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Fig. 12


Best-fit Teff and log g for Star 1 (α Tau) converted to luminosity, using three different mass values (triangles up – 0.6 M, squares – 1.1 M, triangles down – 1.6 M), and direct Teff and log g values from Table 1 (black cross with error bars). Solid lines are evolutionary tracks for Z = 0.008 and Y = 0.26 by the Padova group (Bertelli et al. 2008, 2009), labelled to the left with mass in solar masses.

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