We report the discovery of a nearly edge-on disk about the A0 star HD 32297 seen in light scattered by the disk grains revealed in NICMOS PSF-subtracted coronagraphic images. The disk extends to a distance of at least 400 AU (3.3″) along its major axis with a 1.1 μm flux density of 4.81 ± 0.57 mJy beyond a radius of 0.3″ from the coronagraphically occulted star. The fraction of 1.1 μm starlight scattered by the disk, 0.0033 ± 0.0004, is comparable to its fractional excess emission at 25 + 60 μm of ～0.0027 as measured from IRAS data. The disk appears to be inclined 10.5° ± 2.5° from an edge-on viewing geometry, with its major axis oriented 236.5 ± 1° eastward of north. The disk exhibits unequal brightness on opposing sides and a break in the surface brightness profile along the NE-side disk major axis. Such asymmetries might implicate the existence of one or more (unseen) planetary mass companions.
展开▼
