Young Galaxies and QSO Absorption-line Systems
Author: Sueli M. Viegas
Publisher:
Published: 1997
Total Pages: 200
ISBN-13:
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The Hubble Deep Field
Author: Space Telescope Science Institute (U.S.). Symposium
Publisher: Cambridge University Press
Published: 1998-10-13
Total Pages: 328
ISBN-13: 9780521630979
DOWNLOAD EBOOKThe Hubble Deep Field (HDF) is the deepest optical image of the Universe ever obtained. It is the result of a 150-orbit observing programme with the Hubble Space Telescope. It provides a unique resource for researchers studying the formation and evolution of stars and galaxies. This timely volume provides the first comprehensive overview of the HDF and its scientific impact on our understanding in cosmology. It presents articles by a host of world experts who gathered together at an international conference at the Space Telescope Science Institute. The contributions combine observations of the HDF at a variety of wavelengths with the latest theoretical progress in our understanding of the cosmic history of star and galaxy formation. The HDF is set to revolutionize our understanding in cosmology. This book therefore provides an indispensable reference for all graduate students and researchers in observational or theoretical cosmology.
QSO Absorption Lines
Author: J. Chris Blades
Publisher: Cambridge University Press
Published: 1988-08-18
Total Pages: 362
ISBN-13: 9780521345613
DOWNLOAD EBOOKThis second title in the series published for the Space Telescope Science Institute researches the current models of quasar absorption and the systems of absorption lines in the spectra of quasars. Experts in this field discuss the nature of the absorbing process in the vicinity of quasars, the "Lyman-alpha forest", metal-line systems, and quasars as probes of high redshift galaxies. The Hubble Space Telescope will be a valuable tool for learning more about the physics and astronomy of quasars.
QSO Absorption Lines
Author: Georges Meylan
Publisher: Springer Science & Business Media
Published: 2013-11-11
Total Pages: 481
ISBN-13: 3540494588
DOWNLOAD EBOOKThe controversial question of whether the majority of the narrow absorption lines observed in QSO spectra represent cosmological intervening systems or ejecta from the QSO themselves is settled. QSO absorption line spectroscopy, initially a mere technique, has matured into an essential extragalactic research tool for understanding the content of the Universe at redshifts between 0 and 4, and beyond. The only previous important meeting devoted to "QSO Absorption Lines" was held in May 1987 at the Space Telescope Science Institute in Baltimore, Maryland, U.S.A. Since that time, nearly a decade ago, research has been ex tremely active in this now well-established field of astrophysics. Theoretical stud ies and simulations have taken advantage of the constant progress in computer technology, and during these last few years, the observational results have bene fited largely from the new facillities offered by the Hubble Space Telescope in the UV wavelength range and the Keck Telescope for high-resolution spectroscopy.
The Evolution of Galaxies and Their Environment
Author: David J. Hollenbach
Publisher:
Published: 1993
Total Pages: 424
ISBN-13:
DOWNLOAD EBOOKStructure and Evolution of the Intergalactic Medium from QSO Absorption Line Systems
Author: Patrick Petitjean
Publisher: Atlantica Séguier Frontières
Published: 1997
Total Pages: 490
ISBN-13: 9782863322291
DOWNLOAD EBOOKTheoretical Astrophysics: Volume 3, Galaxies and Cosmology
Author: T. Padmanabhan
Publisher: Cambridge University Press
Published: 2000
Total Pages: 644
ISBN-13: 9780521566308
DOWNLOAD EBOOKThis timely volume provides comprehensive coverage of all aspects of cosmology and extragalactic astronomy at an advanced level. Beginning with an overview of the key observational results and necessary terminology, it covers important topics: the theory of galactic structure and galactic dynamics, structure formation, cosmic microwave background radiation, formation of luminous galaxies in the universe, intergalactic medium and active galactic nuclei. This self-contained text has a modular structure, and contains over one hundred worked exercises. It can be used alone, or in conjunction with the previous two accompanying volumes (Volume I: Astrophysical Processes, and Volume II: Stars and Stellar Systems).
The Environment and Evolution of Galaxies
Author: J.M. Shull
Publisher: Springer Science & Business Media
Published: 1993-10-31
Total Pages: 608
ISBN-13: 9780792325420
DOWNLOAD EBOOKIn July 1992, over 300 astronomers attended the Third Tetons Summer School on the subject of `The Environment and Evolution of Galaxies'. This book presents 28 papers based on invited review talks and a panel discussion on `The Nature of High Redshift Objects'. The major themes include: the Interstellar and Intergalactic Medium, Galaxy Formation and Evolution, Cooling Flows, Quasars and Radiation Backgrounds, and Interactions between Galaxies/AGNs and their Environment. Recent advances with the ROSAT, COBE and Hubble Space Telescope are discussed, together with current theoretical developments. The tutorial nature of the papers make this book a valuable supplement for professional astonomers, graduate students, and senior undergraduates. As with previous Tetons conferences, this book provides both the current state of observational and theoretical research and material complementary to courses in extragalactic and interstellar astrophysics.
Astronomical Data Analysis Software and Systems XI
Author: David A. Bohlender
Publisher:
Published: 2002
Total Pages: 588
ISBN-13:
DOWNLOAD EBOOKTowards Understanding Galaxies at Large Redshift
Author: Richard G. Kron
Publisher: Springer Science & Business Media
Published: 2012-12-06
Total Pages: 346
ISBN-13: 9400929196
DOWNLOAD EBOOKThis workshop was intended as an update and an extension of the workshop 011 the "Spectral Evolution of Galaxies" that was held in Erice two years ago. It concentrates 011 Ilew developments concerning galaxies seen at large look back times. This seemed also a good opportunity to look ahead to the next generation of ground- and space based instrumentation, and to consider various future strategies for collecting information concerning the edge of the observable universe. The main idea was to bring together people with specialities in modelling galaxy components (such as stars, clusters, gas, and dust) as well as whole stellar systems (stellar populations, star formation rates, chemical enrichment), and people specialized in making direct measurements of galaxies and clusters at large look back times. The confrontation of expectations and observations was planned to be the central theme of the conference, which explains the title "Towards Understanding Galaxies at Large Redshift". The first part of the workshop focussed on the physical processes that operate in galaxies, and that would likely have some observable manifestation at large redshifts. In the second part the most recent observational work was reported, and we were pleased to have the participation of most of the groups active in this field. The last part was directed towards new approaches to be made possible by the next generation of instrumentation, although in general all the contributions were indeed in this spirit of setting more ambitious goals.
