Fig. 10.
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Histograms for properties of unbound starless (SL), prestellar (PRE), and all protostellar (PS PS-C) clumps. (a) Mean temperature. (b) Flux density. (c) Mean clump opacity spectral index (d) Mass, plotted on a logarithmic scale. (e) Mean clump column density. (f) Peak clump column density. The dotted line in (e) and (f) correspond to Av = 7.
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