Fig. 9
Mixing length parameter along stellar evolutionary tracks with solar metallicity against the normalized age for the masses from 0.7 to 1.5 M⊙ (indicated). The tracks are derived from the functional fits f(Teff,log g) of αMLT-calibrations with sbot and Δs (top and bottom panel, respectively) and all tracks end on the RGB when log g = 1.
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