Fig. 5
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Surface density profile evolution for Γ0 (top-left), Γ2 (top-right), Γ4 (bottom-left), and Γ8 (bottom-right). The planet’s position at 10 au is marked by a dashed red line. The planet opens a primary gap and excites three overdensities (D1, D2, D3). Surface density profiles are obtained by integrating the volumetric density over the polar angle (θ) and then averaging over the azimuthal angle (ϕ) for each orbit.
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