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Fig. 2


Upper panel: time evolution of Γ(M,EOS) for some stellar models evolving from the PMS to the WD stage. The mass range is 0.1–1.7 M (see symbols in the left upper corner). The adopted initial chemical composition is X = 0.73, Z = 0.01 and the mixing-length parameter αMLT = 1.5. Lower panel: specific nuclear power for the same models.

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