Fig. 6

Planet migration tracks for different model parameter. Starting from the standard model (in red) with (α,ṁ,q) = (0.003,10-7,0.001), individual parameters have been varied while keeping two others fixed. We varied α (left panel), ṁ (middle panel), and q (right panel). The full and dotted lines correspond to non-accreting and accreting planets, respectively.
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