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Fig. 4

image

Flux contributions in the optical and the IR for Mon-660 at i = 77°. The modeled CoRoT and 4.5 μm fluxes coming from the star are represented as filled squares and filled circles, respectively. The 4.5 μm fluxes coming from the wall and the disk are plotted with solid triangles and asterisks, respectively. The light asterisks represent the total modeled flux.

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