The homogeneous evolution of massive stars

Details The homogeneous evolution of massive stars The homogeneous evolution of massive stars

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...213..127b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 213, no. 1-2, April 1989, p. 127-132. Research supported by NSERC.

Astronomy and Astrophysics

Astrophysics

10

Stellar Composition, Stellar Evolution, Stellar Mass, Stellar Models, B Stars, O Stars, Stellar Interiors, Supermassive Stars, Wolf-Rayet Stars

Scientific paper

The homogeneous evolution of massive stars is investigated. A semi-analytic model, capable of describing the hydrogen burning phase of massive, chemically homogeneous stars, is developed. By comparing our model results with the detailed calculations of supermassive, Population III stars and fully mixed stars, it is found that the model provides a good description to the evolution of fully mixed stars. The model is applied to OBN blue stragglers.

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