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Numerical simulations of radiative zones and possible effects on evolutionarymodels
Published online by Cambridge University Press: 13 January 2006
Abstract
This paper discusses numerical simulations performed in order to better understand the dynamics of various physical processes present in the radiative regions of stars. Those processes include semi-convection, Eddington-Sweet meridional circulation and anisotropic turbulence. The impact of some of those results on evolutionary models is also discussed.
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- Research Article
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- © EAS, EDP Sciences, 2005
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