Fig. 6
The SED of the excess emission close to the star. Black dots are ESO photometry, blue dots AKARI photometry. The red dot refers to the near-IR interferometric measurement (Absil et al. 2009), the green dot to the unresolved excess emission at the location of the star in the Herschel PACS 70 μm image. The dashed line represents Fν ∝ ν0.8.
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