NGC 2325 is an elliptical galaxy in the constellation of Canis Major. Its velocity with respect to the cosmic microwave background is 2,356±25 km/s, which corresponds to a Hubble distance of 113.4 ± 8.1 Mly (34.76 ± 2.48 Mpc). However, 16 non-redshift measurements give a much closer mean distance of 74.53 ± 3.94 Mly (22.850 ± 1.209 Mpc). It was discovered by British astronomer John Herschel on 1 February 1837. NGC 2325 is a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure. It also has an active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Galaxy group NGC 2325 is a member of a galaxy group known as [CHM2007] HDC 421. The group contains at least eight galaxies, including IC 456, ESO 427-22, MCG-05-17-006, MCG-05-17-004, MCG-05-17-008, and two others.
Supernova One supernova has been observed in NGC 2325:
SN 2010ih (Type Ia, mag. 13.3) was discovered by The CHilean Automatic Supernova sEarch (CHASE) on 29 September 2010. A prediscovery image taken on 16 September showed it at magnitude 12.8, making it the brightest supernova of 2010.
See also List of NGC objects (2001–3000)
References
External links Media related to NGC 2325 at Wikimedia Commons NGC 2325 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


