Fig. 2
Time evolution of the envelope after core accretion is halted in the case of Mcore = 5 M⊕. The upper panel (a) shows the envelope mass Menv (solid line) and the core mass Mcore (dashed line) and the lower panel (b) presents the luminosity L. This is in good agreement with Ikoma et al. (2000), Fig. 2, even though the used opacities from Ferguson et al. (2005) (g98.7.02.tron) are not exactly equivalent.
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