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Fig. 8


Distribution of counter-orbiting objects that can be produced by a parabolic, prograde, coplanar fly-by of a perturber with mass ratios of m = 0.1 (panel a), m = 1.0 (panel b), m = 20.0 (panel c), and pericentre that results in a mass-density drop at ≈30 au (black dots). The red circles show the solar system minor bodies from Table 6.

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