Fig. F.2.
Top panel: variation with age in the fractional mass of the convective core, in 2.5 M⊙ solar-calibrated models. Bottom panel: resulting profiles of the hydrogen-abundance X in the 10 R⊙ red-giant model. The solid and dot-dashed lines show the original and revised LPCODE models, and the dashed lines show the corresponding ASTEC model.
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