NGC 4696
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| NGC 4696 | |
|---|---|
 A multiwavelength image of NGC 4696. X-ray emission is red, radio emission is blue, and infrared emission is green. |
|
| Observation data (J2000 epoch) | |
| Constellation | Centaurus |
| Right ascension | 12h 48m 49.3s[1] |
| Declination | -41° 18′ 40″[1] |
| Redshift | 2958 ± 15 km/s[1] |
| Distance | 116 ± 9 Mly (35 ± 3 Mpc)[2] |
| Type | E1 pec[1] |
| Apparent dimensions (V) | 4′.5 × 3′.2[1] |
| Apparent magnitude (V) | 11.4[1] |
| Other designations | |
| PGC 43296[1] | |
| See also: Galaxy, List of galaxies | |
NGC 4696 is an elliptical galaxy. It lies around 150 million light years away in the constellation Centaurus. It is the brightest galaxy in the Centaurus Cluster, a large, rich cluster of galaxies in the constellation of the same name.[3] The galaxy is surrounded by many dwarf elliptical galaxies also located within the cluster.[3]
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[edit] See also
[edit] References
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 4696. http://nedwww.ipac.caltech.edu/. Retrieved 2006-10-19.
- ^ J. L. Tonry, A. Dressler, J. P. Blakeslee, E. A. Ajhar, A. B. Fletcher, G. A. Luppino, M. R. Metzger, C. B. Moore (2001). "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances". Astrophysical Journal 546 (2): 681–693. arXiv:astro-ph/0011223. Bibcode 2001ApJ...546..681T. doi:10.1086/318301.
- ^ a b A. Sandage, J. Bedke (1994). Carnegie Atlas of Galaxies. Washington, D.C.: Carnegie Institution of Washington. ISBN 0-87279-667-1.
Coordinates: 
12h 48m 49.3s, −41° 18′ 40″
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