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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
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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).
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- Session 6: Effect of Rotation and Magnetic Field in Stellar Evolution
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- Copyright © Reidel 1981
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