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Spectral Evolution of Galaxies

Proceedings of the Fourth Workshop of the Advanced School of Astronomy of the “Ettore Majorana” Centre for Scientific Culture, Erice, Italy, March 12–22, 1985

  • Cesare Chiosi
  • Alvio Renzini

Part of the Astrophysics and Space Science Library book series (ASSL, volume 122)

Table of contents

  1. Front Matter
    Pages i-xii
  2. Introductory Lecture

    1. Front Matter
      Pages 1-1
  3. Galaxy and Star Formation Processes

  4. Stellar Populations in the Local Group

    1. Front Matter
      Pages 131-131
    2. Jay A. Frogel
      Pages 143-156
    3. A. E. Whitford
      Pages 157-170
    4. M. Aaronson, K. H. Cook, J. Norris
      Pages 171-181
  5. Towards Modelling the Spectral Evolution of Galaxies

  6. Empirical Population Synthesis

    1. Front Matter
      Pages 319-319
    2. Robert W. O’Connell
      Pages 321-343
    3. B. Rocca-Volmerange, B. Guiderdoni
      Pages 357-362
    4. Francesco Bertola
      Pages 363-367
    5. R. Nesci
      Pages 369-371
  7. Galaxies at Large Lookback Times

    1. Front Matter
      Pages 373-373
    2. Donald Hamilton
      Pages 391-401
    3. Peter R. M. Eisenhardt
      Pages 403-410
    4. B. Guiderdoni, B. Rocca-Volmerange
      Pages 411-418
    5. P. R. F. Stevenson, T. Shanks, R. Fong
      Pages 439-446
  8. Chemical Evolution of Galaxies and Miscellanea

    1. Front Matter
      Pages 447-447
    2. R. Güsten
      Pages 449-467
    3. M. Tosi, Angeles I. Diaz
      Pages 469-472
    4. M. A. Shaw, G. F. Gilmore
      Pages 477-484
  9. Back Matter
    Pages 485-490

About these proceedings

Introduction

As it was said by one of the participants to this workshop" In our attempts to understand the spectral evolution of galaxies, we are fortunate indeed to have the ability to look back in time and observe galaxies as they were billions of years ago. Perhaos in no other discipline is it possible to gain such a direct view to hJstory. The galaxies we seek to study are remote, their light faint, and thus only recently has it become technicaJlv feasible to sample the spectra of normal luminosity galaxies at lookback times of five billion years or more" .... or, perhaps. even to see galaxies in the process of their formation. or shortly afterwards. This fourth workshop organized by the "Advanced School ot Astronomy was indeed centered on the "Spectral Evolution of Galaxies". on reviewing and discussing the relevant astrophysical processes and on assessing our current ability to model and understand the evolution of stellar populations. Following an opening session dealing with some outstanding questions of galaxy evolution. Session I addressed the specific problems of galaxy and star formation processes. topics of uncertainty and controversy to which IRAS observations may give novel perspectives. The properties of stellar populations in the local group of galaxies formed the basis of Session II. Session III dealt with the fundaments of the theory of spectral and photometrical evolution of stellar populations. and with recent developments in the theory of stellar structure. a necessary step to model and understand galactic evolution.

Keywords

Bulge Galaxy astronomy star stellar

Editors and affiliations

  • Cesare Chiosi
    • 1
  • Alvio Renzini
    • 2
  1. 1.Institute of AstronomyUniversity of PadovaItaly
  2. 2.Department of AstronomyUniversity of BolognaItaly

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-009-4598-2
  • Copyright Information Springer Science+Business Media B.V. 1986
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-94-010-8543-4
  • Online ISBN 978-94-009-4598-2
  • Series Print ISSN 0067-0057
  • Buy this book on publisher's site