Fig. 13
Formation scenario of a planetary system. Top: schematic picture of the protoplanetary disk. The brown and white filled circles denote the planets and drifting pebbles. Bottom: assumed Stokes numbers, the origins of the turbulence (ZVI, COV, and VSI), and the resulting accretion probability in the Stokes (solid line) and in the Epstein (dashed line) regimes.
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