Fig. 1
Density (upper panel) and temperature (lower panel) profiles of primordial atmospheres as a function of altitude, for core masses of 0.1 M⊕ (black), 1 M⊕ (green), and 3 M⊕ (red). The dashed lines represent the individual Hill radii of the cores. These data represent a snapshot at 1 Myr from the time-dependent atmospheric evolution simulations and a star with 1 M⊙ (see Stökl et al. 2016).
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