| NGC 3269 | |
|---|---|
 DSS image of NGC 3269 | |
| Observation data (J2000 epoch) | |
| Constellation | Antlia |
| Right ascension | 10h 29m 57.08s[1] |
| Declination | −35° 13′ 27.7″[1] |
| Redshift | 0.012601[2] |
| Heliocentric radial velocity | 3754 km/s[2] |
| Distance | 171.7 Mly (52.65 Mpc)[3] |
| Apparent magnitude (V) | 12.26[1] |
| Apparent magnitude (B) | 13.22[1] |
| Characteristics | |
| Type | SB(r)0-a[1] |
| Other designations | |
| MCG -06-23-040, PGC 30945[2] | |
NGC 3269 is a barred spiral or lenticular galaxy in the constellation Antlia. It is a member of the Antlia Cluster, which lies about 40.7 megaparsecs (132.7 million light-years) away.[4]
- ^ a b c d e "Search specification: NGC 3269". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-18.
- ^ a b c "NGC 3269". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-18.
- ^ Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv:astro-ph/0610732. Bibcode:2007ApJ...655..790C. doi:10.1086/510201. S2CID 11672751.
- ^ Dirsch, B.; Richtler, T.; Bassino, L. P. (September 2003). "The globular cluster systems of NGC 3258 and NGC 3268 in the Antlia cluster" (PDF). Astronomy and Astrophysics. 408 (3): 929–939. arXiv:astro-ph/0307200. Bibcode:2003A&A...408..929D. doi:10.1051/0004-6361:20031027. S2CID 763415. Retrieved March 10, 2012.