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Fig. B.3

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OH 119 µm P-Cygni profile toward the hot core (FIR continuum peak), compared to other line profiles. The OH 119 µm absorption dip agrees with [O I] 63 µm absorption at +6 km s−1 (hot core velocities). The [C II] 158 µm emission and [O I] 63 µm absorption at +2 km s−1 corresponds to a gas structure in the foreground.
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