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Fig. 2

image

Grey filled histograms show spectra converted to brightness temperature (Tb) scale: spectrum extracted towards the central position, the B-shock position, and an average within a radius of 0.′′ 5 around the peak of the dust continuum emission, which is multiplied by a factor of 4 for a better visibility. The blue labels show the species listed in Table 1, pink labels show transitions of CH3OH (and its isotopologue) discussed in Paper I. The spectra have been shifted along the y-axis for a better visibility.

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