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Fig. 5

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Gas surface density after 100 000 binary orbits in each setup. Distance is in binary separations and the color scale is normalized to the maximum of each image. Panels on the left and right show the setups with h/r = 0.03 and h/r = 0.05 respectively. In each panel, the columns show the setups with the same binary eccentricity, being 0.15, 0.25, and 0.35 from left to right. The upper row of each panel contains the setups with no planet, and the lower row the setups with planet. A white dashed line shows the best cavity fit, while the black dashed line shows the best peak ring fit. A white triangle is used to show the position of the planet.

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