Effects of Mass Loss on Stellar Evolution

IAU Colloquium no. 59 Held in Miramare, Trieste, Italy, September 15–19, 1980

  • C. Chiosi
  • R. Stalio

Part of the Astrophysics and Space Science Library book series (ASSL, volume 89)

Table of contents

  1. Front Matter
    Pages i-xxii
  2. Winds from Early Type Stars: Observations

    1. Karel A. van der Hucht, Peter S. Conti
      Pages 35-37
    2. Mario Perinotto, Piero Benvenuti, Carla Cacciari
      Pages 45-50
    3. E. G. Tanzi, M. Tarenghi, N. Panagia
      Pages 51-56
    4. Y. Andrillat, Ch. Fehrenbach
      Pages 57-60
    5. B. Wolf, O. Stahl, W. J. Altenhoff
      Pages 61-64
    6. M. J. Barlow, L. J. Smith, A. J. Willis
      Pages 65-65
    7. S. Bensammar, S. Gaudenzi, C. Rossi, H. M. Johnson, P. S. Thé, E. J. Zuiderwijk et al.
      Pages 67-69
    8. R. Viotti, L. Rossi, F. D’Antona
      Pages 71-74
    9. S. P. Tarafdar
      Pages 79-82
    10. Roberto H. Mendez, Alberto D. Verga
      Pages 83-86
  3. Winds from Late Type Stars: Observations

    1. A. K. Dupree
      Pages 87-110
    2. T. Tanabe, F. Kamijo
      Pages 113-115

About this book

Introduction

The IAU Colloquium No. 59, "The effects of mass loss on Stellar Evolution" was held on September 15-19, 1980 at the International Centre for Theoretical Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du­ ring the IAU Symposium No. 83 "Mass loss and evolution of 0 type stars" (Qualicum Beach, Victoria, Canada) when we felt that mass loss and its effects on the evolution of stars was too broad a subject for being confined to 0 type stars only. Therefore we thought that a conference dealing with the general problem of mass loss across the whole HR diagram would have been of interest to all people working in the field. The main idea was that bringing together Astronomers and Astrophysicists of the widest range of interests and e~ pertize - all in some way related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti­ cal developments on the problem of mass loss from early ty­ pe stars avoided this meeting to be a simple updating of the Qualicum Beach Symposium as far as this issue is concerned.

Keywords

Accretion Galaxy star stars stellar

Editors and affiliations

  • C. Chiosi
    • 1
  • R. Stalio
    • 2
  1. 1.Istituto di AstronomiaPadovaItaly
  2. 2.Osservatorio AstronomicoTriesteItaly

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-009-8500-1
  • Copyright Information Springer Science+Business Media B.V. 1981
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-94-009-8502-5
  • Online ISBN 978-94-009-8500-1
  • Series Print ISSN 0067-0057
  • About this book
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