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Fig. 4

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Distribution of zmax/Rin values relative to the mass accretion rate acc (in units of M yr-1), the power law p of the disk density change from Eq. (3), the temperature power law q from Eq. (2), and the inner disk radius Rin from Eq. (1). Results are shown for three types of objects, as indicated in the figure: Herbig Ae, T Tau, and brown dwarfs. The box-and-whisker plots at the far right show the range of results for each object: boxes show the median line and the first and third quartile, while the whiskers show the 10th and 90th percentile.

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