Fig. 16
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Growth tracks of an in situ forming planet at 5 AU. Shown are a 10 MMSN disk calculated with the model of San Sebastián et al. (2019) (blue), our model with fixed size (red, black), and the dynamic size calculation (magenta, green), in the nominal case and when only considering collisions once ϕ > 1. The solid lines are core masses and the dashed lines are the envelope masses.
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