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Fig. 1


Extended disc perturbed by an embedded planet. Azimuthally averaged radial distribution of the geometrical cross-section, as a function of particle sizes, for four different configurations: a) nominal (run G); b) Saturn-mass planet (μ = 2 × 10-4, run J); c) high optical depth (τ = 2 × 10-2, run I); d) low optical depth (τ = 5 × 10-5, run H).

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