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Fig. 5


Simulated ZIMPOL images of the different mass and orbit radius cases studied. Upper to bottom rows correspond to a 3   Myr disc model with a planet of masses Mp =  [1,9,15]    MJup, respectively. Left to right columns show the different planet orbit cases, Rp =  [20,40,60]    AU, respectively. The white dot indicates the position of the planet in each image and the black contour lines correspond to the intensity ring detected by ALMA at 850   μm.

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