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. Author manuscript; available in PMC: 2020 Oct 14.
Published in final edited form as: Astrophys J. 2019 Oct 14;884(1):10.3847/1538-4357/ab418e. doi: 10.3847/1538-4357/ab418e

Fig. 17.—

Fig. 17.—

60 K models at time t = 106 yr. Abundances of the initial ice components are shown in the left panels, with dust shown as a dotted line. Results for two model setups are shown: low UV (upper panels) and high UV (lower panels).