Fig. 5

Same as Fig. 4, but assuming now that ten planetary embryos are growing and migrating in every protoplanetary disc. The number of points is 5010. Planets on the vertical line at 1000 AU are planets ejected from the system. Their mass represents their mass at the time of ejection. Planets on the vertical line at 0.005 AU are planets that have collided with the central star. We do not include in our models planet-star interactions that could modify the orbital evolution of planets in the innermost parts of the disc.
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