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Fig. 5

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Herschel PACS 160 μm image of HIP 92043 as observed (left) and residual image (right) after subtraction of a point source scaled to the predicted source flux from the stellar optical position. Contours in both images are in 1-σ increments of sky noise from –2 to +4-σ (1-σ noise ~3.2 × 10-5 Jy/arcsec2). The light blue contour denotes the flux half-peak contour, as shown in Fig. 4. Image scale is 2′′ per pixel and orientation is N up, E left.

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