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Fig. 14

image

Left: mean deviation of disk masses (gas + dust) derived from 1100 μm continuum and molecular lines fluxes from the true disk mass extracted from the simulations. The gray bars indicate the full range of values for the different orientations. Right: mean deviation of stellar masses measured from molecular lines from the true stellar mass. The colors indicate the different simulations: 3D MHD simulations in blue, 3D MHD pseudo-disk simulation in red, and 2D semi-analytical model in green. The error bars indicate the standard error of the mean. The shaded region shows the area within a factor of 2.

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