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The Evolution of Galaxies

III — From Simple Approaches to Self-Consistent Models

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  • © 2003

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Table of contents (136 chapters)

  1. Introduction

  2. Formation and Early Evolution of Galaxies

Keywords

About this book

Galaxies have a history. This has become clear from recent sky surveys which have shown that distant galaxies, formed early in the life of the Universe, differ from the nearby ones. New observational windows at ultraviolet, infrared and millimetric wavelengths (provided by ROSAT, IRAM, IUE, IRAS, ISO) have revealed that galaxies contain a wealth of components: very hot gas, atomic hydrogen, molecules, dust, dark matter... A significant advance is expected from the results of new instruments (VLT, FIRST, XMM) which will allow one to explore the most distant Universe.
Three Euroconferences were planned to punctuate this new epoch in galactic research, bringing together specialists in various fields of Astronomy. This book contains the proceedings of the third conference and presents the actual state-of-the-art of modelling galaxy evolution.

Editors and Affiliations

  • Institute of Theoretical Physics and Astrophysics, University of Kiel, Germany

    Gerhard Hensler, Stefan Harfst, Pavel Kroupa, Christian Theis

  • LUTH, Observatoire de Meudon, France

    Grażyna Stasińska

Bibliographic Information

  • Book Title: The Evolution of Galaxies

  • Book Subtitle: III — From Simple Approaches to Self-Consistent Models

  • Editors: Gerhard Hensler, Grażyna Stasińska, Stefan Harfst, Pavel Kroupa, Christian Theis

  • DOI: https://doi.org/10.1007/978-94-017-3315-1

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: Springer Science+Business Media Dordrecht 2003

  • Hardcover ISBN: 978-1-4020-1182-5Published: 31 July 2003

  • Softcover ISBN: 978-90-481-6248-2Published: 01 December 2010

  • eBook ISBN: 978-94-017-3315-1Published: 11 November 2013

  • Edition Number: 1

  • Number of Pages: XII, 686

  • Topics: Astronomy, Observations and Techniques, Astrophysics and Astroparticles

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