Fig. D.3

Abundances vs. H2 for CH3OH, C2 H5OH, CH3 CHO, CH3 OCHO, HC3 N, CH3 CN, CH2 CHCN, and C2H5CN using IC 5 with a density of 109 cm−3 and a fast warm-up time of 50 kyr are shown for G35.20 A (left), B1/B2 (middle), and B3 (right). The time period shown is only a part of the modeled time, from 18 000 to 35 000 yr. The time range in which all abundancescan be reproduced with an error of 1 order of magnitude are shaded in gray. The abundance of C2 H5CN in A and B3 is not reproduced so a small black ellipse shows the gap between the lower abundance limit and the modeled abundance.
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