Fig. B.2
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Millimeter flux in binary systems located in Orion, Lupus, and Taurus as a function of their projected separation. The flux of each system is rescaled at 140 pc, i.e., the average distance of Taurus. The Class II sources are Orion A (this work), Lupus (Zurlo et al. 2021; Ansdell et al. 2018), and Taurus (Akeson et al. 2020; Manara et al. 2019; Akeson & Jensen 2014; Harris et al. 2012). The Class 0, I, and FT sources are Orion (Tobin et al. 2022). We only considered systems detected by ALMA (0.87 mm).
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