| NGC 5967 | |
|---|---|
NGC 5967 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Apus |
| Right ascension | 15h 48m 15.9241s |
| Declination | −75° 40′ 22.219″ |
| Redshift | 0.009623±0.0000190 |
| Heliocentric radial velocity | 2,885±6 km/s |
| Distance | 116.04 ± 2.62 Mly (35.578 ± 0.802 Mpc) |
| Apparent magnitude (V) | 12.6b |
| Characteristics | |
| Type | SAB(rs)c |
| Size | ~115,800 ly (35.50 kpc) (estimated) |
| Apparent size (V) | 2.9′ × 1.7′ |
| Other designations | |
| ESO 042- G 010, IRAS 15421-7531, 2MASX J15481597-7540226, PGC 56078 | |
NGC 5967 is a barred spiral galaxy in the constellation of Apus. Its velocity with respect to the cosmic microwave background is 2,961±8 km/s, which corresponds to a Hubble distance of 142.5 ± 10.0 Mly (43.68 ± 3.06 Mpc). However, 18 non-redshift measurements give a much closer mean distance of 116.04 ± 2.62 Mly (35.578 ± 0.802 Mpc). It was discovered by British astronomer John Herschel on 7 June 1836.
NGC 5967 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.
One supernova has been observed in NGC 5967: