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Author: Space Telescope Science Institute (U.S.). Symposium
Publisher: Cambridge University Press
ISBN: 9780521630979
Category : Science
Languages : en
Pages : 328
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Book Description
The 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.
Author: Space Telescope Science Institute (U.S.). Symposium
Publisher: Cambridge University Press
ISBN: 9780521630979
Category : Science
Languages : en
Pages : 328
Get Book Here
Book Description
The 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.
Author: Immo Appenzeller
Publisher: Springer Science & Business Media
ISBN: 3540758240
Category : Science
Languages : en
Pages : 353
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Book Description
The high-redshift galaxies became a distinct research ?eld during the ?nal decade of the20thcentury. AtthattimetheLyman-breaktechniquemadeitpossibletoidentify signi?cant samples of such objects, and the new generation of 8 to 10-m telescopes resulted in ?rst good spectroscopic data. Today the high-redshift galaxies have developed into one of the important topics of astrophysics, accounting for about 5–10% of the publications in the major scienti?c journals devoted to astronomy. Because high-redshift galaxies is a rapidly developing ?eld and since new results are published constantly, writing a book on this topic is challenging. On the other hand, in view of the large amount of individual results now in the literature, and in view of the still growing interest in this topic, it appears worthwhile to summarize and evaluate the available data and to provide an introduction for those who wish to enter this ?eld, or who, for various reasons, might be interested in its results. The end of the ?rst decade of the 21st century appears to be a good point in time to attempt such a summary. The current generation of ground-based 8 to 10-m - optical telescopes, the Hubble Space Telescope, and the most important large radio telescopes have by now been in operation since about one or two decades. Although these instruments will continue to produce important scienti?c results for some time to come, many of the initial programs exploiting their unique new possibilities have been completed.
Author: I. Pérez-Fournon
Publisher: Cambridge University Press
ISBN: 9780521825917
Category : Science
Languages : en
Pages : 302
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Book Description
This volume presents lectures of the XI Canary Islands Winter School of Astrophysics written by experts in the field.
Author: J.E. Barnes
Publisher: Springer Science & Business Media
ISBN: 9401146659
Category : Science
Languages : en
Pages : 530
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Book Description
These proceedings offer professional astronomers an overview of the rapidly advancing subject of galaxy interactions at low and high redshifts. The symposium gave participants an exciting glimpse of a developing synthesis highlighting galactic encounters and their role in the history of the Universe.
Author: Steven Arthur Dawson
Publisher: Universal-Publishers
ISBN: 1581122942
Category : Science
Languages : en
Pages : 203
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Book Description
As late as 1995, the anticipated widespread population of primeval galaxies remained at large, lurking undetected at unknown redshifts, with undiscovered properties. We present results from our efforts to detect and characterize primeval galaxies by their signature high-redshift Lyman-alpha emission lines utilizing two observational techniques: serendipitous slit spectroscopy and narrowband imaging. By pushing these techniques to their utmost limits, we probe the Lyman-alpha-emitting galaxy population out to redshifts as high as z = 6.5. Galaxies at this epoch reside in a universe which is just 800 million years old, a mere 6% of its current age. As such, this work provides one account of the manner by which observational cosmology has recently shifted from merely marveling at the incredible lookback times implied by the first few high-redshift detections, to the routine assembly of high-redshift datasets designed to address specific astrophysical issues.
Author: Halton C. Arp
Publisher: Cambridge University Press
ISBN: 9780521363143
Category : Science
Languages : en
Pages : 220
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Book Description
Contests the 'establishment' view of quasars as the most distant objects in the universe.
Author: Jacqueline Bergeron
Publisher: Atlantica Séguier Frontières
ISBN: 9782863320518
Category : Astrophysics
Languages : en
Pages : 548
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Book Description
Author: Jose Kam
Publisher: Independently Published
ISBN: 9781093540628
Category :
Languages : en
Pages : 356
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Book Description
The high-redshift galaxies became a separate research? During the nineties of the 20th century AtthattimetheLyman-breaktechniqumadeitpossibletoidentify signi? Cant samples of such items, and a new generation of 8 to 10-meter binoculars? Rst good spectroscopic data? Today, high-redshift galaxies have been developed in one of the important topics in astronomy, accounting for approximately 5-10% of publications in leading scientists? C magazines are dedicated to astronomy. Because the high-redshift galaxy is growing rapidly? Since large and new results are constantly published, it is challenging to write a book on this topic. On the other hand, considering the large amount of personal results now in the literature, and considering the increasing interest in this subject, it is worthwhile to summarize and evaluate the available data and provide an introduction to those seeking it. To enter it? Elderly, or who, for various reasons, may be interested in its consequences. The decade of the 21st century appears to be a good point to try such summaries. The current generation of 8 to 10 meters based on the ground - optical telescope, the Hubble Space Telescope, and the most important large radio telescope have been running for almost a decade or so. Although these instruments will continue to produce significant scientific, some results for the coming time, many early programs that have taken advantage of their unique new possibilities have been completed.
Author: Ralf Bender
Publisher: Springer Science & Business Media
ISBN: 9783540002055
Category : Science
Languages : en
Pages : 394
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Book Description
Measuring the masses of galaxies as a function of redshift is perhaps one of the most challenging open issues in current astronomical research. The evolution of the baryonic and dark matter components of galaxies is not only a critical test of the hierarchical formation paradigm, but ultimately also provides new clues on the complex interplay between star formation, the cooling and heating of gas and galaxy merging processes. This book reviews current techniques to measure the baryonic (stellar) and dark masses of nearby galaxies, and focusses on ongoing attempts to measure theses same quantities in galaxies at higher and higher redshifts. It also gives room to future perspectives, with special emphasis on new survey projects and satellite missions.
Author: Sugata Kaviraj
Publisher: Cambridge University Press
ISBN: 9781107138261
Category : Science
Languages : en
Pages : 0
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Book Description
IAU Symposium 319 was the largest galaxy evolution meeting at the IAU General Assembly in 2015. This volume presents a summary of the current state of the art in galaxy evolution studies, and provides a perspective on future large spectro-photometric surveys which will become available in the next decade. Topics covered include the emergence of galaxies and their constituent black holes during the first few billion years, the evolving interstellar medium as seen through modern instrumentation like Herschel, Planck and ALMA, and a look ahead to future ground- and space-based instruments that will become the workhorse facilities of the next decade, such as JWST and the SKA precursors. This volume will appeal to those who are interested in the formation and evolution of galaxies over cosmic time, as well as those who are active in developing, or on the science teams for, new astronomical instrumentation.
