| NGC 2139 | |
| Image Scale: | 1.3 |
| Epoch: | J2000 |
| Z: | 0.006148 |
| Type: | SAB(rs)cd |
| Appmag V: | 11.6 |
| Appmag B: | 11.98 |
| Notes: | Bulgeless |
NGC 2139 is a barred spiral galaxy in the constellation of Lepus. It was discovered on November 17, 1784, by the German-English astronomer William Herschel. The galaxy is located at a distance of 36.98order=flipNaNorder=flip from the Sun and is receding with a radial velocity of 1,836 km/s.
The overall form of this galaxy is irregular with spiral arms and the appearance of tidal features, suggesting a potential recent merger event. There is no central bulge of significance. The morphological classification is SAB(rs)cd, which indicates a barred spiral galaxy (SAB) with a transitional inner ring structure (rs) and loosely wound spiral arms (cd). It is a star forming galaxy with a formation rate of ·yr−1. There is a plume extending to the south of the galaxy.
A luminous filament runs through the center of the galaxy, which includes a small nuclear cluster. This cluster is only old with a mass of . It is offset at a distance of 320 pc from the center of the galaxy and may come to rest there on a time scale of around 100 million years. The cluster is a source of X-ray emission.
During September 1995, a type II supernova was discovered by Robert Evans and associates. Designated SN 1995ad, it was positioned in one of the spiral arms, west and south of the NGC 2139 nucleus. The recession velocity was consistent with that of the host galaxy.
2 other supernovae have been observed in NGC 2139: SN 2022qhy (type Ibn, mag. 15.9)[1] and SN 2023zcu (type II, mag. 19.1).[2]