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Late Stages of Stellar Evolution Computational Methods in Astrophysical Hydrodynamics

Proceedings of the Astrophysics School II Organized by the European Astrophysics Doctoral Network at Ponte de Lima Portugal, 11–23 September 1989

  • Editors
  • C. B. de Loore

Part of the Lecture Notes in Physics book series (LNP, volume 373)

Table of contents

  1. Front Matter
  2. Camiel Bert de Loore
    Pages 2-95
  3. Alain Omont
    Pages 161-211
  4. Jean Heyvaerts
    Pages 313-354
  5. Jean-Paul Zahn
    Pages 355-390
  6. Back Matter

About these proceedings

Introduction

This collection of 7 lectures is intended to be a textbook for graduate students who want to learn about modern developments in astronomy and astrophysics. The first part surveys various aspects of the late stages of stellar evolution, including observation and theory. B.C. de Loore's long article on stellar structure is followed by reviews on supernovae, on circumstellar envelopes, and on the evolution of binaries. The second part deals with the important problem of modeling stellar evolution based on the computational hydrodynamics.

Keywords

Astrophysik astrophysics computational hydrodynamics stellar evolution stellar structure

Bibliographic information

  • DOI https://doi.org/10.1007/BFb0032277
  • Copyright Information Springer-Verlag 1991
  • Publisher Name Springer, Berlin, Heidelberg
  • eBook Packages Springer Book Archive
  • Print ISBN 978-3-540-53620-8
  • Online ISBN 978-3-540-46921-6
  • Series Print ISSN 0075-8450
  • Series Online ISSN 1616-6361
  • Buy this book on publisher's site