Fig. B.1
Post-formation entropy as function of total mass. The dark (light) blue lines are for cold accretion and a core mass of 32 (49) M⊕. The red curves are for hot accretion. The solid lines are the nominal model and identical to Fig. 2. The dotted curves are simulations without the photospheric pressure. The dashed lines are for a full ISM grain opacity.
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