Fig. 15
Left: abundance profile of water with respect to H2 for IRAS4A for varying the interstellar radiation field (Gisrf) between 1 (red), 10 (blue) and 100 (cyan). Middle: as for the left plot, but for cosmic-ray UV rates (Gcr) of 3 × 10-5 (blue), 10-4 (red) and 3 × 10-4 (cyan). Right: the abundance profile of water for IRAS 15398 with Girsf = 0 (red) and Girsf = 1 (blue).
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