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Fig. 11

image

Efficiency of accreted (red line) and survived particles (green line) as a function of Stokes number for different planetary masses. The laminar disc run is represented with solid lines, while the VSI run with dashed lines. The fit from Lambrechts & Johansen (2014) is overplotted for intermediate τs values with a dashed grey line (see Eq. (40)).

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