Fig. 1
RZ Psc (filled square) on the HR diagram. The errors indicate the precision of the determination of the Teff and lgg. The light gray solid line is the ZAMS. Thin solid lines are the evolutionary tracks from Siess et al. (2000) models, these tracks are labeled with the corresponding values of the stellar masses. The dashed lines are the isochrones for the ages 1, 10, and 30 Myr.
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