Fig. 7
Left and center panels: observed and modeled VLT-VISIR 18.7 μm images. Contour lines show 10,20,...% of the peak emission. Right panel: cut through the observed and modeled images (Δδ = 0). Red line: observed intensity. Black, green, and blue lines: modeled intensities for different outer radii of the warm dust inner disk (Rinner,dust = 1,3, or 10 AU).
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