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Fig. A.1

image

From left to right: spectra of H2CO 30,3−20,2, HCO 31,3−21,2, HDCO 32,1−22,0, 32,2−22,1, 31,3−21,2, 30,3−20,2 and D2CO 30,3−20,2 observed toward AFGL5142, IRAS 05358+3543, and G5.89-0.39 using the IRAM 30 m telescope (Fontani et al. 2011, 2015) and the APEX SEPIA Band 5 receiver (this work). Red and blue lines indicate the fitted different velocity components for AFGL5142 and G5.89-0.39 with fixed velocity and width. The C13CS N = 15−14 and J = 15−14 transition is shown in the fourth panels from the top.

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