| NGC 4027 | |
|---|---|
 ESO image of NGC 4027 (mirrored). | |
| Observation data (J2000 epoch) | |
| Constellation | Corvus |
| Right ascension | 11h 59m 30.2s[1] |
| Declination | −19° 15′ 55″[1] |
| Redshift | 1671 ± 6 km/s[1] |
| Distance | 83 Mly (25.6 Mpc)[2] |
| Apparent magnitude (V) | 11.7[1] |
| Characteristics | |
| Type | SB(s)dm[1] |
| Apparent size (V) | 3'.2 × 2'.4[1] |
| Other designations | |
| UGCA 260, PGC 37773, Arp 22, VV 066, VIII Zw 158[1] | |
NGC 4027 (also known as Arp 22) is a barred spiral galaxy approximately 83 million light-years away[2] in the constellation Corvus. It is also a peculiar galaxy because one of its spiral arms goes out more than the other. This is probably due to a galactic collision in NGC 4027's past.
One supernova has been observed in NGC 4027: SN 1996W (type II, mag. 16).[3]
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 4027. Retrieved 2006-10-31.
- ^ a b "Distance Results for NGC 4027". NASA/IPAC Extragalactic Database. Retrieved 2010-05-16.
- ^ Transient Name Server entry for SN 1996W. Retrieved 30 March 2023.