Fig. 15

Mass accretion rate from 10%WHα (left panel) and EWHα (right panel) versus stellar mass. Diamonds and triangles represent Cha I and γ Vel stars, where filled and empty symbols refer to UVES and GIRAFFE data, respectively. Squares mark the position of the possible accretors. Big red diamonds represent the median values of Ṁacc for stellar masses of Cha I members binned at 0.2 M⊙, where both confirmed and possible accretors were considered. The dashed line represents the relation, while the “noise boundaries” at 3 Myr and 10 Myr due to chromospheric activity are overplotted by dash-dotted lines (Manara et al. 2013). Mean error bars are overplotted in the right corners of both panels.
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