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Fig. 9

image

Evolution of the planet orbit (top panel) and the planet-vortex angular distance (bottom panel) in simulations of the inviscid disk model. Red line: MI1 case, green line MI2 case, and blue line MI3 case. The dashed area indicates the first U-turn of the planet in the MI1 case and in the MI2 case (respectively from left to right). The horizontal dashed line indicates the vortex orbital distance and the vertical line shows when the planet crosses the vortex orbit in the MI1 case.

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