Fig. 4
Left panel: time evolution of the radial profiles of the eccentricity (solid lines) and inclination (dashed lines) for 100 km-sized planetesimals. Right panel: time evolution of the relative velocity between planetesimals with 100 km radius. In brackets we show the total mass of the planet at the given times. The black curve corresponds to the time (and mass) at which the planet reaches the cross-over mass.
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