NGC 2545 is a barred spiral galaxy in the constellation of Cancer. Its velocity with respect to the cosmic microwave background is 3,613±16 km/s, which corresponds to a Hubble distance of 173.8 ± 12.2 Mly (53.29 ± 3.74 Mpc). Additionally, 15 non-redshift measurements give a closer distance of 158.97 ± 11.44 Mly (48.740 ± 3.507 Mpc). It was discovered by German-British astronomer William Herschel on 11 January 1787. NGC 2545 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. It is also a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
NGC 2545 group NGC 2545 is a member of a group of galaxies named after it (also known as LGG 156). This group contains 5 galaxies, including NGC 2565, UGC 4308, CGCG 119-44, and CGCG 119-56.
Supernova One supernova has been observed in NGC 2545:
SN 2008hn (Type Ic, mag. 18.4) was discovered by the Lick Observatory Supernova Search (LOSS) on 25 November 2008.
See also List of NGC objects (2001–3000)
References
External links Media related to NGC 2545 at Wikimedia Commons NGC 2545 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


