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Fig. 11

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Cumulative fraction of the total dust mass fd,tot that has encountered a location where the dust density ρd exceeds the Roche density ρR as a function of the time t after the start of the strong-clumping phase td,clump. Simulations of the streaming instability in isolation (blue lines) as well as of the scenarios SIwhileVSI (orange lines) and SlafterVSI (green lines) with an initial dust-to-gas surface density ratio of 2% and a Stokes number of 0.1 are depicted. The cumulative fractions (solid lines) increase close to linearly (dashed lines) with time, with the increase being strongest in the scenario SIwhileVSI and weakest if only the streaming instability is taken into account.

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