Thermohaline instability and rotation-induced mixing: I. Low- and intermediate-mass solar metallicity stars up to the end of the AGB

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作者
Charbonnel, C. [1 ,2 ]
Lagarde, N. [1 ]
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[1] Geneva Observatory, University of Geneva, Chemin des Maillettes 51, 1290 Versoix, Switzerland
[2] Laboratoire d'Astrophysique de Toulouse-Tarbes, CNRS UMR 5572, Université de Toulouse, 14 Av. E. Belin, 31400 Toulouse, France
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Stars:; abundances; -; evolution; Interiors; Rotation; sydrodynamics;
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