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Fig. 9


Comparison between simulation results and the simple estimates derived in Sect. 5.2 after 3 Myr of dust evolution. The upper panel is for a turbulence value of αt = 10-3, the lower panel for αt = 10-2. The estimates have been calculated using the dust accretion rate of the simulations at 50 AU which are 1.6 × 10-6 and /yr, respectively. The division between the different fit formulas is described in Sect. 5.2.

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