Free Access

Fig. 6


Disk mass, derived from (sub)-mm fluxes, in units of solar masses (top panel) and stellar mass (bottom panel) as a function of the mass of the parent body for all targets in this paper. Binaries are highlighted with diamonds. A conservative estimate of disk mass uncertainty arising from unknown individual distances is shown in the bottom left of the top panel, assuming a conservative Δdist = ±10% (cf. Torres et al. 2007, who estimate a “depth” of Taurus of 20 pc). Dotted lines show the typical sensitivity limits derived from Eq. (3) for targets in Taurus (F1300,lim ≈ 1 mJy, dist = 140 pc) and TW Hya (F1300,lim ≈ 0.05 mJy, dist = 50 pc), using BCAH98 isochrones to convert mass to luminosity.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.