NGC 4611 is an intermediate spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 6,437 ± 22 km/s, which corresponds to a Hubble distance of 94.9 ± 6.7 Mpc (~310 million light-years).[1] It was discovered by French astronomer Édouard Stephan on 17 May 1881.[2] This galaxy was also observed by the American astronomer Lewis Swift on 20 April 1889, and listed in the Index Catalogue as IC 805.[2]
| NGC 4611 | |
|---|---|
 NGC 4611 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 41m 25.4331s[1] |
| Declination | +13° 43′ 46.198″[1] |
| Redshift | 0.020404[1] |
| Heliocentric radial velocity | 6117 ± 1 km/s[1] |
| Distance | 309.7 ± 21.7 Mly (94.94 ± 6.65 Mpc)[1] |
| Apparent magnitude (V) | 14.3[1] |
| Characteristics | |
| Type | Sbc C[1] |
| Size | ~130,100 ly (39.89 kpc) (estimated)[1] |
| Apparent size (V) | 1.2′ × 0.2′[1] |
| Other designations | |
| IRAS F12389+1400, 2MASX J12412541+1343458, IC 805, UGC 7849, MCG +02-32-179, PGC 42564[1] | |
According to the SIMBAD database, NGC 4611 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.[3]
Supernova
editSee also
editReferences
edit- 1 2 3 4 5 6 7 8 9 10 11 "Results for object NGC 4611". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 23 July 2024.
- 1 2 Seligman, Courtney. "New General Catalogue Objects: NGC 4611". Celestial Atlas. Retrieved 13 December 2024.
- ↑ "NGC 4611". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 13 December 2024.
- ↑ "SN 2023dtz". Transient Name Server. IAU. Retrieved 13 December 2024.
External links
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Media related to NGC 4611 at Wikimedia Commons- NGC 4611 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
