Fig. 6
Resonance capture of a Jupiter-mass planet evolving assuming type II migration. Starting at n1/n2 > 2, the planet is ultimately trapped in the 2/1 MMR (top panel). Starting at 1.67 < n1/n2 < 2, the planet is trapped in the 5/3 MMR (middle panel), and starting at n1/n2 < 1.67, in the 3/2 MMR (bottom panel).
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