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Fig. 5


Scattered light predictions at 1.2 μm of the hydrodynamic model (bottom middle and bottom right panels) with a misalignment angle between the inner and outer disk of ~30°, compared to the observations (bottom left panel). The locations of the two stars are indicated with white circles. All images are scaled by r2. The upperpanels show a schematic of the 3D structure, with a color coding (green, purple) that indicates the regions of the disk above and below the plane perpendicular to the line of sight. Model A corresponds to the blue solution of Fig. 4, model B to the red.

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