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Astrophysics and Space Science

, Volume 36, Issue 2, pp 439–450 | Cite as

Discussion of simple stability criteria for stars with central helium burning

  • M. Gabriel
  • S. Refsdal
  • H. Ritter
Article
  • 25 Downloads

Abstract

The validity of simple stability criteria for stars with central He-burning used in earlier papers is investigated. The determinant of secular stability for σ=0 is related to quantities defined as far as possible at the surface of the He-core and at the bottom of the envelope. This relation is used to discuss the validity of two intuitive criteria for secular stability.

Keywords

Burning Helium Early Paper Stability Criterion Helium Burning 
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 1975

Authors and Affiliations

  • M. Gabriel
    • 1
  • S. Refsdal
    • 2
  • H. Ritter
    • 2
  1. 1.Institut d'AstrophysiqueCointe-OugréeBelgique
  2. 2.Hamburger SternwarteHamburgBundesrepublik Deutschland

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