Complex organic molecules in low-mass protostars on Solar System scales - II. Nitrogen-bearing species

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Fig. C.7

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Same as Fig. C.1 but for NH₂CHO and a high temperature for the model. This graph is presented to demonstrate that it is not possible to derive an upper limit for theexcitation temperature of this molecule because the model used in this plot is very similar to the model in Fig. C.6.

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