Fig. 16
Line cooling in the 795–903 GHz range in two sources in Orion. The symbols mark the percentage of line emission in each dominant cooling species in OMC-2 FIR 4 (crosses, this work) and in Orion KL (circles, Comito et al. 2005). The upper limits are 5σ. Note that the units are in percent of all line flux within the 795 to 903 GHz range, excluding continuum emission.
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