegler, M.; Rauch, T.; Werner, K.; Koppen, J.; Kruk, J. W.

2013-01-01

Spectral analyses of hot, compact stars with non-local thermodynamical equilibrium (NLTE) model-atmosphere techniques allow the precise determination of photospheric parameters such as the effective temperature (T(sub eff)), the surface gravity (log g), and the chemical composition. The derived photospheric metal abundances are crucial constraints for stellar evolutionary theory. Aims. Previous spectral analyses of the exciting star of the nebula A35, BD-22deg3467, were based on He+C+N+O+Si+Fe models only. For our analysis, we use state-of-the-art fully metal-line blanketed NLTE model atmospheres that consider opacities of 23 elements from hydrogen to nickel. We aim to identify all observed lines in the ultraviolet (UV) spectrum of BD-22deg3467 and to determine the abundances of the respective species precisely. Methods. For the analysis of high-resolution and high signal-to-noise ratio (S/N) far-ultraviolet (FUSE) and UV (HST/STIS) observations, we combined stellar-atmosphere models and interstellar line-absorption models to fully reproduce the entire observed UV spectrum. Results. The best agreement with the UV observation of BD-22deg3467 is achieved at T(sub eff) = 80 +/- 10 kK and log g = 7.2 +/- 0.3. While T(sub eff) of previous analyses is verified, log g is significantly lower. We re-analyzed lines of silicon and iron (1/100 and about solar abundances, respectively) and for the first time in this star identified argon, chromium, manganese, cobalt, and nickel and determined abundances of 12, 70, 35, 150, and 5 times solar, respectively. Our results partially agree with predictions of diffusion models for DA-type white dwarfs. A combination of photospheric and interstellar line-absorption models reproduces more than 90% of the observed absorption features. The stellar mass is M approx. 0.48 Solar Mass. Conclusions. BD.22.3467 may not have been massive enough to ascend the asymptotic giant branch and may have evolved directly from the extended horizontal branch to the white dwarf state. This would explain why it is not surrounded by a planetary nebula. However, the star, ionizes the ambient interstellar matter, mimicking a planetary nebula.

Symbol, Mask and Myth in the Poetry of Resistance by Qaisar Aminpoor

Directory of Open Access Journals (Sweden)

Kobra Rowshanfekr

2013-05-01

Full Text Available Abstract Analytical and statistical method of research is used in current study. After discovering and classifying of symbols and myths, they categorized into five areas which derived from nature, positive and negative characters, animals and other items which with regard to their essence cannot be included among natural, characteristic and animal areas. Then functional range of these sections and variety and ingenuity of the poet in the use of these concepts will be examined in this study and we'll try to answer to these questions that how much quantity range of symbol , mask and myth elements are used in Aminpoor's poetry and what kinds of concepts are included in his poetry?  Poetry of war in early years, had fallen into a slogan Poets policy was improvement of speech toward imaginary horizons. The use of symbolic speech is one way of emergence, consolidation and spread of the poetic imagination in the war poem (Poorjafi., 1384: p 22. Identity, ambiguity and seeking a path to literary and artistic richness are the major trends of Aminpoor in the use of symbolic elements.  Mythic approach and using of historic characters, which became a part of nation's history (Abbas, 1992: p 125, in Aminpoor's poetry are used to create a hero and heroism in his poetry and expressing resistance ideas as well. Hence, poets by recreating historical, national and religious characters, according to the needs of the community, strengthen a sense of strength, durability against foreign domination and flatter their power and steady to their enemies (Lak, 1384: pp. 64, 69.  However, in mask poetry, Aminpoor uses historical, religious and Sufi figures and with recreating these characters, impose his own thoughts and perspectives upon them completely (Ahmad Ali El Zobaidi, 2008: pp. 140 & Ashari Zayed, 1978: p 93.  "from the countless names of your martyr / Abel was the first name / anymore / do not remember these days / Abel / was my other name" (A. M., 1388: p

Enacs Survey of Southern Galaxies Indicates Open Universe

Science.gov (United States)

1996-02-01

New Light on Rich Clusters of Galaxies and their Formation History In the context of a comprehensive Key-Programme , carried out with telescopes at the ESO La Silla Observatory, a team of European astronomers [1]. has recently obtained radial velocities for more than 5600 galaxies in about 100 rich clusters of galaxies. With this programme the amount of information about the motions of galaxies (the kinematical data) in such clusters has almost been doubled. This has allowed the team to study the distribution of the cluster masses, and also the dynamical state of clusters in new and interesting ways. An important result of this programme is that the derived masses of the investigated clusters of galaxies indicate that the mean density of the Universe is insufficient to halt the current expansion; we may therefore be living in an open Universe that will expand forever. Clusters of galaxies as tracers of large-scale structure About 40 years ago, American astronomer George Abell, working at the Palomar Observatory in California, was the first to perform a systematic study of rich clusters of galaxies , that is clusters with particularly many member galaxies located within a relatively restricted region in the sky. He identified several thousands of such clusters, and he numbered and described them; they are now known to astronomers as `Abell clusters'. More than twenty years earlier, Swiss-American astronomer Fritz Zwicky, using the famous 100-inch Mount Wilson telescope above Los Angeles, concluded that the total mass of a rich cluster of galaxies is probably much larger than the combined mass of the individual galaxies we can observe in it. This phenomenon is now known as the `Missing Dark Matter' , and many attempts have since been made to understand its true nature. Although the existence of this Dark Matter is generally accepted, it has been very difficult to prove its existence in a direct way. Rich clusters have several components: in addition to several

Test of the decaying dark matter hypothesis using the Hopkins Ultraviolet Telescope

Science.gov (United States)

Davidsen, A. F.; Kriss, G. A.; Ferguson, H. C.; Blair, W. P.; Bowers, C. W.; Kimble, R. A.

1991-01-01

Sciama's hypothesis that the dark matter associated with galaxies, galaxy clusters, and the intergalactic medium consists of tau neutrinos of rest mass 28-30 eV whose decay generates ultraviolet photons of energy roughly 14-15 eV, has been tested using the Hopkins Ultraviolet Telescope flows aboard the Space Shuttle Columbia. A straightforward application of Sciama's model predicts that a spectral line from neutrino decay photons should be observed from the rich galaxy cluster Abell 665 with an SNR of about 30. No such emission was detected. For neutrinos in the mass range 27.2-32.1 eV, the observations set a lower lifetime limit significantly greater than Sciama's model requires.

Initial analysis of the HL-2A tokamak visible light measurements

International Nuclear Information System (INIS)

Shi Le; Zheng Yinjia

2005-01-01

Measurement of H α radial distribution is an important part in a plasma experiment. During the HL-2A experiment, CCD photos recorded the plasma radiation information using a plasma imaging system, particularly the H α line emission information (with H α filter in front of the camera). Since the line of light radiation measurement involves a line integral of the radiating region, data handling and analysis are necessary. The H α radial distribution along an HL-2A tokamak radial radius can be obtained by using an Abel inversion transformation with plasma imaging on the HL-2A tokamak. This paper provides a reliable measurement method on the HL-2A tokamak. (authors)

Summation of divergent series and Zel'dovich's regularization method

International Nuclear Information System (INIS)

Mur, V.D.; Pozdnyakov, S.G.; Popruzhenko, S.V.; Popov, V.S.

2005-01-01

The method of summation of divergent series, including series of a perturbation theory, which is an analog of the Zel'dovich regularization procedure in the theory of quasistationary states is considered. It is shown that this method is more powerful than the well-known Abel and Borel methods, but compatible with them (i. e., gives the same value for the sum of the series). The restrictions to the range of parameters which appear after removal of the regularization of integrals by this method are discussed. The dynamical Stark shifts and widths of weakly bound s states in a field of circularly polarized electromagnetic wave are calculated at different values of the Keldysh adiabaticity parameter and multiquantum parameter [ru

Respect par les Canadiens de 10 à 17 ans des Directives canadiennes en matière de mouvement sur 24 heures pour les enfants et les jeunes

Directory of Open Access Journals (Sweden)

Ian Janssen

2017-01-01

Full Text Available Introduction : Le document Directives canadiennes en matière de mouvement sur 24 heures pour les enfants et les jeunes publié en 2016 contient des recommandations quant à l’activité physique quotidienne d’intensité moyenne à élevée, au temps de loisir passé devant un écran et au sommeil chez les jeunes de 5 à 17 ans. Cette étude a pour objectif d’estimer le pourcentage de Canadiens de 10 à 17 ans qui respectent ces recommandations. Méthodologie : Nous avons analysé un échantillon national représentatif de 22 115 jeunes. Les données sur le comportement actif ont été autodéclarées. Le respect des recommandations des Directives repose sur les éléments suivants : accumulation d’au moins 60 minutes par jour d’activité physique d’intensité moyenne à élevée, pas plus de 2 heures par jour de temps de loisir passé devant un écran et de 9 à 11 heures de sommeil continu par nuit pour les jeunes de 10 à 13 ans ou de 8 à 10 heures de sommeil continu par nuit pour les jeunes de 14 à 17 ans. Résultats : Seulement 3 % des jeunes de l’échantillon respectaient les trois recommandations clés. Vingt-cinq pour cent respectaient deux recommandations, 51 % en respectaient une et 21 % n’en respectaient aucune. La recommandation en matière de sommeil était la plus respectée par les enfants et les jeunes (66 %, suivie de celle en matière d’activité physique d’intensité moyenne à élevée (35 % et de celle relative au temps passé devant un écran (8 %. Conclusion : Une faible proportion (moins de 3 % de Canadiens de 10 à 17 ans respectent les trois principales recommandations des Directives canadiennes en matière de mouvement sur 24 heures pour les enfants et les jeunes.

De l'atome antique à l'atome quantique à la recherche des mystères de la matière

CERN Document Server

Gruber, Christian

2013-01-01

Les atomes et les molécules constituent les éléments fondamentaux de la matière. Cet état de fait, aujourd'hui admis par tous, repose toutefois sur un paradoxe : nul n'est en mesure d'en percevoir immédiatement la réalité. 500 ans avant notre ère, Démocrite pose pourtant les bases de ce qui deviendra la théorie atomique ; suivront vingt-cinq siècles d'interrogations et de recherches dans l'espoir de percer les secrets de l'invisible. C'est à la découverte de cette épopée scientifique et humaine que cet ouvrage invite le lecteur. Il décrit, depuis la philosophie naturelle antique jusqu'à la révolution quantique actuelle, la soif de savoir qui a guidé l'homme sur les traces de la nature ultime de la matière. Synthétique, didactique et tout spécialement conçu pour un lectorat non scientifique, il présente les principaux concepts théoriques et les expériences fondatrices qui ont progressivement transformé l'hypothèse atomique en une réalité scientifique. Un livre rare, jusqu'à pré...

C2 Swan spectrum used as a molecular pyrometer in transferred arc and the influence noise to signal ratio on the temperature values

International Nuclear Information System (INIS)

Nassar, H

2014-01-01

The C 2 Swan system molecular emission spectrum is frequently observed in arc plasmas containing hydrocarbons. The spectra emitted from 5 kw in the transferred arc reactor at atmospheric pressure by CH 4 /CO 2 /Ar mixture are recorded with the help of an optical system consisting of a linear CCD array coupled with 2m spectrometer. The rotational temperature of 4300±300 K is found from the experimental Abel inverted spectra in the arc center after a point-to-point comparison of the spectrum with a computer simulated one. The influence of the noise to signal ratio has been studied, if the noise to signal ratio is about 10% we found an error of 7% at temperature 3000 K and 10% at 6000 K.

Discrete coupled derivative nonlinear Schroedinger equations and their quasi-periodic solutions

International Nuclear Information System (INIS)

Geng Xianguo; Su Ting

2007-01-01

A hierarchy of nonlinear differential-difference equations associated with a discrete isospectral problem is proposed, in which a typical differential-difference equation is a discrete coupled derivative nonlinear Schroedinger equation. With the help of the nonlinearization of the Lax pairs, the hierarchy of nonlinear differential-difference equations is decomposed into a new integrable symplectic map and a class of finite-dimensional integrable Hamiltonian systems. Based on the theory of algebraic curve, the Abel-Jacobi coordinates are introduced to straighten out the corresponding flows, from which quasi-periodic solutions for these differential-difference equations are obtained resorting to the Riemann-theta functions. Moreover, a (2+1)-dimensional discrete coupled derivative nonlinear Schroedinger equation is proposed and its quasi-periodic solutions are derived

Introduction to Abelian varieties

CERN Document Server

Murty, V Kumar

1993-01-01

The book represents an introduction to the theory of abelian varieties with a view to arithmetic. The aim is to introduce some of the basics of the theory as well as some recent arithmetic applications to graduate students and researchers in other fields. The first part contains proofs of the Abel-Jacobi theorem, Riemann's relations and the Lefschetz theorem on projective embeddings over the complex numbers in the spirit of S. Lang's book Introduction to algebraic and abelian functions. Then the Jacobians of Fermat curves as well as some modular curves are discussed. Finally, as an application, Faltings' proof of the Mordell conjecture and its intermediate steps, the Tate conjecture and the Shafarevich conjecture, are sketched. - H. Lange for MathSciNet.

Observations of gravitational lenses

International Nuclear Information System (INIS)

Fort, B.

1990-01-01

During the last tow years a burst of results has come from radio and optical surveys of ''galaxy lenses'' (where the main deflector is a galaxy). These are reviewed. On the other hand, in September 1985 we pointed out a very strange blue ring-like structure on a Charge-Coupled Device image of the cluster of galaxies Abell 370. This turned out to be Einstein arcs discovery. Following this discovery, new observational results have shown that many rich clusters of galaxies can produce numerous arclets: tangentially distorted images of an extremely faint galaxy population probably located at redshift larger than 1. This new class of gravitational lenses proves to be an important observational topic and this will be discussed in the second part of the paper. (author)

Cosmic Dawn: The First Star in the Universe

Energy Technology Data Exchange (ETDEWEB)

Abel, Tom

2008-04-29

What was the first thing in the Universe? A black hole or a star? How did it form? Even our biggest and best telescopes cannot tell us. Direct calculation with supercomputers, however, can. The first luminous objects in the Universe were very massive stars shining one million times as brightly as our sun. They died quickly and seeded the cosmos with the chemical elements necessary for life. One star at a time, galaxies started to assemble just one hundred million years after the Big Bang, and they are still growing now. Join Dr. Abel in a fascinating journey through the early universe, where he uses the latest computer animations of early star formation, supernovae explosions and the buildup of the first galaxies.

PROBLEMAS INVERSOS MAL COLOCADOS EM QUÍMICA

Directory of Open Access Journals (Sweden)

João P. Braga

Full Text Available What is an ill-posed inverse problem? The answer to this question is the main objective of the present paper and the pre-requisite to follow the material requires only elementary calculus. The first mathematical formulation of an inverse problem, due to N. H. Abel, together with the fundamental work by Jacques Hadamard, are explored at the beginning of the paper. A prototype system is used to consider the regularization concept. Three numerical methods, the Tikhonov regularization, the decomposition into singular values and the Hopfield neural networks, applied to remove the singularity are examined. General aspects of the ill-posed inverse problems in chemistry with emphasis in thermodynamics and a set of general rules for other areas of science are also analyzed.

Frequency effects in silane plasmas for PECVD

International Nuclear Information System (INIS)

Howling, A.A.; Dorier, J.L.; Hollenstein, C.; Finger, F.; Kroll, U.

1991-09-01

It is generally recognised that the excitation frequency is an important parameter in rf plasma-assisted deposition. VHF silane plasmas (50-100 MHz) have been shown to produce high quality amorphous silicon films up to 20 A/s, and therefore the aim of this work is to compare the VHF range with the 13.56 MHz industrial frequency in the same reactor. The principal diagnostics used are electrical measurements and a CCD camera for spatially-resolved plasma-induced emission with Abel inversion of the plasma image. We present a comparative study of key discharge parameters such as deposition rates, plasma uniformity, ion impact energy, power transfer efficiency and powder formation for the rf range 13-70 MHz. (author) 5 figs., 19 refs

Summation of Divergent Series and Zeldovich's Regularization Method

International Nuclear Information System (INIS)

Mur, V.D.; Pozdnyakov, S.G.; Popruzhenko, S.V.; Popov, V.S.

2005-01-01

A method for summing divergent series, including perturbation-theory series, is considered. This method is an analog of Zeldovich's regularization method in the theory of quasistationary states. It is shown that the method in question is more powerful than the well-known Abel and Borel methods, but that it is compatible with them (that is, it leads to the same value for the sum of a series). The constraints on the parameter domain that arise upon the removal of the regularization of divergent integrals by this method are discussed. The dynamical Stark shifts and widths of loosely bound s states in the field of a circularly polarized electromagnetic wave are calculated at various values of the Keldysh adiabaticity parameter and the multiquantum parameter

X-ray absorption radiography for high pressure shock wave studies

Science.gov (United States)

Antonelli, L.; Atzeni, S.; Batani, D.; Baton, S. D.; Brambrink, E.; Forestier-Colleoni, P.; Koenig, M.; Le Bel, E.; Maheut, Y.; Nguyen-Bui, T.; Richetta, M.; Rousseaux, C.; Ribeyre, X.; Schiavi, A.; Trela, J.

2018-01-01

The study of laser compressed matter, both warm dense matter (WDM) and hot dense matter (HDM), is relevant to several research areas, including materials science, astrophysics, inertial confinement fusion. X-ray absorption radiography is a unique tool to diagnose compressed WDM and HDM. The application of radiography to shock-wave studies is presented and discussed. In addition to the standard Abel inversion to recover a density map from a transmission map, a procedure has been developed to generate synthetic radiographs using density maps produced by the hydrodynamics code DUED. This procedure takes into account both source-target geometry and source size (which plays a non negligible role in the interpretation of the data), and allows to reproduce transmission data with a good degree of accuracy.

A Fiber Interferometer for the Magnetized Shock Experiment

International Nuclear Information System (INIS)

Yoo, Christian

2012-01-01

The Magnetized Shock Experiment (MSX) at Los Alamos National Laboratory requires remote diagnostics of plasma density. Laser interferometry can be used to determine the line-integrated density of the plasma. A multi-chord heterodyne fiber optic Mach-Zehnder interferometer is being assembled and integrated into the experiment. The advantage of the fiber coupling is that many different view chords can be easily obtained by simply moving transmit and receive fiber couplers. Several such fiber sets will be implemented to provide a time history of line-averaged density for several chords at once. The multiple chord data can then be Abel inverted to provide radially resolved spatial profiles of density. We describe the design and execution of this multiple fiber interferometer.

First oceanographic atlas of the Gulf of Mexico. National Award of Oceanographic Research

International Nuclear Information System (INIS)

Vidal L., F.; Vidal L., V.M.; Hernandez O., A.

1991-01-01

First oceanographic atlas of the Gulf of Mexico National award of oceanographic research. As a result of the research activities applied by Federal Electricity Commission related with oceanographic studies for nuclear stations siting and licensing in coastal areas, doctors Victor Manuel and Francisco Vidal Lorandi and Master in Sciences Abel Hernandez Ochoa got the oceanographic research National award, instituted recently by Mexican Government, by research work published in Oceanographic Atlas of the Gulf of Mexico, Volume II. Atlas presents synthetized oceanographic information about mexican gulf circulation, as well as residence time and water masses distribution. Atlas includes information related with siting and licensing of nuclear stations on shore and has also application, among others, in petroleum, fishery, maritime transportation, and tourism sectors

An integrable (2+1)-dimensional Toda equation with two discrete variables

International Nuclear Information System (INIS)

Cao Cewen; Cao Jianli

2007-01-01

An integrable (2+1)-dimensional Toda equation with two discrete variables is presented from the compatible condition of a Lax triad composed of the ZS-AKNS (Zakharov, Shabat; Ablowitz, Kaup, Newell, Segur) eigenvalue problem and two discrete spectral problems. Through the nonlinearization technique, the Lax triad is transformed into a Hamiltonian system and two symplectic maps, respectively, which are integrable in the Liouville sense, sharing the same set of integrals, functionally independent and involutive with each other. In the Jacobi variety of the associated algebraic curve, both the continuous and the discrete flows are straightened out by the Abel-Jacobi coordinates, and are integrated by quadratures. An explicit algebraic-geometric solution in the original variable is obtained by the Riemann-Jacobi inversion

Hard X-Ray Properties of the Merging Cluster Abell 3667 as Observed with Suzaku

Science.gov (United States)

2008-08-01

3667 as Observed with Suzaku Kazuhiro NAKAZAWA Department of Physics, The University of Tokyo, 7-3-1 Hongo , Bunkyo-ku, Tokyo 113-0033 nakazawa...of Tokyo, 7-3-1 Hongo , Bunkyo-ku, Tokyo 113-0033 Kazuo MAKISHIMA Department of Physics, The University of Tokyo, 7-3-1 Hongo , Bunkyo-ku, Tokyo 113

Ideological and poetic topic of land in the 1930s. Eerik Haamer / Tiina Abel

Index Scriptorium Estoniae

Abel, Tiina, 1951-

2010-01-01

1930. aastate eesti maalikunstist, motiividest. Maalikunstnik Eerik Haameri loomingust. Kujutati Eesti maastikku, maaelu, maainimest. Eerik Haamer jäädvustas peamiselt Saaremaa ja Ruhnu rannarahva argielu

Dark matter dynamics in Abell 3827 : new data consistent with standard cold dark matter.

OpenAIRE

Massey, R.; Harvey, D.; Liesenborgs, J.; Richard, J.; Stach, S.; Swinbank, M.; Taylor, P.; Williams, L.; Clowe, D.; Courbin, F.; Edge, A.; Israel, H.; Jauzac, M.; Joseph, R.; Jullo, E.

2018-01-01

We present integral field spectroscopy of galaxy cluster Abell 3827, using Atacama Large Millimetre Array (ALMA) and Very Large Telescope/Multi-Unit Spectroscopic Explorer. It reveals an unusual configuration of strong gravitational lensing in the cluster core, with at least seven lensed images of a single background spiral galaxy. Lens modelling based on Hubble Space Telescope imaging had suggested that the dark matter associated with one of the cluster's central galaxies may be offset. The ...

The Case of Abel: Religion as Boon and Bane for a Catholic Gay Man.

Science.gov (United States)

Cerbone, Armand R; Danzer, Graham

2017-08-01

Conservative religions that condemn homosexual sexual orientation and acts as unnatural and sinful pose significant challenges for gay persons whose faith is a core part of their identity. The condemnation presents a serious barrier to the acceptance and integration of their sexuality, a primary task of psychosexual development. As a result, they can manifest depression, anxiety, suicidal ideation, and even suicide attempts. The ecclesiastical censure also imposes an untenable dilemma for homosexuals in that they feel pressed to reject their sexual identity or renounce their spiritual identity and heritage. Psychotherapists who treat gay persons caught in this quandary can find themselves facing a similar problem: how to help their homosexual client reconcile their proscribed sexuality with their spiritual commitments. The case presented here recounts the treatment over many years of a gay man suffering from such a conflict and his eventual accommodation of both his homosexuality and his faith. Recommendations are offered for constructive treatment with those torn between two conflicting core identities. © 2017 Wiley Periodicals, Inc.

Inmigrantes italianos en Argentina: la Correspondencia entre Oreste, Abele y Luigi Sola (1901-1922

Directory of Open Access Journals (Sweden)

María Teresa Sanhueza

2015-01-01

Full Text Available Los estudios históricos de la inmigración generalmente se concentran más en el análisis de datos y números que dan cuenta del comportamiento de masas de individuos y menos en las experiencias individuales. Es por eso que la correspondencia epistolar de la familia Sola, intercambiada sin interrupción a lo largo de 22 años, 1901 a 1922, debe ser analizada no solo como documento histórico sino también en sus dimensiones sociales y políticas ya que, en su conjunto, ofrece una instantánea de la experiencia inmigratoria, en el momento en que evidencia la comunicación bidireccional establecida entre los miembros de una familia particular y muestra una perspectiva transnacional de cómo la inmigración transformó a Italia y a Argentina, es decir, entendida como discurso público al tiempo que como discurso privado.

Epidemiología de las lesiones por quemaduras Epidemiology of lesions provoked by burns

Directory of Open Access Journals (Sweden)

José A Viñas Díaz

2009-12-01

Full Text Available Las quemaduras son una causa importante de muerte accidental, solo superadas por los accidentes de automóviles. Con el objetivo de conocer algunos aspectos de la epidemiología de las quemaduras en Pediatría en la provincia de Pinar del Río (Cuba, se realizó una investigación transversal, descriptiva que abarcó 26 casos con edades comprendidas entre 0-18 años, ingresados con el diagnóstico de quemaduras no intencionales en el Servicio de Caumatología del Hospital "Abel Santamaría Cuadrado" Pinar del Río. (Cuba, durante el año 2006. Se revisaron las historias clínicas y para el tratamiento de la información se utilizó la estadística descriptiva, determinando la relación entre las variables estudiadas. Se encontró que el grupo más afectado era el menor de 15 años (96.2 %, en la cocina (42.3 %por escaldadura, por líquidos calientes (53,8%. No hubo fallecidos. La prevención es un aspecto decisivo para evitar este tipo de accidente.Burns are one of the most important causes of accidental death, only exceeded by traffic accidents. This paper is aimed at knowing issues related to the epidemiology of burns in pediatric ages in Pinar del Rio Province, Cuba. A cross-sectional, descriptive study was conducted with 26 burned children (0-18 years old admitted to the Caumatology Service at "Abel Santamaria" General University Hospital, during 2006. Clinical records were the source of information and descriptive statistics for showing frequencies and X² at 95 % of certainty was used for homogeneity. The group of ages younger than 15 years old was the most affected (96.2 %. Burns were mainly produced at the kitchen (42, 3 % by hot liquids (scalds (53.8 %, among other causes without mortality. Prevention is a decisive action to avoid this type of accident.

Analysis of Lymphangioleiomyomatosis (LAM) patent tomograms: Stereology and modeling

International Nuclear Information System (INIS)

Faber, V.; Wing, G.M.; Winter, L.; Zahrt, J.D.

1995-01-01

Lymphangioleiomyomatosis (LAM) is an insidious disease of young women which attacks the lungs and if untreated results in death. Treatment is radical. Currently a woman diagnosed as having LAM (usually by computed tomography (CT) of the lung) is run through an exhausting set of tests and exercises to determine the extent of the disease. Image processing techniques have been able to quantify the tomograms by providing a histogram of the number of cyst intercepts of a given area. The images are digital, so the data are discrete, and the areas are in terms of square pixels. It is hoped that by analyzing the data and by recovering the probability density of the cysts themselves one can provide a set of parameters that will aid in the early diagnosis of the disease and that will correlate well with the physiology. The desire to invert the data, that is to determine the probability density of the cysts from the probability density of the circular intersections of the cysts with the tomographic plane, led to a re-examination of the Wicksell equation. In Section 2, the authors transform Wicksell's equation in diameter (a generalized Abel equation) into an equation in areas (the original Abel equation). In Section 3 they present the adjoint equation in several equivalent forms. Analytic solutions of the adjoint equation necessary for later use are developed in Section 4. Outside of the framework of integral equations they have done some modeling of the data. They find that, to a very high degree of reliability, the data follows a simple power law. The distribution of spheres likewise follows a simple power law. These considerations are given in Section 5. Then in Section 6 they explore the exponential model as an alternative. Section 7 solves the Wicksell equation and uses the Golberg device, via the adjoint, to solve a related problem. They finally get to the number of cysts and their average size in Section 8. Their conclusions are in Section 9

THE DYNAMICAL STATE OF BRIGHTEST CLUSTER GALAXIES AND THE FORMATION OF CLUSTERS

International Nuclear Information System (INIS)

Coziol, R.; Andernach, H.; Caretta, C. A.; Alamo-MartInez, K. A.; Tago, E.

2009-01-01

A large sample of Abell clusters of galaxies, selected for the likely presence of a dominant galaxy, is used to study the dynamical properties of the brightest cluster members (BCMs). From visual inspection of Digitized Sky Survey images combined with redshift information we identify 1426 candidate BCMs located in 1221 different redshift components associated with 1169 different Abell clusters. This is the largest sample published so far of such galaxies. From our own morphological classification we find that ∼92% of the BCMs in our sample are early-type galaxies and 48% are of cD type. We confirm what was previously observed based on much smaller samples, namely, that a large fraction of BCMs have significant peculiar velocities. From a subsample of 452 clusters having at least 10 measured radial velocities, we estimate a median BCM peculiar velocity of 32% of their host clusters' radial velocity dispersion. This suggests that most BCMs are not at rest in the potential well of their clusters. This phenomenon is common to galaxy clusters in our sample, and not a special trait of clusters hosting cD galaxies. We show that the peculiar velocity of the BCM is independent of cluster richness and only slightly dependent on the Bautz-Morgan type. We also find a weak trend for the peculiar velocity to rise with the cluster velocity dispersion. The strongest dependence is with the morphological type of the BCM: cD galaxies tend to have lower relative peculiar velocities than elliptical galaxies. This result points to a connection between the formation of the BCMs and that of their clusters. Our data are qualitatively consistent with the merging-groups scenario, where BCMs in clusters formed first in smaller subsystems comparable to compact groups of galaxies. In this scenario, clusters would have formed recently from the mergers of many such groups and would still be in a dynamically unrelaxed state.

Estesioneuroblastoma. Presentación de un caso Esthesioneuroblastoma. A case report

Directory of Open Access Journals (Sweden)

Luís Enrique Torres Rodríguez

2012-10-01

Full Text Available El neuroblastoma olfatorio o "estesioneuroblastoma" es un tumor embrionario, infrecuente, derivado de neuroblastos de las ramificaciones nasales del sistema sensorial olfatorio, cuyo asiento es el epitelio respiratorio neuroectodérmico; fue descrito originalmente en 1924. La presentación más común es la de un crecimiento polipoide que causa epistaxis u obstrucción nasal con anosmia de larga evolución. Es localmente muy recidivante, aunque se han reportado metástasis regionales y a distancia. El objetivo de este trabajo es caracterizar desde el punto de vista patológico un paciente masculino, atendido en el servicio de Cirugía Maxilofacial del Hospital General Docente "Abel Santamaría Cuadrado" de la provincia de Pinar del Río, con un aumento de volumen en la hemicara en relación al seno maxilar izquierdo. Este paciente también tenía un tratamiento por una sinusitis maxilar, al cual se le hizo una biopsia insicional y se obtuvo como resultado un estesioneuroblastoma con metástasis frontal. Se expone por tratarse de una enfermedad poco frecuente en nuestro medio.Olfactory neuroblastoma or "esthesioneuroblastoma" is an infrequent embryonate tumor, derived from the neuroblasts belonging to the nasal ramification of sensory-olfactory system, which seat is the neuroectodermic respiratory epithelium that was described in 1924 originally. The most common presentation is a polypoid growth that provokes epistaxis or nasal obstruction with a large natural history of anosmia. It is very recurrent locally, thought regional or distant metastases have been reported. This work was aimed at characterizing a male patient from the pathologic view point who attended to the Maxillofacial Surgery Service at "Abel Santamaria Cuadrado" University Hospital, Pinar del Rio, presenting an increase of volume on the hemiface in relation to the left maxillary sinus. This patient was under treatment because of a maxillary sinusitis, the incisional biopsy showed

Algunos aspectos epidemiológicos en la morbilidad obstétrica crítica Some epidemiological aspects in critical obstetric morbidity

Directory of Open Access Journals (Sweden)

Jorge M Balestena Sánchez

2006-12-01

Full Text Available Con la finalidad de analizar el comportamiento de la morbilidad en la paciente obstétrica crítica se realizó una investigación retrospectiva, transversal, analítica en el Hospital Universitario "Abel Santamaría Cuadrado", durante el periodo de mayo del 2001 hasta diciembre de 2004. El universo quedó conformado por todas las pacientes obstétricas (embarazadas o puérperas que ingresaron en dicho hospital en el período antes mencionado, la muestra se formó con todas aquellas pacientes que ingresaron en la terapia intensiva, se estudiaron variables relacionadas con la madre, el embarazo y el parto. Utilizamos el por ciento, el promedio y la desviación estándar así como el test de diferencia de proporciones (Z, con nivel de significación de pIn order to analyze the behaviour of the morbidity rate in the critical obstetric patient a retrospective, cross-sectional, analytical research was performed at Abel Santamaría Cuadrado University Hospital, from May 2001 to December 2004. The whole sample was comprised by all the obstetric patients (pregnant or puerperal who were admitted at such hospital during the period above mentioned. The sample comprised all those patients admitted at the Intensive Unit Care. Variables related to the mother, the pregnancy, and labor were analyzed. The percentage, the average and standard deviation were used, as well as the ratio difference test with a level of significance p<0.05. Also, odds ratio (OR was used to ascertain the risk factor and the attributable percentage risk, as well as the confidence interval for OR 95%. The serious maternal morbidity was highly associated with the aging, pregnant, multipara, those who underwent previous labors, bronchial asthma, hypertension, and heart disease, as well as the hypertensive processes during pregnancy. The obstetric causes were most frequent. Anemia and respiratory sepsis were the predominant complications. As a conclusion, there are maternal events capable

Filaments and clusters of galaxies

International Nuclear Information System (INIS)

Soltan, A.

1987-01-01

A statistical test to investigate filaments of galaxies is performed. Only particular form of filaments is considered, viz. filaments connecting Abell clusters of galaxies. Relative position of triplets ''cluster - field object - cluster'' is analysed. Though neither cluster sample nor field object sample are homogeneous and complete only peculiar form of selection effects could affect the present statistics. Comparison of observational data with simulations shows that less than 15 per cent of all field galaxies is concentrated in filaments connecting rich clusters. Most of the field objects used in the analysis are not normal galaxies and it is possible that this conclusion is not in conflict with apparent filaments seen in the Lick counts and in some nearby 3D maps of the galaxy distribution. 26 refs., 2 figs. (author)

Prediction of phonon thermal transport in thin GaAs, InAs and InP nanowires by molecular dynamics simulations: influence of the interatomic potential

Energy Technology Data Exchange (ETDEWEB)

Carrete, J; Longo, R C; Gallego, L J, E-mail: jesus.carrete@usc.es [Departamento de Fisica de la Materia Condensada, Facultad de Fisica, Universidad de Santiago de Compostela, E-15782 Santiago de Compostela (Spain)

2011-05-06

A number of different potentials are currently being used in molecular dynamics simulations of semiconductor nanostructures. Confusion can arise if an inappropriate potential is used. To illustrate this point, we performed direct molecular dynamics simulations to predict the room temperature lattice thermal conductivity {lambda} of thin GaAs, InAs and InP nanowires. In each case, simulations performed using the classical Harrison potential afforded values of {lambda} about an order of magnitude smaller than those obtained using more elaborate potentials (an Abell-Tersoff, as parameterized by Hammerschmidt et al for GaAs and InAs, and a potential of Vashishta type for InP). These results will be a warning to those wishing to use computer simulations to orient the development of quasi-one-dimensional systems as heat sinks or thermoelectric devices.

Implications for gravitational lensing and the dark matter content in clusters of galaxies from spatially resolved x-ray spectra

Science.gov (United States)

Loewenstein, M.

1994-01-01

A simple method for deriving well-behaved temperature solutions to the equation of hydrostatic equilibrium for intracluster media with X-ray imaging observations is presented and applied to a series of generalized models as well as to observations of the Perseus cluster and Abell 2256. In these applications the allowed range in the ratio of nonbaryons to baryons as a function of radius is derived, taking into account the uncertainties and crude spatial resolution of the X-ray spectra and considering a range of physically reasonable mass models with various scale heights. Particular attention is paid to the central regions of the cluster, and it is found that the dark matter can be sufficiently concentrated to be consistent with the high central mass surface densities for moderate-redshift clusters from their gravitational lensing properties.

The pedagogical work of the sculptor René Valdés Cedeño (1916-1976

Directory of Open Access Journals (Sweden)

Sonia Tellez-Vigueaux

2017-12-01

Full Text Available René Valdés Cedeño (1916-1976 was a Havana sculptor who made most of his artistic production in Santiago de Cuba. Pedagogue par excellence held various positions at the Provincial School of Plastic Arts José Joaquín Tejada. His work as a teacher of generations of sculptors earned him the recognition of his students and the Ministry of Education. Author of important works such as the Spirit of the Mountain, located in the Puerto de Boniato, Monument of the Abel Santamaría Square Park, among others. He had great skill with the chisel, he works stone and marble. However, his life and work has been little studied and deepened. So this article aims to show the pedagogical work of this artist.

On the multi-index (3 m-parametric) Mittag-Leffler functions, fractional calculus relations and series convergence

Science.gov (United States)

Paneva-Konovska, Jordanka

2013-10-01

In this paper we consider a family of 3 m-indices generalizations of the classical Mittag-Leffler function, called multi-index (3 m-parametric) Mittag-Leffler functions. We survey the basic properties of these entire functions, find their order and type, and new representations by means of Mellin-Barnes type contour integrals, Wright p Ψ q -functions and Fox H-functions, asymptotic estimates. Formulas for integer and fractional order integration and differentiations are found, and these are extended also for the operators of the generalized fractional calculus (multiple Erdélyi-Kober operators). Some interesting particular cases of the multi-index Mittag-Leffler functions are discussed. The convergence of series of such type functions in the complex plane is considered, and analogues of the Cauchy-Hadamard, Abel, Tauber and Littlewood theorems are provided.

Comparisons of NIF convergent ablation simulations with radiograph data.

Science.gov (United States)

Olson, R E; Hicks, D G; Meezan, N B; Koch, J A; Landen, O L

2012-10-01

A technique for comparing simulation results directly with radiograph data from backlit capsule implosion experiments will be discussed. Forward Abel transforms are applied to the kappa*rho profiles of the simulation. These provide the transmission ratio (optical depth) profiles of the simulation. Gaussian and top hat blurs are applied to the simulated transmission ratio profiles in order to account for the motion blurring and imaging slit resolution of the experimental measurement. Comparisons between the simulated transmission ratios and the radiograph data lineouts are iterated until a reasonable backlighter profile is obtained. This backlighter profile is combined with the blurred, simulated transmission ratios to obtain simulated intensity profiles that can be directly compared with the radiograph data. Examples will be shown from recent convergent ablation (backlit implosion) experiments at the NIF.

Genome-Wide Association Study Reveals Genetic Architecture of Eating Behaviors in Pigs and its Implications for Humans Obesity by Comparative Genome Mapping

DEFF Research Database (Denmark)

Do, Duy Ngoc; Strathe, Anders Bjerring; Ostersen, Tage

2013-01-01

per visit (TPV), mean feed intake per visit(FPV) and mean feed intake rate (FR) were available on 1130 boars. All boars weregenotyped using the Illumina Porcine SNP60 BeadChip. The association analyseswere performed using the GenABEL package in R. Sixteen SNPs had moderategenome-wide significant (p...... association with feeding behavior traits. Locus M1GA0016584 located close to theMSI2 gene on chromosome (SSC) 14 was very strongly associated with NVD (p =9.6E-07). Thirty six SNPs were located in genome regions where QTLs havepreviously been reported......, dephosphorylation and positive regulation of peptide secretiongenes were found highly significantly associated with feeding behavior traits byfunctional annotation. This is the first GWAS to identify genetic variants and biologicalmechanisms for feeding behavior in pigs and these results are important...

The cluster environments of powerful, high-redshift radio galaxies

International Nuclear Information System (INIS)

Yates, M.G.

1989-01-01

We present deep imaging of a sample of 25 powerful radio galaxies in the redshift range 0.15 gr ) about each source, a measure of the richness of environment. The powerful radio galaxies in this sample at z>0.3 occupy environments nearly as rich on average as Abell class 0 clusters of galaxies, about three times richer than the environments of the z<0.3 radio galaxies. This trend in cluster environment is consistent with that seen in radio-loud quasars over the same redshift range. Our previous work on the 3CR sample suggested that the fundamental parameter which correlates with the richness of environment might be the radio luminosity of the galaxy, rather than its redshift. Our direct imaging confirms that the most powerful radio galaxies do inhabit rich environments. (author)

Continuous Emission Spectrum Measurement for Electron Temperature Determination in Low-Temperature Collisional Plasmas

International Nuclear Information System (INIS)

Liu Qiuyan; Li Hong; Chen Zhipeng; Xie Jinlin; Liu Wandong

2011-01-01

Continuous emission spectrum measurement is applied for the inconvenient diagnostics of low-temperature collisional plasmas. According to the physical mechanism of continuous emission, a simplified model is presented to analyze the spectrum in low temperature plasma. The validity of this model is discussed in a wide range of discharge parameters, including electron temperature and ionization degree. Through the simplified model, the continuous emission spectrum in a collisional argon internal inductively coupled plasma is experimentally measured to determine the electron temperature distribution for different gas pressures and radio-frequency powers. The inverse Abel transform is also applied for a better spatially resoluted results. Meanwhile, the result of the continuous emission spectrum measurement is compared to that of the electrostatic double probes, which indicates the effectiveness of this method. (low temperature plasma)

Cold dark matter dominated, inflationary universe with Omega(0) less than 1 and n less than 1

International Nuclear Information System (INIS)

Vittorio, N.; Matarrese, S.; Lucchin, F.

1988-01-01

The theoretical prejudice for a flat universe with an initially scale-invariant power spectrum has restricted the number of cosmological scenarios investigated for studying the formation of structure in the universe. A cold dark matter-dominated universe with a density parameter Omega(0) and a primordial spectral index n different from unity is considered, and its possible consistency with the inflationary model is discussed. It is shown that some of the difficulties of a flat cold dark matter scenario can be avoided by having Omega(0) less than 1 and n less than 1. For Omega(0) roughly 0.4 and n roughly 0.75 a good agreement is obtained with the large-scale drifts, the bounds on the cosmic microwave background smoothness, the Abell cluster abundance, and their correlation function. 85 references

An arc facility for investigating non-LTE thermodynamic and transport phenomena in low and high pressure plasmas

International Nuclear Information System (INIS)

Sedghinisab, A.; Eddy, T.L.; Murray, R.T.

1986-01-01

This paper discusses a high pressure arc facility modified for computerized control and data acquisition to simplify measurements of non-LTE plasmas. The non-LTE methods have shown that numerous spectral lines and continuum must be accurately, precisely and quickly measured.The instrumentation uses a 1-m monochrometer with programmed wavelength slews and scans; oplasma scans; and monitoring of chamber pressure, current, voltages, and location. Multiple flows of various gases can be provided simultaneously. Plasma self absorption is determined via a concave back mirror and shutter with final alignment via computer plots. The raw data is corrected for absorption, zeroed, centered and smoothed. The net line intensity is then determined and Abeled prior to feeding into LTE or non-LTE analysis methods. Sample results are presented at 0.1,1 and 10 atm

Schlieren Cinematography of Current Driven Plasma Jet Dynamics

Science.gov (United States)

Loebner, Keith; Underwood, Thomas; Cappelli, Mark

2016-10-01

Schlieren cinematography of a pulsed plasma deflagration jet is presented and analyzed. An ultra-high frame rate CMOS camera coupled to a Z-type laser Schlieren apparatus is used to obtain flow-field refractometry data for the continuous flow Z-pinch formed within the plasma deflagration jet. The 10 MHz frame rate for 256 consecutive frames provides high temporal resolution, enabling turbulent fluctuations and plasma instabilities to be visualized over the course of a single pulse (20 μs). The Schlieren signal is radiometrically calibrated to obtain a two dimensional mapping of the refraction angle of the axisymmetric pinch plasma, and this mapping is then Abel inverted to derive the plasma density distribution as a function radius, axial coordinate, and time. Analyses of previously unknown discharge characteristics and comparisons with prior work are discussed.

FUNGSI LEMBAGA PEMASYARAKATAN SEBAGAI TEMPAT UNTUK MELAKSANAKAN PEMBINAAN DAN PELAYANAN TERPIDANA MATI SEBELUM DIEKSEKUSI

Directory of Open Access Journals (Sweden)

Budiyono Budiyono

2009-09-01

Full Text Available Penitentiary was a place to conduct coaching Educate Prisoners and Child Socialization. There are pro-death penalty views (Retensionist and cons of death penalty (abolitionist on the existence of death penalty and execution. This issue is causing problems from the aspect of regulation that is the basis of service provision on death row since capital punishment on all the services there are no specific rules. The problem is the placement and service must be performed by the prisons before the execution on death row, before it is executed on death row man alive who is naturally still have rights that must be protected as a right to physical care and health until the corresponding executable , including also get their rights, as for the rights referred to was referring to the provisions of Article 14 of Act No.12/1995 about Correctional.   Kata kunci : Lembaga Pemasyarakatan,  Pidana mati, Peraturan khusus

City Connects: Redesigning Student Support for Academic Success. The Abell Report. Volume 29, No. 3

Science.gov (United States)

Manekin, Sarah

2016-01-01

Public school systems employ a range of professionals to provide support to children and youth in schools. For students living in poverty and experiencing trauma, the work of these professionals is particularly necessary and urgent. Ranging from the treatment of acute mental health issues and accommodations for students with special needs, to…

Participation in benchmark MATIS-H of NEA/OCDE: uses CFD codes applied to nuclear safety. Study of the spacer grids in the fuel elements

International Nuclear Information System (INIS)

Pena-Monferrer, C.; Chiva, S.; Munoz-cobo, J. L.; Vela, E.

2012-01-01

This paper develops participation in benchmark MATIS-H, promoted by the NEA / OECD-KAERI, involving the study of turbulent flow in a rod beam with spacers in an experimental installation. Its aim is the analysis of hydraulic behavior of turbulent flow in the subchannels of the fuel elements, essential for the improvement of safety margins in normal and transient operations and to maximize the use of nuclear energy through an optimal design of grids.