Fig. B.1
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Similar to Figure 5, but for the disk parameters of αt = 10−2, ξp/g = 2%. After stochastic collisions between protoplanets in this high-turbulent disk, the protoplanet represented by the orange solid line undergo rapid growth and trigger gas accretion at approximately 1.3 Myr. It subsequently evolves into a gas giant with an orbital period of 100 days.
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