Local mixing length theory with compositional effects: First application to asymptotic giant branch evolution

Open Access

Fig. 1.

Chemical abundances of He (dotted lines), C (continuous lines) and O (dashed lines) of stellar models of initial mass M_in = 1 M_⊙ (left panel), 1.5 M_⊙ (middle), and 3 M_⊙ (right) at the end of the AGB phase. The blue lines correspond to the case where MLT was used, the orange ones are for MLT♯, and the black ones are for GNA.

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