| NGC 5876 | |
|---|---|
 The barred spiral galaxy NGC 5876. | |
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 15h 09m 31.5629s[1] |
| Declination | +54° 30′ 23.384″[1] |
| Redshift | 0.010851 [1] |
| Heliocentric radial velocity | 3253 ± 2 km/s[1] |
| Distance | 160.0 ± 11.2 Mly (49.05 ± 3.43 Mpc)[1] |
| Apparent magnitude (V) | 12.7[1] |
| Characteristics | |
| Type | SB(r)ab?[1] |
| Size | ~174,300 ly (53.43 kpc) (estimated)[1] |
| Apparent size (V) | 2.4' x 1.2'[1] |
| Other designations | |
| IRAS F15081+5441, 2MASX J15093156+5430228, IC 1111, UGC 9747, MCG +09-25-028, PGC 54110, CGCG 274-028[1] | |
NGC 5876 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3325 ± 5 km/s, which corresponds to a Hubble distance of 49.05 ± 3.43 Mpc (∼160 million light-years).[1] However, three non redshift measurements give a distance of 65.6 ± 0.346 Mpc (~214 million light-years).[2] The galaxy was discovered by American astronomer Lewis Swift on 11 June 1885. Swift observed the galaxy again on August 27, 1888, and not realizing that he had already observed it, entered the galaxy into the Index Catalogue as IC 1111.[3]
According to the SIMBAD database, NGC 5876 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[4]
One supernova has been observed in NGC 5876: SN 2024igg (type Ia-SC, mag. 17.8).[5]
- ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 5876. Retrieved 15 August 2024.
- ^ "Distance Results for NGC 5876". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 15 August 2024.
- ^ Seligman, Courtney. "NGC 2805". Celestial Atlas. Retrieved 15 August 2024.
- ^ "NGC 5876". SIMBAD astronomical database. Strasbourg Astronomy Data Centre. Retrieved 11 August 2024.
- ^ "SN 2024igg". Transient Name Server. IAU. Retrieved 15 August 2024.