N-bearing complex organics toward high-mass protostars - Constant ratios pointing to formation in similar pre-stellar conditions across a large mass range

Open Access

Fig. D.5

Showing that excitation temperature of 150 K does not match the observations for CH₃NH₂ in source 767784. The various symbols are the same as Fig. 2. Again here some lines are overestimated and if the column density is decreased the lines that are perfect fits now will be underestimated.

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