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Fig. 4

image

Top left: best-fit H-band V2 from the radiative transfer (red diamonds) and PIONIER V2. Top right: same for the PIONIER closure phases that were only used to check for consistency (Bmax is the longest baseline of the triplet). Bottom left: best-fit K-band V2 from the radiative transfer (red line) and AMBER V2 (black). Bottom right: same for the modeled N-band visibilities and the MIDI data (detailed in Matter et al. 2014).

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