Fig. 14

Theoretical evolution of lithium A(Li) (left panel) and the carbon isotopic ratio (right panel) as a function of effective temperature (from the main sequence up to the early-AGB) computed with thermohaline instability and rotation-induced mixing at solar metallicity for 4.0 M⊙ (VZAMS = 144 km s-1, solid black line), 2.7 M⊙ (VZAMS = 110 and 250 km s-1, blue and light blue dashed lines, respectively), and 2.5 M⊙ (VZAMS = 110 km s-1, red dashed line). The 4.0 M⊙ model following standard evolution theory is also indicated by dash-dotted line. Lithium detection and 12C/13C determination for cluster members are indicated by green symbols.
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