Likely new disk growth in a blue-sequence E galaxy.
Left: HI contours overlaid on the optical image of NGC7360, a disky E with counterrotating gas and stars (new VLA data; Kannappan, Matthews, et al. 2006, in prep.). Right: Optical absorption-line cross-correlation profile as a function of slit position along the major axis, revealing a secondary stellar disk rotating with the gas (Kannappan, Guie, & Baker 2006, submitted). Triangles mark the primary stellar rotation curve.