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Convection and the Relevant Problems of Stellar Structure, Evolution and Oscillations
Published online by Cambridge University Press: 26 May 2016
Abstract
The main results of stellar structure, evolution and oscillations given by our non-local statistical theory of convection are summarized in this paper. A main difficulty of convection theories, i.e. supersonic convection, is also discussed.
- Type
- Session C. Convection
- Information
- Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 181 - 192
- Copyright
- Copyright © Astronomical Society of the Pacific 2003