Fig. 10

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Initial semimajor axes and eccentricities of objects captured by leading (red) and trailing (blue) islands in the exponential migration model. The timescales of migration τ are marked in each panel. The vertical dashed lines are the inner and outer edge of the belt of test particles, and the numbers near them are the instant migration rates of Neptune when the nominal resonance arrives at both edges of the planetesimals’ belt.
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