Discussion of Simple Stability Criteria for Stars with Central Helium Burning

Details Discussion of Simple Stability Criteria for Stars with Central Helium Burning Discussion of Simple Stability Criteria for Stars with Central Helium Burning

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..36..439g&link_type=abstract

Astrophysics and Space Science, Volume 36, Issue 2, pp.439-450

Astronomy and Astrophysics

Astrophysics

Scientific paper

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.

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