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NGC 4277
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| NGC 4277 | |
|---|---|
 NGC 4277 imaged by the Vera C. Rubin Observatory | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 20m 03.7208s[1] |
| Declination | +05° 20′ 28.904″[1] |
| Redshift | 0.007295±0.00000667[1] |
| Heliocentric radial velocity | 2,187±2 km/s[1] |
| Distance | 121.9 ± 8.6 Mly (37.37 ± 2.64 Mpc)[1] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 14.2g[1] |
| Characteristics | |
| Type | SAB0/a?(rs)[1] |
| Size | ~21,000 ly (6.45 kpc) (estimated)[1] |
| Apparent size (V) | 1.13′ × 0.81′[1] |
| Other designations | |
| HOLM 368F, VCC 386, 2MASX J12200369+0520161, MCG +01-32-009, PGC 39759, CGCG 042-029[1] | |
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).[1] It was discovered by German-British astronomer William Herschel on 17 April 1786.[2]
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.[3][4]
Virgo cluster
[edit]NGC 4277 is a member of the Virgo Cluster.[4][5]
Supernova
[edit]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.[6]
Image gallery
[edit]-
NGC 6993 imaged by SDSS
See also
[edit]References
[edit]- ^ a b c d e f g h i j k "Results for object NGC 4277". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 29 December 2025.
- ^ Seligman, Courtney. "New General Catalogue Objects: NGC 4277". Celestial Atlas. Retrieved 29 December 2025.
- ^ Asmus, D.; Greenwell, C. L.; Gandhi, P.; Boorman, P. G.; Aird, J.; Alexander, D. M.; Assef, R. J.; Baldi, R. D.; Davies, R. I.; Hönig, S. F.; Ricci, C.; Rosario, D. J.; Salvato, M.; Shankar, F.; Stern, D. (2020). "Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 MPC". Monthly Notices of the Royal Astronomical Society. 494 (2): 1784. arXiv:2003.05959. Bibcode:2020MNRAS.494.1784A. doi:10.1093/mnras/staa766.
- ^ a b "NGC 4277". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 29 December 2025.
- ^ "NAME Virgo Cluster". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 29 December 2025.
- ^ "SN 2020ftl". Transient Name Server. IAU. Retrieved 29 December 2025.
External links
[edit]
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
