Fig. 12
HR diagrams log g*–Teff (top) and L*∕L⊙ (bottom) and the positions of the individual components of HR 10. PARSEC V2.1s evolutionary tracks (red) and isochrones (green) are used. Isochrones correspond to 50, 100, 200, 400, 500, 530 (highlighted) and 600 Myr. Solid (dotted) blue lines in the lower panel are the evolutionary tracks with no rotation (rotation) for stars with 1.7 and 2.5 M⊙ from Ekström et al. (2012) (see Sect. 7.5). The two magenta triangles in the lower HR diagram show luminosities, described below in the main text.
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