Fig. 1
Scattered light images. The HST/ACS images at 0.6 μm (left) and at 0.8 μm (center) and the HST/NICMOS image at 1.1 μm (right). The images are oriented north-up and the HST/ACS images are rebinned to the HST/NICMOS scale of 0.076″/pix. The plotted coordinate system indicates the distance from the star in arcseconds along the two axes. Note the different flux scales in mJy/as2 and the fact that the stellar PSF residuals are heavily truncated in these scales. The object in the SW is a background galaxy.
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