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Fig. 5

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Observed spectra of the species identified in the frequency coverage of the N2H+−N2D+ data (black histograms). The transitions are labelled in the top-left corner of each panel. The red histograms show the spectral fit performed with CLASS, which is a Gaussian fit for all transitions except for the ND3 and CN ones, for which we fit the hyperfine structure using the HFS routine. The vertical dotted line in each panel shows the source Vlsr = 5.65 km s−1, corresponding to the weighted average measured in the N2H+ and N2D+ lines.

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