Overview
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.
Full Product Details
Author: Immo Appenzeller
Publisher: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG
Imprint: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
Edition: 2009 ed.
Dimensions:
Width: 15.50cm
, Height: 1.80cm
, Length: 23.50cm
Weight: 0.738kg
ISBN: 9783540758235
ISBN 10: 3540758232
Pages: 352
Publication Date: 09 July 2009
Audience:
Professional and scholarly
,
Professional & Vocational
Format: Hardback
Publisher's Status: Active
Availability: In Print
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Reviews
From the reviews: This ambitious book aims to summarize our view of high-redshift galaxies and their contents. ! He describes how to find high-redshift objects, how to characterize them, how to deal with selection effects, and so on. ! Appenzeller has done a fine job in summarizing the study of high-redshift galaxies and this will act as an excellent introduction to the subject for students and researchers. (Paul O'Brien, The Observatory, Vol. 130 (1214), February, 2010)
Aus den Rezensionen: ! Hochwillkommen ist ! ein Buch, das die bisherigen Forschungsergebnisse zusammenfasst und einer breiteren Leserschaft zuganglich macht. Die Zielgruppe des Autors sind nicht nur Astronomen, sondern alle Wissenschaftler mit Kenntnissen der Physik. ! Das Buch endet mit einem Ausblick in die Zukunft ! Einfluss auf die Forschung vorgestellt. ! Dieses Buch ist in einem sachlich-nuchternem Stil geschrieben und ist ausserst nutzlich fur ! Studenten und Dozenten. Es eignet sich aber auch fur den aktiven Wissenschaftler als Einfuhrung in das Thema oder einen raschen Auberblick. (JOSEF FRIED, in: Sterne und Weltraum, June/2010, Issue 6, S. 112)
Author Information
Prof. Immo Appenzeller is the emeritus director of the Heidelberg Observatory (Landessternwarte Heidelberg). From 1994 - 1997 he served as General Secretary of the International Astronomical Union. He was PI or CO of various large national and international instrumentation and research projects. His current main research topics are very distant (young) galaxies, active galaxies and QSOs, massive luminous stars, cosmic X-ray sources, astronomical instrumentation.
