Fig. A.1
Top panel: continuum-subtracted, spatially-integrated emission from the NJ, 88−77 line of SO (344.311 GHz). Bottom panel: continuum-subtracted, spatially-integrated emission from NS (345.823 GHz). The emission from NS partially overlaps with that from 12CO J = 3−2 (in Fig. 1, the emission around VLSR = −62 km s-1 corresponds to NS).
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