NGC 4617 is a spiral galaxy in the constellation of Canes Venatici. Its velocity with respect to the cosmic microwave background is 4,831±13 km/s, which corresponds to a Hubble distance of 232.4 ± 16.3 Mly (71.25 ± 4.99 Mpc). However, four non-redshift measurements give a closer mean distance of 198.96 ± 2.10 Mly (61.000 ± 0.644 Mpc). It was discovered by German-British astronomer William Herschel on 9 March 1788. NGC 4617 is an active galaxy nucleus candidate, 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.
Supernovae Two supernovae have been observed in NGC 4617:
SN 2005ab (Type II, mag. 16.7) was discovered by Japanese astronomer Kōichi Itagaki on 5 February 2005. SN 2007ss (Type Ia, mag. 16.6) was discovered by Japanese astronomer Yoshimi Ichimura on 20 December 2007.
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4617 at Wikimedia Commons NGC 4617 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


