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Fig. C.1

image

CH3NH2 transitions detected towards NGC 6334I in the range 890.2 to 891.7 GHz (ALMA Band 10). The red line represents the synthetic spectrum of CH3NH2 assuming a column density of 2 × 1017 cm−2, an excitation temperature of 100 K and a FWHM line width of 3.2 km s−1, in a 00.′′26 × 0.′′26 beam (equivalent to the angular resolution of the data). The abscissa is the rest frequency with respect to the radial velocity towards the region (−7 km s−1). The data are shown in black.

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