Gas disk interactions, tides and relativistic effects in the rocky planet formation at the substellar mass limit

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Fig. 8

Medians of accumulated collisions of embryos (top panel) and of embryos that collided with the central object (bottom panel) of all IDA20 (red lines) and CN08 simulations (blue lines) before and after the dissipation of the gas-disk at 10 Myr (vertical line).

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