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Fig. 17


Comparison between the eccentricities distribution for the evolution of the 7 original particles in the 1:3 MMR region (dotted histogram) and the averaged eccentricities for the test particles that released the resonance while Neptune migrates, becoming fossilized (continuous black histogram). The peak at e ~ 0.21 suggests that 2004XR190-like orbits might be formed close to 1:3 MMR with Neptune.

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