NGC 4277 is an intermediate spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 2,533±24 km/s, which corresponds to a Hubble distance of 121.9 ± 8.6 Mly (37.37 ± 2.64 Mpc). It was discovered by German-British astronomer William Herschel on 17 April 1786. NGC 4277 has a possible 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.
Virgo cluster NGC 4277 is a member of the Virgo Cluster.
Supernova One Supernova has been observed in NGC 4277:
SN 2020ftl (Type Ia, mag. 18.5) was discovered by the Catalina Real-time Transient Survey and Mirco Villi on 2 April 2020.
Image gallery
See also List of NGC objects (4001–5000)
References
External links Media related to NGC 4277 at Wikimedia Commons NGC 4277 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images



