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Fig. 8

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Contour plots showing time-averaged and azimuthally-integrated radial mass flux distributions in the various layered disc models with embedded planets. The cyan dotted line indicates the location where the column density measured from the disc surface corresponds to ΣA. The vertical white dotted line denotes the location of the 2:1 outer Lindblad resonance. Note that only the upper hemisphere of the disc is simulated.

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