NGC 4696 is an elliptical galaxy in the constellation Centaurus. Its velocity with respect to the cosmic microwave background is 3,251±23 km/s, which corresponds to a Hubble distance of 156.4 ± 11.0 Mly (47.95 ± 3.38 Mpc). However, 25 non-redshift measurements give a much closer mean distance of 122.63 ± 3.90 Mly (37.600 ± 1.196 Mpc). It was discovered by British astronomer James Dunlop on 7 May 1826. NGC 4696 is the brightest galaxy in the Centaurus Cluster, a large, rich cluster of galaxies in the constellation of the same name. The galaxy is surrounded by many dwarf elliptical galaxies also located within the cluster. There is believed to be a supermassive black hole at the center of the galaxy.
Supernova One supernova has been observed in NGC 4696:
SN 2017ejb (Type Ia, mag. 17.2078) was discovered by the Distance Less Than 40 Mpc Survey (DLT40) on 28 May 2017.
References
External links Media related to NGC 4696 at Wikimedia Commons http://www.eurekalert.org/pub_releases/2010-08/eic-n4a081010.php http://apod.nasa.gov/apod/ap161207.html


