Fig. 3
Cumulative distribution plots for Perseus disk masses calculated from ALMA flux densities and Orion disk masses from Tobin et al. (2020), both calculated with the same opacity assumptions of κ1.3 mm = 0.9 cm2 g−1. The Perseussample consist of 77 sources (38 Class 0 and 39 Class I), the Orion sample consist of 415 sources (133 Class 0 and 282). Medians are indicated in the labels.
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