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Fig. 4

image

Chemical model abundances of CH3CN (black) and CH3NC (green) for the warm-up stage of a hot core type model where the main destruction pathway for CH3 NC (H+CH3NC) has been disabled. Solid lines denote gas-phase abundances, while dashed lines indicate grain-surface abundances. The top panel shows the model with a final collapse density of nH = 1.6 × 107 cm−3 and the bottom panel shows the model with a final collapse density of nH = 6 × 1010 cm−3.

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