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Fig. 8

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Architecture of our simulated planetary systems around a 0.6 M and a 0.8 M K-dwarf star, for two or four different gas surface density values and different initial disk masses (IDM) after 20 Myr of N-body integration using GENGA. Outcomes for the initial disk mass 5 M are not displayed. The point size indicates the masses in M of the formed planets. The gray zone is the region inside the inner truncation radius, and the dashed gray line shows the inner edge of the gas disk.

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