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Fig. 13


Top row: eccentricity vs. semi-major axis for the planets formed in 3D-POP (left) and 2D-POP (right). Bottom row: inclination vs. semi-major axis for 3D-POP (left) and 2D-POP (right). Vertical axes are on logarithmic scale. The size of each circle is proportional to the cubic root of the planetary mass.

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