Fig. 4
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Same as Fig. 3, but for simulation Nbis5, in which an additional ice giant of Uranus mass was added in the simulation and the final resonance chain (2:1, 2:1, 4:3, 5:4) was obtained. This simulation is stable during the gas disc phase; however, it becomes unstable during the mock evaporation phase (see Sec. 2.4 for more details).
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