Fig. 8
Comparison of the absorption features seen in the 13CO (3−2) and HCO+ (1−0) lines toward the peak of the 890 μm continuum emission. For the sake of comparison, the interferometric 13CO (3−2) spectrum has been obtained after reconstructing the data with a synthesized beam equal to the single-dish beam of the HCO+ line observations with IRAM 30-m telescope (see Sect. 3.3.3).
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