Fig. D.2
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Distribution of dust temperature as a function of H2 column density for the sampled positions of California, Perseus, and the regions of Orion A for which no NH3-based gas temperature is available. The gray line represents the simple analytic fit to the equilibrium dust temperature described in the text. Dust temperature data are from Lada et al. (2017, California), Zari et al. (2016, Perseus), an Lombardi et. al. (2014, Orion A).
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