Fig. 8
Left panel: ten systems after 3 Myr of evoluton in the protoplanetary disc (runf5). Right panel: same systems, after 100 Myr of evolution(runf5-C). Only one remained stable, here shown as the light-green system, while the other systems all underwent a post-gas instability. These latter systems contain fewer but more massive planets and are less strongly size-sorted with orbital distance.
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