Fig. 3
Dynamical evolution of the planets in stage II of evolution. The mass increase of the planets is shown the top-right panel. The orbital decay of the semimajor axes and the mean-motion ratio on the top-left panel. The bottom-left panel shows the eccentricity as a function of time, while the evolution of the resonant angle σ1 and the secular angle Δϖ is shown on the bottom-right panel.
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