Planetesimal fragmentation and giant planet formation - II. Dependencies with planetesimal relative velocities and compositions

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Fig. 3

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Core masses (solid lines) and envelope masses (dashed lines) as function of time. Here, as in Figs. 5, 8, 9, 12, and 13, the red thick lines correspond to the baseline model, while the gray thin lines correspond to the formation of the planet without planetesimal fragmentation.

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