Fig. 13
IRDIS J-band r2-scaled Qφ image convolved with an elliptical Gaussian kernel (132 × 94 mas) to match the angular resolution of the ALMA Band 9 observation from Pérez et al. (2014). The superimposed contours show the ALMA Band 9 (0.45 mm) dust continuum with the beam size in the bottom left. We assumed that the star is located in the cavity center of the ALMA image.
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