Fig. B.1
Stellar luminosity as function of time and stellar mass based on the stellar evolutionary model of Baraffe et al. (2003, 2015). The dots are data from the stellar evolution model, and the dashed line corresponds to the same luminosity. The black and red represent the stars above or below the hydrogen-burning limit. When the star is younger than
~ 10 Myr, 
, while 
when stars are older.
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