Redistribution of ices between grain populations in protostellar envelopes - Only the coldest grains get ices

Open Access

Fig. 2

Effects of n_H on the ice sublimation and re-freeze with Models Dens6, Dens7, Standard, Dens10, and Dens12 from top to bottom. Left: ice thickness (black lines) changes with T_d (red lines in the background). The thicker lines show larger grains. Right: n/n(H₂) for ice (solid lines) and gas-phase (dotted lines) species.

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