Fig. 7
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Snapshots of the final semi-major axis and eccentricity distribution of embryos and planetesimals for the simulation sets 232, 233 and 234, showing the decreasing efficiency of embryo formation. Apart from the top panel, the planetesimal population closer than 2.5 au is completely mixed (black for terrestrial group material, red for Jovian group material). Almost no planetesimals reside on orbits with a > 2.5 au. The colour bar shows the fraction of Jovian group material incorporated in the embryos.
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