The β Pictoris system: Setting constraints on the planet and the disk structures at mid-IR wavelengths with NEAR

Open Access

Fig. 8

Images of the centro-symmetrical subtraction of the disk at 11.25 µm, obtained with VISIR in 2004 on VLT UT3 (top) and at 11.7 µm obtained in 2015 (bottom). In both images, the disk has rotated, respectively, 33° and 34° with respect to the north.

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