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Convection and the Relevant Problems of Stellar Structure, Evolution and Oscillations

Published online by Cambridge University Press:  26 May 2016

D. R. Xiong  and
L. Deng
D. R. Xiong
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, P.R. China
L. Deng
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, P.R. China

Abstract

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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 

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