Fig. 7
Cumulative mass functions for the complexes, indicating the fractional mass above a chosen column density (or visual extinction, AV) threshold. The dotted red and dashed blue lines show the relation for Orion A (star-forming) and California (more quiescent) clouds, respectively, both of which have the total mass of about M = 105 M⊙ clouds (Kainulainen et al. 2009b).
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