Fig. 10
The M–L relationship during the evolutionary phase at constant mass for the cold-classical (low core mass) population, analogous to Fig. 8. In the panel at 20 and 50 Myr, the gray solid and black dashed lines show the M−L relation of classical hot start (Burrows et al. 1997) and cold start (Marley et al. 2007) models, respectively.
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