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Fig. 3

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Smoothed C17O(2−1), H13CO+(4−3), DCO+(4−3), N2H+(3−2), and N2D+(3−2) spectra. Overlaid on the C17O, DCO+, N2H+, and N2D+ spectra are the hf-structure fits. The relative velocities of individual hf components in these transitions are labelled with a short bar on the spectra towards IRAS 05399. The H13CO+ spectra are overlaid with a single Gaussian fit. The fits to the lines at the systemic velocity  ~9 km s-1 are shown as green lines, whereas the red lines show fits to the lines at lower velocities. Note that H13CO+(4 − 3) observations were carried out only towards three sources and the line is detected only towards IRAS 05399 and SMM 4 (at  ~1.5 km s-1).

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