Abstract
Present knowledge on penetration and overshooting from stellar envelopes is reviewed and current assumptions are checked against laboratory experiments and numerical simulations. Emphasis is laid on quasi-adiabatic envelopes and, more precisely, on solar-type stars. Overshooting from the core is explicitly avoided.[/p]
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© 1990 Springer-Verlag
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Massager, J.M. (1990). Penetration and overshooting from a convection zone. In: Goupil, MJ., Zahn, JP. (eds) Rotation and Mixing in Stellar Interiors. Lecture Notes in Physics, vol 366. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53059-2_24
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DOI: https://doi.org/10.1007/3-540-53059-2_24
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