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This article has an erratum: [https://doi.org/10.1051/0004-6361/201628623e]


Fig. A.1

image

Dust mass vs stellar mass for ρ Oph BDs (red) and TTS (blue). The top panel shows the results obtained by computing dust masses from Eq. (1) with T = 20 K for all objects. The mid panel when adopting the scaling law of T with L suggested by van der Plas et al. (2016). The bottom panel adopting the scaling law of Andrews et al. (2013), as in Sect. 4.1. The dashed green lines show the dust mass in a disk with 10%, 1%, 0.1% the stellar mass, computed assuming a gas-to-dust mass ratio of 100.

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