Galaxies at High Redshift

Galaxies at High Redshift

Author: I. Pérez-Fournon

Publisher: Cambridge University Press

Published: 2003-03-20

Total Pages: 302

ISBN-13: 9780521825917

DOWNLOAD EBOOK

This volume presents lectures of the XI Canary Islands Winter School of Astrophysics written by experts in the field.


Lyman Alpha Emitting Galaxies at High Redshift

Lyman Alpha Emitting Galaxies at High Redshift

Author: Steven Arthur Dawson

Publisher: Universal-Publishers

Published: 2005

Total Pages: 203

ISBN-13: 1581122942

DOWNLOAD EBOOK

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.


Galaxy Interactions at Low and High Redshift

Galaxy Interactions at Low and High Redshift

Author: International Astronomical Union. Symposium

Publisher: Springer Science & Business Media

Published: 1999-09-30

Total Pages: 560

ISBN-13: 9780792358329

DOWNLOAD EBOOK

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.


The Environment and Evolution of Galaxies

The Environment and Evolution of Galaxies

Author: J.M. Shull

Publisher: Springer Science & Business Media

Published: 2012-12-06

Total Pages: 597

ISBN-13: 9401118825

DOWNLOAD EBOOK

In 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.


The Hubble Deep Field

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 EBOOK

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.


ESSCIRC '97

ESSCIRC '97

Author: H. Grünbacher

Publisher: Atlantica Séguier Frontières

Published: 1997

Total Pages: 462

ISBN-13: 9782863322208

DOWNLOAD EBOOK


Building Galaxies: From The Primordial Universe To The Present, Procs Of The Xixth Rencontres De Moriond

Building Galaxies: From The Primordial Universe To The Present, Procs Of The Xixth Rencontres De Moriond

Author: Veronique Cayatte

Publisher: World Scientific

Published: 2000-07-17

Total Pages: 494

ISBN-13: 9814542776

DOWNLOAD EBOOK

These proceedings provide a summary of the state-of-the-art in the understanding of physical processes which control galaxy formation. Many topics are discussed which present the latest observational results: dust extinction, the role of AGNs in the formation of massive galaxies, etc. How future instruments such as NGST, ALMA, FIRST, KMT and SKAI can help to resolve these questions is also addressed. The book will serve as a useful reference in the field for many years to come.


The Epoch of Galaxy Formation

The Epoch of Galaxy Formation

Author: Carlos S. Frenk

Publisher: Springer Science & Business Media

Published: 2012-12-06

Total Pages: 442

ISBN-13: 9400909195

DOWNLOAD EBOOK

Scientists in the late twentieth century are not the first to view galaxy formation as a phenomenon worthy of explanation in terms of the known laws of physics. Already in 1754 Kant regarded the problem as essentially solved. In his Univerlal Natural Hutory and Theory 0/ the H eaven$ he wrote; "If in the immesurable space in which all the suns of the Milky Way have formed themselves, we assume a point around which, through some cause or other, the first formation of nature out of chaoo began, there the largest mass and a body of extraordinary attraction will have arisen which has thereby become capable of compelling all the systems in the process of being formed within an enormous sphere around it, to fall towards itself as their centre, and to build up a system around it on the great scale . . . . Observation puts this conjecture almost beyond doubt. " More than 200 years later, a similar note of confidence was voiced by Zel'dovicb at an IAU symposium held in Tallin in 1911; "Extrapolating . . . to the next symposium somewhere in the early eighties one can be pretty sure that the question of the formation of galaxies and clusters will be solved in the next few years. " Perhaps few astronomers today would share Kant's near certainty or feel that Zel'dovich's prophecy has been fulfilled, Many, however, will sympathize with the optimistic olltlook of these two statements.