Comparative study of evolutionary tracks of massive stars

Details Comparative study of evolutionary tracks of massive stars Comparative study of evolutionary tracks of massive stars

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...203...71d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 203, no. 1, Sept. 1988, p. 71-78.

Astronomy and Astrophysics

Astrophysics

17

Early Stars, Hertzsprung-Russell Diagram, Stellar Evolution, Stellar Models, Interstellar Extinction, Stellar Color, Stellar Magnitude, Stellar Mass, Stellar Temperature

Scientific paper

The effects of mass loss, convection, and opacity on the structure of stars are analyzed, and an overview of various evolutionary computations is given. The different constraints are analyzed and the underlying physics are outlined. The differences in predicted effective temperature and luminosity for various masses, compositions, and the spread in location in the H-R diagram are given for the initial main sequence and at the end of core hydrogen burning. They are also given for the 'red points' where the evolutionary tracks change their rightward motion into a leftward one.

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