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Fig. 13

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Sulphur-bearing species column densities as a time function (gas phase) for the hot core Model 5 with a star mass of 10 M, fr = 0.85, and 0.1 S sulphur abundance. The points indicate the observational results of SO, SO2, CS, OCS, H2CS, and H2S. In this case,  S+ freezes out to form OCS (50%) and H2S (50%) on the mantles at the end of Phase I.

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