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On the Presence of Turbulent Diffusion in Stars and its Effect on Stellar Evolution

Published online by Cambridge University Press:  14 August 2015

E. Schatzman
E. Schatzman*
Affiliation:
Observatoire de Nice, B.P. 252 - Nice-Cedex 06007 - France

Extract

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The presence of a mild turbulence inside rotating stars has been considered by Howard et al (1967) and by Bretherton et al (1968) in connection with the problem of the solar flattening, raised by Dicke (1970). The possibility of using abundance determination to test the existence of that turbulence has been considered by Schatzman (1969).

Type
Session 6: Effect of Rotation and Magnetic Field in Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 281 - 283
Copyright
Copyright © Reidel 1981