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Fig. 9


Growth tracks of pebble accreting and migrating protosatellites in the circum-jovian CPD assuming 0 = 10−6 M yr−1, r0 = 10 RJup, and pebbles with a constant Stokes number St = 5 × 10−3. Here, clearly, protosatellites cannot grow to masses comparable to that of the Galilean moons (marked as yellow dots) before reaching the inner edge of the disk.

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