Fig. 3

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emin and Pres for different MMRs under various ȧN values. The horizontal axis represents the final location of each MMR, the vertical axis shows the minimum initial eccentricity, emin, for each MMR, the color of the points indicates Neptune’s migration rate ȧN in the simulation, and the size of the points represents the number of captured small bodies, Pres. Some of the major MMRs are marked with dashed black lines, with their corresponding p and q values indicated above the lines, while other MMRs are shown with gray dashed lines.
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