Fig. 8

The M−L relationship during the evolutionary phase at constant mass for the cold-nominal population, analogous to Fig. 2. In the top left panel at 20 Myr, the gray lines and shaded regions indicate the observed luminosities and derived masses for 51 Eri b and β Pic b. In the panel at 50 Myr, the gray solid and black dashed lines show the M−L relation of Burrows et al. (1997) and Marley et al. (2007), respectively.
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