Fig. 10
Disk dust masses vs. central object mass for the BD (red) and stellar (blue) populations in Lupus. Detected sources from ALMA observations are represented as circles; upper limits of nondetections are shown as triangles. Dust mass uncertainties and upper limits as described in Sect. 4.5. Uncertainties of M⋆ are 1σ. Linear regression shown for the entire disk population (stars and BDs).
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