Fig. 5
Cumulative distribution function of dust masses for Class 0 and Class I disks in Perseus and Orion and Class II disks in Lupus measured with ALMA Top: Perseus disk masses calculated with κ1.3 mm = 2.3 cm2 g−1 from the ALMA fluxes. Bottom: Orion disk masses calculated with the κ0.89 mm = 1.3 cm2 g−1 (Tobin et al. 2020). Medians are indicated in the labels.
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