Numerical simulations of Neptune's migration yield empirical expressions for eccentricity thresholds and capture efficiencies into exterior mean motion resonances, depending on migration rate, distance, and resonance order.
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Numerical estimation of the capture ability of Neptunian mean motion resonances
Numerical simulations of Neptune's migration yield empirical expressions for eccentricity thresholds and capture efficiencies into exterior mean motion resonances, depending on migration rate, distance, and resonance order.