NGC 4013 is an edge-on barred spiral galaxy about 55 millionlight-years away in the constellationUrsa Major. The disk of NGC 4013 shows a distinct "peanut"-shaped bulge in long exposure photographs that N-body computer simulations suggest is consistent with a stellar bar seen perpendicular to the line of sight.
Infrared image of the galaxy showing a ring of heavy star formation
A recent deep color image of NGC 4013 revealed a looping tidal stream of stars extending over 80 thousand light-years from the Galactic Center. This structure is thought to be the remnants of a smaller galaxy that was torn apart by tidal forces as it collided with NGC 4013.
In January, 1991, M. Shaw reported an apparent supernova seen on an image taken December 30, 1989, at apparent magnitude 12, which was then given the designation SN 1989Z. However, later analysis suggested that this object was actually a foreground variable star, or an outburst from a cataclysmic variable star.
123456"SIMBAD". Results for NGC 4013. Retrieved 2009-12-25.
↑Combes, F. and Sanders, R.H., "Formation and properties of persisting stellar bars", Astronomy and Astrophysics, vol. 96, no. 1-2, Mar. 1981, p. 164-173.