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Fig. 12


Synthetic images produced with GRaTeR for the extended-disc/embedded-planet case (nominal case, run G) assuming the central star is an A0V. We consider four different wavelengths: a) 0.5  μm (scattered light); b) 10  μm; c) 50  μm; and d) 300  μm. In each image, the flux has been normalized.

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