Fig. 6
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Distance–mass diagrams for single-embryo populations with varying parameterisations of Σactive. Top row shows results for temporally and spatially constant Σactive, while the bottom row shows results with the accretion velocity being a fraction of the local sound speed, fs × cs. Accretion layer thicknesses increase from left to right. Formation tracks are shown for 200 randomly selected simulations coloured by migration regime.
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