Disk masses as function of ﹩M_{*}﹩ (top panel) and of ﹩\dot{M}_{\mathrm{acc}\,}﹩ (bottom panel) for the Taurus sample; binaries unresolved in the millimeter observations have not been included. Only a few of the Taurus BDs shown in the top panel have measured ﹩\dot{M}_{\mathrm{acc}\,}﹩ and appear in Fig. 1 and in the bottom panel. Lines are the same as in Fig. 1. Note that all models practically overlap in the bottom panel.