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Fig. 3
Continuum-subtracted HIFI spectra of the C18O 9–8 and CS 11–10 lines (in black). The model fits are shown as red lines over the spectra. Vertical dotted lines indicate the VLSR at 99.4 km s-1. The spectra have been smoothed to 0.2 km s-1. The unidentified line in absorption seen at 88.6 km s-1 is indicated.
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