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Fig. 7

image

Comparison of the semi-major axis evolution (solid black) in the FARGO simulations vs. the azimuthally averaged surface density at the 2:1 (solid blue) and 3:2 (solid orange) mean motion resonance location in the corresponding disc. Only the runs in which the planet was parked due to planet-disc interactions are shown. The horizontal dotted lines are drawn at Σ2:1 = 10−1 g cm‒2 and Σ3:2 = 10−2 g cm‒2 and cross the corresponding vertical line where the planet is considered to be parked fully.

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