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- W1663098762 abstract "Our understanding of transport processes in stars is still in its infancy. First consider overshooting. There is now ample evidence from, e.g., the best-observed binary stars and fits of models to observed colour-magnitude (C-M) diagrams that some amount of mixing must occur beyond the classical boundary of the convective core set by the Schwarzschild criterion. Such mixing can be achieved by convective penetration; however, despite impressive progress on the theoretical front, a rigorous prediction of the extent of overshooting has not yet been achieved. As a result, most stellar evolutionary calculations have simply opted to extend convective core sizes by an amount (usually measured as a fraction of a pressure scale height) that produces reasonable consistency with observations. But how realistic are such models? To what extent does the overshooting depend on mass and/or evolutionary state? What is the role of rotation in determining the size of convective cores? How much does rotation-induced meridional circulation contribute to such mixing?" @default.
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- W1663098762 date "2002-01-01" @default.
- W1663098762 modified "2023-09-26" @default.
- W1663098762 title "Joint Discussion 5 - Mixing and Diffusion in Stars: Introduction and Brief Overview" @default.
- W1663098762 doi "https://doi.org/10.1017/s1539299600013460" @default.
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