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Fig. 13


Disk mass versus stellar mass in Taurus (Andrews & Williams 2005, open symbols) and in the CrA region (filled symbols). In both cases, inverted triangles mark upper limits. For objects with different disk models, we only display the mass derived from the best-fit model, although the differences in the masses between the models for each object are minimal thanks to the strong constraint provided by the PACS fluxes.

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