Galaxy Evolution in Groups and Clusters

A JENAM 2002 Workshop Porto, Portugal 3–5 September 2002

  • Catarina Lobo
  • Margarida Serote Roos
  • Andrea Biviano

Table of contents

  1. Front Matter
    Pages i-vi
  2. Properties and Evolution of Galaxies in Groups and Clusters

    1. Front Matter
      Pages 7-7
    2. E. Ellingson
      Pages 9-18
    3. Marisa Girardi, Fabio Mardirossian, Marino Mezzetti, Enrico Rigoni
      Pages 31-35
    4. Marc E. Zimer, Ann I. Zabludoff, John S. Mulchaey
      Pages 37-42
    5. Roberto De Propris, S. A. Stanford, Peter Eisenhardt, Mark Dickinson
      Pages 43-47
  3. The Evolution of Brightest Cluster Galaxies

    1. Front Matter
      Pages 49-49
    2. Chris Collins, Sarah Brough, Doug Burke, Robert Mann, Paul Lynam
      Pages 51-60
    3. Alexander Fritz, Bodo L. Ziegler, Richard G. Bower, Ian Smail, Roger L. Davies
      Pages 61-66
    4. Anthony H. Gonzalez, Ann I. Zabludoff, Dennis Zaritsky
      Pages 67-71
    5. Dajana Džanović, R. M. Sharples, A. J. Benson, C. S. Frenk
      Pages 73-77
    6. Reinaldo De Carvalho, Ignacio De La Rosa, Steve Zepf
      Pages 79-84
  4. Dwarfs and Low Surface Brightness Galaxies in Clusters

    1. Front Matter
      Pages 85-85
    2. L. Infante, Steffen Mieske, M. Hilker
      Pages 87-96
    3. L. Makarova, E. Grebel, I. Karachentsev, A. Dolphin, V. Karachentseva, M. Sharina et al.
      Pages 107-111
    4. Michael D. Gregg, Michael J. Drinkwater, Michael J. Hilker, Steven Phillipps, J. Bryn Jones
      Pages 113-117
  5. Spectral, Morphological and Color Transformations of Cluster Galaxies

    1. Front Matter
      Pages 119-119

About this book

Introduction

Galaxy groups and clusters provide excellent laboratories for studying galaxy properties in different environments and at different look-back times. In particular, the recent detections of high-redshift cluster candidates, only possible with the current high-technology instrumentation, add a new dimension to the problem. Along with the ever increasing computing power and sophisticated algorithms to model clusters of galaxies, it may help us to understand the origins of today's groups and clusters, as well as of their member galaxies. These workshop proceedings provide a snapshot of the current research in this subject, covering the observations, theory and numerical simulations relevant to galaxy evolution in groups and clusters. In this book, intended primarily to researchers in the field, particular emphasis is given to the recent impressive progress in the field, on important new results, and on the future prospects and open questions to be tackled.

Keywords

Population Redshift Universe X-ray cluster density dispersion environment environmental effects evolution feedback galaxy iron morphology segregation

Editors and affiliations

  • Catarina Lobo
    • 1
  • Margarida Serote Roos
    • 2
  • Andrea Biviano
    • 3
  1. 1.Centro de Astrofísica e Faculdade de CiencasUniversidade do PortoPortugal
  2. 2.Centro de Astronnomia e AstrofísicaUniversidade de LisboaPortugal
  3. 3.INAF — Osservatorio Astronomico di TriesteItaly

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-010-0107-6
  • Copyright Information Kluwer Academic Publishers 2003
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-94-010-3975-8
  • Online ISBN 978-94-010-0107-6
  • About this book
Industry Sectors
Aerospace