Fig. 13
Evolution in the HRD of all the models with initial stellar masses between 0.3 and 1.0 M⊙ for Yini = 0.248, 0.4, and 0.8 (top, middle, and bottom, respectively). For the very low-mass models, we stop the evolution if it exceeds 14 Gyr. At this age, the (0.3, 0.248) and (0.3; 0.4) models are still on the pre-main sequence, therefore they are not present in the HRD.
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