Fig. 3
Azimuthally averaged vortensity ⟨ η2D ⟩ φ (blue lines) and disk eccentricity (red lines) versus the disk radial extension for the hydrodynamical simulations of Fig. 2 after 1000 (dotted lines) and 2000 (solid lines) orbits. The vertical lines correspond to the positions of the two planets.
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