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Fig. 2.
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TIMMI2 10.4 μm image (epoch 2006). The lower left circle shows the FWHM of a standard star measured before the object. The contours delineate [5, 35, 200, 560] × 1σ levels where the latter corresponds to half of the peak value. No Airy-rings are visible, although the source was classified as point-like.
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