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Stellar Evolution

  • A. G. W. Cameron
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 22)

Abstract

In these lectures I shall concentrate on those aspects of Stellar Evolution which appear relevant to the study of the structure and the evolution of the Galaxy. I shall not review the techniques used for the numerical computation of stellar evolution, but will assume that the interested reader can consult standard reference works for such topics. The lectures by Professor Ledoux discuss the formation of stars from the interstellar gas. Here we shall be concerned with the reverse process, in which stars lose mass back to the interstellar medium. We shall also be interested in late stages of evolution of stars in which they have properties especially interesting for the determination of galactic distances and we shall discuss the properties of some of the endpoints of stellar evolution.

Keywords

Neutron Star Massive Star White Dwarf Main Sequence Stellar Evolution 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1971

Authors and Affiliations

  • A. G. W. Cameron
    • 1
    • 2
  1. 1.Belfer Graduate School of ScienceYeshiva UniversityNew YorkUSA
  2. 2.Institute for Space Studies, Goddard Space Flight CenterNASANew YorkUSA

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