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Evolution of a 30 M⊙ star with mass loss

Published online by Cambridge University Press:  14 August 2015

H. J. Falk  and
R. Mitalas
H. J. Falk
Affiliation:
University of Western Ontario
R. Mitalas
Affiliation:
University of Western Ontario

Abstract

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Evolutionary tracks for a 30 M⊙ star with mass loss rates (0.0, 1.0, 2.5, 5.0, 10.0)x10−7 M⊙/yr have been calculated. The effect of the different rates on the main sequence lifetime and on the effective temperature of the core He burning is discussed.

Type
Session 6: Evolution with Mass Loss: Single Stars
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 371 - 374
Copyright
Copyright © Reidel 1979 

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