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Fig. 1.

image

PMS evolution of standard non-accreting models with masses M = 0.7 and 0.8 M, and Z = 0.0001. Left panel: evolution in the HR diagram. We marked the position of the models at 1 Myr (filled triangles) and 10 Myr (filled squares). Right panel: evolution of the temperature at the base of the convective envelope as a function of age. The yellow shaded zone shows the Li-burning temperature range (TLi = 2.5−3.2 × 106 K, see text). We also marked the region where the deuterium burning supplies more than 50% of the total luminosity (thick magenta line).

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