The Physical Properties In The Interstellar Medium Of Low Metallicity Dwarf Galaxies

Download The Physical Properties In The Interstellar Medium Of Low Metallicity Dwarf Galaxies full books in PDF, epub, and Kindle. Read online The Physical Properties In The Interstellar Medium Of Low Metallicity Dwarf Galaxies ebook anywhere anytime directly on your device. Fast Download speed and no annoying ads. We cannot guarantee that every ebooks is available!

The Physical Properties in the Interstellar Medium of Low-metallicity Dwarf Galaxies

Author : Diane Cormier
Publisher :
ISBN 13 :
Total Pages : 257 pages
Book Rating : 4.:/5 (866 download)

DOWNLOAD NOW!

Book Synopsis The Physical Properties in the Interstellar Medium of Low-metallicity Dwarf Galaxies by : Diane Cormier

Download or read book The Physical Properties in the Interstellar Medium of Low-metallicity Dwarf Galaxies written by Diane Cormier and published by . This book was released on 2012 with total page 257 pages. Available in PDF, EPUB and Kindle. Book excerpt: In the framework of galaxy evolution, local star-forming dwarf galaxies are ideal laboratories to study star formation processes at low metallicity and the role of metal enrichment on the physical conditions. My thesis has focused on the study of the gas properties of the dwarf galaxies from "The Herschel Dwarf Galaxy Survey", combining observations and modeling efforts. I have investigated the role of the most important tracers of the multi-phase the interstellar medium (ISM), in the mid-infrared to submillimeter range. Particular attention was paid to the ionized and neutral gas coolants observed with Herschel Space Observatory (e.g. [OIII] 88, [OI]63, [CII] 157 micron lines), and to the CO molecule, probing the molecular phase, with complementary ground-based observations. The data are interpreted in physical terms (density, radiation field, filling factors) with radiative transfer models. This work has helped elucidate the structure and conditions of the low-metallicity ISM. It highlights the porosity of the ISM of dwarf galaxies, with ultraviolet photons from the massive star-forming regions excitinig the gas out to large distances. This results in the presence of large volume filling factor diffuse ionized/neutral gas, clumpy photodissociation regions, and little observed molecular gas due to large-scale photodissociation.

Properties of the Interstellar Medium of the Star-forming Galaxy, IC10, at Various Spatial Scales

Author : Fiorella Lucia Polles
Publisher :
ISBN 13 :
Total Pages : 0 pages
Book Rating : 4.:/5 (12 download)

DOWNLOAD NOW!

Book Synopsis Properties of the Interstellar Medium of the Star-forming Galaxy, IC10, at Various Spatial Scales by : Fiorella Lucia Polles

Download or read book Properties of the Interstellar Medium of the Star-forming Galaxy, IC10, at Various Spatial Scales written by Fiorella Lucia Polles and published by . This book was released on 2017 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt: The properties of the Interstellar Medium (ISM) strongly influence the environment and processes that lead to star-formation, which in turn, drives the evolution of a galaxy. Dwarf galaxies in the Local Group are perfect laboratories to investigate how the metal-poor ISM affects the interplay between gas, dust and stars. In this thesis, I investigate the properties of the HII regions and the diffuse ionized gas of the nearby dwarf galaxy IC10, which has a metallicity of 1/3 solar. Its proximity (d=700 kpc) enables the analysis on different spatial scales: from the compact clumps (~25 pc) to the whole star-forming body of the galaxy (~650pc). In order to measure the physical properties of the ISM, I model the infrared emission lines observed with Spitzer and Herschel with photoionization and photodissociation models. I present an extensive exploration of different methods to determine the most reliable ISM properties, based on the available constraints. I determined the properties of the brightest star-forming clumps within the galaxy and show that the emission at large scales (~300 pc) is dominated by that of the compact, bright clumps that lie within the region. I further demonstrate the need for a multi-component model to fully reproduce the observations.

Constraining the Properties of the Metal-poor ISM with Interferometric CO Observations of Low Metallicity Dwarf Galaxies

Author : Edward M. Molter
Publisher :
ISBN 13 :
Total Pages : pages
Book Rating : 4.:/5 (927 download)

DOWNLOAD NOW!

Book Synopsis Constraining the Properties of the Metal-poor ISM with Interferometric CO Observations of Low Metallicity Dwarf Galaxies by : Edward M. Molter

Download or read book Constraining the Properties of the Metal-poor ISM with Interferometric CO Observations of Low Metallicity Dwarf Galaxies written by Edward M. Molter and published by . This book was released on 2015 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: Metal deficient dwarf galaxies are critical test beds for theories about the structure of star forming clouds at low metallicity, the chemical evolution of the inerstellare medium, and the conditions in the early Universe. I present new high-resolution interferometric observations of the CO (J=1{right arrow] 0) emission line in five nearby metal poor dwarf irregular dwarf galaxies taken with the CARMA array. The first half of this work considers four galaxies with very extreme metaliicites (3-10% Solar), including Leo P, DDO 68, Sextans B. While CO was not detected in any of these systems, we are able to derive very sensitive upper limits to their global CO luminosities, calculate molecular hydrogen masses using various CO-to-H2 conversion factors, and compare these results to chemical evolution models. The second half of this work consists of a case study on the interstellar medium of NGC 6822, a famous Local Group dwarf irregular galaxy at ~30% of Solar metallicity. CARMA resolves ten individual clouds of dense CO emission at ~10 pc linear scales in a central region of the galaxy\. CO luminosities and derived H2 masses are presented for each cloud, and the cloud properties are compared to similar observations in the literature. I then leverage data at a myriuad of wavelenghts to draw spatial comparisons between the distributions of dense molecular gas, atomic gas, and dust at various temperatures.

Toward the Comprehension of the Infrared to Submillimeter View of the Interstellar Medium of Nearby Galaxies

Author : Maud Galametz
Publisher :
ISBN 13 :
Total Pages : 200 pages
Book Rating : 4.:/5 (866 download)

DOWNLOAD NOW!

Book Synopsis Toward the Comprehension of the Infrared to Submillimeter View of the Interstellar Medium of Nearby Galaxies by : Maud Galametz

Download or read book Toward the Comprehension of the Infrared to Submillimeter View of the Interstellar Medium of Nearby Galaxies written by Maud Galametz and published by . This book was released on 2010 with total page 200 pages. Available in PDF, EPUB and Kindle. Book excerpt: This thesis aims to study the interstellar medium (ISM) of low-metallicity galaxies to characterize the physical properties of the gas and dust and to study the influence of metal enrichment on the ISM properties of galaxies. We adopt a multi-wavelength (infrared/submillimeter) approach to model the spectral energy distributions (SEDs) of these galaxies and showed that their fraction of cool dust can be significant compared to their total dust mass. Some dust-to-gas mass ratios are incoherent compared to what is expected from current chemical évolution models, revealing possible reservoirs of gas not detected by current HI or CO observations. I enlarged the first sample to a wider range of metallicities and showed that submm measurements significantly affect the dust mass estimates of galaxies. We also obtained submm observations of a resolved star forming complex of the Large Magellanic Cloud and studied the spatial variations of the SEDs to get a handle on the temperature distribution. I finally present the first images of dwarf galaxies with Herschel. For one of them, we modeled the SEDs of some HII regions and less active regions. The SEDs of HII regions show warmer ranges of dust temperature. We also studied the influence of using amorphous carbon to describe carbon dust in the total dust mass estimates. Our results indicate that SED models including Herschel data may require different dust properties than commonly used.

Dwarf Galaxies (IAU S344)

Author : Kristen B. W. McQuinn
Publisher : Cambridge University Press
ISBN 13 : 9781108471619
Total Pages : 500 pages
Book Rating : 4.4/5 (716 download)

DOWNLOAD NOW!

Book Synopsis Dwarf Galaxies (IAU S344) by : Kristen B. W. McQuinn

Download or read book Dwarf Galaxies (IAU S344) written by Kristen B. W. McQuinn and published by Cambridge University Press. This book was released on 2019-09-30 with total page 500 pages. Available in PDF, EPUB and Kindle. Book excerpt: Dwarf galaxies are important tools for understanding structure formation and galaxy evolution across cosmic time. These low-mass systems allow us to gain a detailed understanding of stellar, chemical, and dynamical properties in the nearby universe; they also provide a unique window into the complex physics of the early universe. The Proceedings of IAU Symposium 344 present our current understanding of dwarf galaxies, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and chemical evolution; the dwarf galaxy-environment connection; low-mass galaxies at high redshift; and dwarfs as cosmological probes. Broad overviews from leaders in the field, detailed presentation of cutting-edge results, and short summaries of a wide range of work are included for each of these topics, suitable for both experts and newcomers to the field.

Galaxies in the Local Volume

Author : Bärbel Silvia Koribalski
Publisher : Springer Science & Business Media
ISBN 13 : 1402069332
Total Pages : 375 pages
Book Rating : 4.4/5 (2 download)

DOWNLOAD NOW!

Book Synopsis Galaxies in the Local Volume by : Bärbel Silvia Koribalski

Download or read book Galaxies in the Local Volume written by Bärbel Silvia Koribalski and published by Springer Science & Business Media. This book was released on 2009-04-29 with total page 375 pages. Available in PDF, EPUB and Kindle. Book excerpt: This timely book presents an overview of the galaxies within the Local Volume, including the Local Group and our closest neighbours, the Andromeda Galaxy and the Magellanic Clouds. Presented here are the latest results from radio, infrared and optical surveys as well as detailed multi-wavelength studies of individual galaxies. The book aims to provide a vibrant forum for presentations and discussions across a broad range of astrophysical topics.

The Interstellar Medium in Galaxies

Author : J.M. van der Hulst
Publisher : Springer Science & Business Media
ISBN 13 : 9401156204
Total Pages : 217 pages
Book Rating : 4.4/5 (11 download)

DOWNLOAD NOW!

Book Synopsis The Interstellar Medium in Galaxies by : J.M. van der Hulst

Download or read book The Interstellar Medium in Galaxies written by J.M. van der Hulst and published by Springer Science & Business Media. This book was released on 2013-12-01 with total page 217 pages. Available in PDF, EPUB and Kindle. Book excerpt: It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen tal developments over the past decade: large CCD's became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an "outside" view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way.

Properties and Kinematics of the Interstellar Medium in a Small Sample of Nearby Dwarf Galaxies

Author : Lisa Marie Young
Publisher :
ISBN 13 :
Total Pages : 334 pages
Book Rating : 4.:/5 (389 download)

DOWNLOAD NOW!

Book Synopsis Properties and Kinematics of the Interstellar Medium in a Small Sample of Nearby Dwarf Galaxies by : Lisa Marie Young

Download or read book Properties and Kinematics of the Interstellar Medium in a Small Sample of Nearby Dwarf Galaxies written by Lisa Marie Young and published by . This book was released on 1997 with total page 334 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Highlights of Astronomy, Volume 11A

Author : Johannes Andersen
Publisher : Springer Science & Business Media
ISBN 13 : 9780792353416
Total Pages : 632 pages
Book Rating : 4.3/5 (534 download)

DOWNLOAD NOW!

Book Synopsis Highlights of Astronomy, Volume 11A by : Johannes Andersen

Download or read book Highlights of Astronomy, Volume 11A written by Johannes Andersen and published by Springer Science & Business Media. This book was released on 1999-01-31 with total page 632 pages. Available in PDF, EPUB and Kindle. Book excerpt: Since 1967, the main scientific events of the General Assemblies of the International Astronomical Union have been published in the separate series, Highlights of Astronomy. The present Volume 11 presents the major scientific presentations made at the XXIIIrd General Assembly, August 18-30, 1997, in Kyoto, Japan. The two volumes (11A + B) contain the text of the three Invited Discourses as well as the proceedings or extended summaries of the 21 Joint Discussions and two Special Sessions held during the General Assembly.

Old Stellar Populations

Author : Santi Cassisi
Publisher : John Wiley & Sons
ISBN 13 : 3527665544
Total Pages : 506 pages
Book Rating : 4.5/5 (276 download)

DOWNLOAD NOW!

Book Synopsis Old Stellar Populations by : Santi Cassisi

Download or read book Old Stellar Populations written by Santi Cassisi and published by John Wiley & Sons. This book was released on 2013-08-29 with total page 506 pages. Available in PDF, EPUB and Kindle. Book excerpt: The book discusses the theoretical path to decoding the information gathered from observations of old stellar systems. It focuses on old stellar systems because these are the fossil record of galaxy formation and provide invaluable information ont he evolution of cosmic structures and the universe as a whole. The aim is to present results obtained in the past few years for theoretical developments in low mass star research and in advances in our knowledge of the evolution of old stellar systems. A particularly representative case is the recent discovery of multiple stellar populations in galactic globular clusters that represents one of the hottest topics in stellar and galactic astrophysics and is discussed in detail. Santi Cassisi has authored about 270 scientific papers, 150 of them in peer-reviewed journals, and the title Evolution of Stars and Stellar Populations.

Characterizing the Interstellar and Circumgalactic Medium in Distant Star-Forming Galaxies

Author : Xinnan Du
Publisher :
ISBN 13 :
Total Pages : 191 pages
Book Rating : 4.:/5 (19 download)

DOWNLOAD NOW!

Book Synopsis Characterizing the Interstellar and Circumgalactic Medium in Distant Star-Forming Galaxies by : Xinnan Du

Download or read book Characterizing the Interstellar and Circumgalactic Medium in Distant Star-Forming Galaxies written by Xinnan Du and published by . This book was released on 2018 with total page 191 pages. Available in PDF, EPUB and Kindle. Book excerpt: Rest-frame ultraviolet (UV) and optical spectroscopy provides valuable information on the physical properties of the neutral and ionized interstellar medium (ISM) in star-forming galaxies. Such observations probe both the systemic interstellar component originating from H II regions, and the multi-phase outflowing component that is associated with star-formation feedback and can ultimately contribute to the circumgalactic and even intergalactic medium (CGM and IGM, respectively). In this dissertation, I investigate the physical properties of ionized gas in star-forming regions, and the kinematics and evolution of the multi-phase outflowing ISM/CGM in distant star-forming galaxies spanning the redshift range z ~ 1-4. This work consists of three studies that examine different aspects of the ISM and CGM, which collectively improve our understanding of the gas content in galaxies and the processes associated with the formation of massive stars near the peak of the star-formation-rate (SFR) density in the universe. I present a comparison of kinematics between the low- and high-ionization absorption features at z ~ 1, and demonstrate that the apparent larger blueshift of interstellar C IV relative to the low-ionization features is likely a result from the nature of resonant transitions instead of an evidence of the faster motion of the highly ionized gas. I further investigate the origin of the highly ionized gas by examining the correlations between the spectral properties of C IV and various galaxy properties. Both the blueshift and equivalent width (EW) of C IV are modulated by SFR and specific SFR, suggesting a direct connection between the highly ionized gas and the formation of massive stars. Nebular emission features provide valuable insights into the physical conditions of the ionized gas in H II regions, as well as the properties of young, massive stars. I show that the nebular C III] emission at z ~ 1 is much weaker compared to the detections from galaxies observed during the epoch of reionization (z > 6), and explore the factors that modulate the strength of this nebular feature. In combination with the results from photoionization models, I further infer the gas-phase metallicity and abundance pattern in the z ~ 1 star-forming galaxies based on the observed rest-frame C III] EW. Studying the lower-redshift analogs of the z > 6 C III] emitters is an alternative way to obtain more detailed information on the physical properties of these extreme-emission-line-galaxies (EELGs). By assembling a sample of EELGs at z ~ 1-2 and examining C III] and other nebular emission features, I aim to characterize the physical conditions of the z > 6 galaxies that are likely responsible for the cosmic reionization. Finally, with carefully constructed samples and uniform measurements, I investigate the evolution of the ISM/CGM at z ~ 2-4 as probed by rest-UV spectroscopy. I discover redshift-independent correlations among Lya emission, low-ionization interstellar absorption lines, and dust extinction. I further show that the covering fraction of neutral gas decreases with increasing redshift at multiple fixed galaxy properties. Gaining a full understanding of galaxy evolution requires further studies of the ISM/CGM in a systemic manner at higher redshifts. With exceptional capabilities in the near-IR and excellent spectroscopic sensitivity, the next generation of large telescopes will enable rest-UV and rest-optical spectroscopic studies of star-forming galaxies out to z > 10. Answering key questions regarding the interplay among massive stars, their contribution to the ionizing background, and feedback will deliver a clear picture of the formation and evolution of these distant star-forming galaxies.

Planets, Stars and Stellar Systems

Author : Gerard Gilmore
Publisher : Springer
ISBN 13 : 9789400756113
Total Pages : 0 pages
Book Rating : 4.7/5 (561 download)

DOWNLOAD NOW!

Book Synopsis Planets, Stars and Stellar Systems by : Gerard Gilmore

Download or read book Planets, Stars and Stellar Systems written by Gerard Gilmore and published by Springer. This book was released on 2013-02-23 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt: This is volume 5 of Planets, Stars and Stellar Systems, a six-volume compendium of modern astronomical research, covering subjects of key interest to the main fields of contemporary astronomy. This volume on “Galactic Structure and Stellar Populations”, edited by Gerard F. Gilmore, presents accessible review chapters on Stellar Populations, Chemical Abundances as Population Tracers, Metal-Poor Stars and the Chemical Enrichment of the Universe, The Stellar and Sub-Stellar Initial Mass Function of Simple and Composite Populations, The Galactic Nucleus, The Galactic Bulge, Open Clusters and Their Role in the Galaxy, Star Counts and the Nature of Galactic Thick Disk, The Infrared Galaxy, Interstellar PAHs and Dust, Galactic Neutral Hydrogen, High-Velocity Clouds, Magnetic Fields in Galaxies, Astrophysics of Galactic Charged Cosmic Rays, Gamma-Ray Emission of Supernova Remnants and the Origin of Galactic Cosmic Rays, Galactic Distance Scales, Globular Cluster Dynamical Evolution, Dynamics of Disks and Warps, Mass Distribution and Rotation Curve in the Galaxy, Dark Matter in the Galactic Dwarf Spheroidal Satellites, and History of Dark Matter in Galaxies. All chapters of the handbook were written by practicing professionals. They include sufficient background material and references to the current literature to allow readers to learn enough about a specialty within astronomy, astrophysics and cosmology to get started on their own practical research projects. In the spirit of the series Stars and Stellar Systems published by Chicago University Press in the 1960s and 1970s, each chapter of Planets, Stars and Stellar Systems can stand on its own as a fundamental review of its respective sub-discipline, and each volume can be used as a textbook or recommended reference work for advanced undergraduate or postgraduate courses. Advanced students and professional astronomers in their roles as both lecturers and researchers will welcome Planets, Stars and Stellar Systems as a comprehensive and pedagogical reference work on astronomy, astrophysics and cosmology.

Chemical Evolution of Galaxies

Author : Francesca Matteucci
Publisher : Springer Science & Business Media
ISBN 13 : 3642224911
Total Pages : 237 pages
Book Rating : 4.6/5 (422 download)

DOWNLOAD NOW!

Book Synopsis Chemical Evolution of Galaxies by : Francesca Matteucci

Download or read book Chemical Evolution of Galaxies written by Francesca Matteucci and published by Springer Science & Business Media. This book was released on 2012-01-05 with total page 237 pages. Available in PDF, EPUB and Kindle. Book excerpt: The term “chemical evolution of galaxies” refers to the evolution of abundances of chemical species in galaxies, which is due to nuclear processes occurring in stars and to gas flows into and out of galaxies. This book deals with the chemical evolution of galaxies of all morphological types (ellipticals, spirals and irregulars) and stresses the importance of the star formation histories in determining the properties of stellar populations in different galaxies. The topic is approached in a didactical and logical manner via galaxy evolution models which are compared with observational results obtained in the last two decades: The reader is given an introduction to the concept of chemical abundances and learns about the main stellar populations in our Galaxy as well as about the classification of galaxy types and their main observables. In the core of the book, the construction and solution of chemical evolution models are discussed in detail, followed by descriptions and interpretations of observations of the chemical evolution of the Milky Way, spheroidal galaxies, irregular galaxies and of cosmic chemical evolution. The aim of this book is to provide an introduction to students as well as to amend our present ideas in research; the book also summarizes the efforts made by authors in the past several years in order to further future research in the field.

Hot Interstellar Matter in Elliptical Galaxies

Author : Dong-Woo Kim
Publisher : Springer
ISBN 13 : 9781461429807
Total Pages : 284 pages
Book Rating : 4.4/5 (298 download)

DOWNLOAD NOW!

Book Synopsis Hot Interstellar Matter in Elliptical Galaxies by : Dong-Woo Kim

Download or read book Hot Interstellar Matter in Elliptical Galaxies written by Dong-Woo Kim and published by Springer. This book was released on 2013-11-29 with total page 284 pages. Available in PDF, EPUB and Kindle. Book excerpt: Based on a number of new discoveries resulting from 10 years of Chandra and XMM-Newton observations and corresponding theoretical works, this is the first book to address significant progress in the research of the Hot Interstellar Matter in Elliptical Galaxies. A fundamental understanding of the physical properties of the hot ISM in elliptical galaxies is critical, because they are directly related to the formation and evolution of elliptical galaxies via star formation episodes, environmental effects such as stripping, infall, and mergers, and the growth of super-massive black holes. Thanks to the outstanding spatial resolution of Chandra and the large collecting area of XMM-Newton, various fine structures of the hot gas have been imaged in detail and key physical quantities have been accurately measured, allowing theoretical interpretations/predictions to be compared and tested against observational results. This book will bring all readers up-to-date on this essential field of research.

Low-metallicity Star Formation (IAU S255)

Author : International Astronomical Union. Symposium
Publisher :
ISBN 13 :
Total Pages : 448 pages
Book Rating : 4.3/5 (91 download)

DOWNLOAD NOW!

Book Synopsis Low-metallicity Star Formation (IAU S255) by : International Astronomical Union. Symposium

Download or read book Low-metallicity Star Formation (IAU S255) written by International Astronomical Union. Symposium and published by . This book was released on 2008 with total page 448 pages. Available in PDF, EPUB and Kindle. Book excerpt: Although low-mass metal-poor galaxies in the local universe have often been proposed as the 'primordial building blocks' in the hierarchical scenario of structure formation, several lines of evidence suggest that this may not be true. Moreover, it is not clear to what extent dwarf galaxies, because they are metal poor and because of their kinematics and structure, can tell us about how star formation proceeded in the early universe. This volume provides an overview and the most recent advances in this debate. IAU Symposium 255 presents the most up-to-date developments in six key areas, including: Population III and metal-free star formation; metal-enrichment, chemical evolution and feedback; explosive events in low-metallicity environments; dust and gas as seeds for metal-poor star formation; metal-poor initial mass functions, stellar evolution and star-formation histories; and low-metallicity star formation in the local universe. This overview is at a level suitable for research astronomers and graduate students.

Literature 1991, Part 2

Author : Astronomisches Rechen-Institut
Publisher : Springer Science & Business Media
ISBN 13 : 3662123762
Total Pages : 1592 pages
Book Rating : 4.6/5 (621 download)

DOWNLOAD NOW!

Book Synopsis Literature 1991, Part 2 by : Astronomisches Rechen-Institut

Download or read book Literature 1991, Part 2 written by Astronomisches Rechen-Institut and published by Springer Science & Business Media. This book was released on 2013-06-29 with total page 1592 pages. Available in PDF, EPUB and Kindle. Book excerpt: "Astronomy and Astrophysics Abstracts" appearing twice a year has become oneof the fundamental publications in the fields of astronomy, astrophysics andneighbouring sciences. It is the most important English-language abstracting journal in the mentioned branches. The abstrats are classified under more than a hundred subject categories, thus permitting a quick survey of the whole extended material. The AAA is a valuable and important publication for all students and scientists working in the fields of astronomy and related sciences. As such it represents a necessary ingredient of any astronomical library all over the world.

Near-Field Cosmology with Dwarf Elliptical Galaxies (IAU C198)

Author : International Astronomical Union. Colloquium
Publisher : Cambridge University Press
ISBN 13 : 9780521852043
Total Pages : 456 pages
Book Rating : 4.8/5 (52 download)

DOWNLOAD NOW!

Book Synopsis Near-Field Cosmology with Dwarf Elliptical Galaxies (IAU C198) by : International Astronomical Union. Colloquium

Download or read book Near-Field Cosmology with Dwarf Elliptical Galaxies (IAU C198) written by International Astronomical Union. Colloquium and published by Cambridge University Press. This book was released on 2005 with total page 456 pages. Available in PDF, EPUB and Kindle. Book excerpt: Proceedings of IAUC 198, covering important issues related to near-field cosmology with dwarf elliptical galaxies.