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Evolution of a 30 M⊙ star with mass loss
Published online by Cambridge University Press: 14 August 2015
Abstract
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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