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Fig. 8
Real part of the visibilities at λ = [0.87,1.0,3.0,7.0] mm at different times of dust evolution when a 20 MJup planet is embedded in the inner disk (10−15 AU) from early stages, and a second planet (15 MJup) is injected after 3 Myr of dust evolution. ALMA Cycle 0 and ATCA data are over-plotted for comparison.
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