Fig. 8

X-ray irradiated cloud with density n = 105.5 cm-3 and radiation field FX = 160 erg cm-2 s-1. (left) The abundances are shown for H, H2, OH, and H2O in three different cases: formation of OH and H2O (i) in gas phase only (ii) in gas phase and on dust with an MRN size distribution, and (iii) in gas phase and on dust with a Weingartner & Draine size distribution. (right) Gas and dust temperatures for the same models. The temperature profiles for the gas only models and those where OH and H2O formation on dust with an MRN distribution are included are the same.
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