Fig. C.1
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Surface density and streamlines for a migrating super-Earth- sized planet with q = 1.5 × 10−5 at tmig = 300Porb after the planet was released. The corresponding migration track is shown in bottom panel of Fig. 4 (αDZ = 10−3 and αMRI = 2.5 × 10−2). There is an excess mass in the rear horseshoe region and the planet thus migrates in the runaway Type III regime.
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