Unknown
Publication Date:
2019-08-28
Description:
The hypotheses underlying theoretical studies of the evolution of massive model stars with and without mass loss are summarized. The evolutionary tracks followed by the models across theoretical Hertzsprung-Russell (HR) diagrams are compared with the observed distribution of B stars in an HR diagram. The pulsational properties of models of massive star are also described.
Keywords:
ASTROPHYSICS
Type:
B Stars With and Without Emission Lines, Parts 1 and 2; p 199-229
Format:
text
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