Fig. 7
(From top to bottom) Evolution along the TP-AGB of the surface abundance of 3He, of N(Li), of the temperature at the base of convective envelope, of the helium-burning luminosity, and of the total stellar mass. The abscissa is the time since the first thermal pulse. Left and right respectively: 2.5 and 6 M⊙ at Z⊙ models computed with thermohaline and rotation-induced mixings.
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