Fig. 11
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Percentage of P3 and 259P clones that remain in main-belt-like orbits (2.064 < a < 3.277 AU and q > 1.65 AU and Q < 4.50 AU) in the backward dynamical evolution. P3 survivors decrease exponentially on an e-folding time ~12 Myr. During the whole computed period of 100 Myr, 98% of the P3 clones left the main belt, while all 259P clones remained in the main belt.
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