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Thermohaline mixing and fossil magnetic fields in red giant stars
Published online by Cambridge University Press: 01 April 2008
Abstract
We discuss the occurence and consequences of thermohaline mixing in RGB stars, as well as the possible inhibition of this process by a fossil magnetic field in Ap star descendants.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S252: The Art of Modeling Stars in the 21st Century , April 2008 , pp. 245 - 246
- Copyright
- Copyright © International Astronomical Union 2008
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