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Fig. 1

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Time evolution of CO depletion factor, fD, evaluated in astrochemical model Grid 1 (left column) and Grid 2 (right column) as a function of the environmental variables of: (a) top row: number density of H nuclei, nH; (b) second row: temperature, T; (c) third row: cosmic ray ionisation rate, ζ; (d) fourth row: visual extinction, Av. In each panel the three remaining variables are held fixed at their fiducial level (i.e. nH = 105 cm−3, T = 15 K, ζ = 10−17 s−1, An = 100 mag). Each time-evolving model is shown by a horizontal line with fD indicated by the colour scale.

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