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Instabilities in Highly Evolved Stellar Models

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Abstract

The structure of heavy stars at highly evolved stages of evolution is considered. It was found that radiation relativistic effects on the electrons and pair creation induce a dynamical instability in stars heavier than about 30 Mo. The evolution of a 30 Mo oxygen star is described in some detail up to the point where it becomes dynamically unstable.


Publication:

The Astrophysical Journal

Pub Date:
June 1967
DOI:

10.1086/149204

Bibcode:
1967ApJ...148..803R