Fig. B.1
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Normalized torques as a function of planetary mass and semi-major axis, assuming circular and coplanar orbits. The different migration regimes are indicated, separating inward from outward migration. The mass required to open a gap in the disk (dashed white line), the planet-to-star mass ratio (q) of 0.002, and the gas depth criterion K=104 are over-plotted (dashed black lines).
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