Fig. 8
H abundance (upper panel), and the logarithm of the squared Brunt-Väisälä and Lamb frequencies (lower panels) corresponding to the stellar models with M⋆ = 1.7 M⊙, Z = 0.015, 
(central abundance) and different assumptions for the value of f of the convective overshooting. The location of these models in the HR diagram is marked in Fig. 3 with black dots.
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