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Fig. 5

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Mid-IR images of disks heated by a T Tauri star at distance of 50 pc and viewed at 30°. The image of a pure disk (top) and a disk plus halo is shown (middle). Color bars are in log (Jy/arcsec2). Bottom: corresponding surface brightness distribution measured as cut along δ through origin of the image. Gaps between emission rings are indicated.

This figure is made of several images, please see below:

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