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Effects of envelope overshoot on intermediate mass stars
Published online by Cambridge University Press: 19 July 2016
Abstract
We find that a certain amount of non-local overshoot at the base of the outer convective envelope affects the evolution of intermediate mass stars in the H-R diagram, producing extended loops even for models computed with significant overshoot from the central convective core, improving in this way upon a weak point of models with core overshoot.
- Type
- Stellar Evolution
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 327 - 328
- Copyright
- Copyright © Kluwer 1991