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Fig. 6

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Comparison of several physical parameters as a function of mass for ASAS-04 with several sets of isochrones. The left column is for the age of 1 Gyr and solar metallicity, the middle column is for 6 Gyr and metallicity below solar (0.01 for PADOVA and Y2, 0.008 for GENEVA and 0.006 for BCAH98), the right column is for solar composition and t = 12 Gyr, except BCAH98 (8 Gyr). From the highest to the lowest, the rows show mass vs. MbolR, log (Tphot), MV and (V − I) colour. The measurements and their uncertainties are taken from Table 3.

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