NGC 1404 is an elliptical galaxy in the Southern constellation Eridanus. It was discovered by British astronomer John Herschel on November 28, 1837. Based on the tip of the red-giant branch distance indicator, it lies at a distance of approximately 60 million light-years from the Milky Way. It is one of the brightest members of the Fornax Cluster.
Characteristics As usual with most elliptical galaxies, NGC 1404 is rich in globular clusters, with a population of them that has been estimated to be around 725; however it has been proposed it could have lost most of its globular clusters due to gravitational interactions with NGC 1399, the brightest galaxy of the Fornax Cluster. Studies using the X-ray telescope Chandra show how the ram-pressure stripping caused by the motion of NGC 1404 through Fornax' intracluster medium is stripping the galaxy of its hot gas, leaving behind a large trail.
Supernovae Two supernovae have been observed in NGC 1404:
SN 2007on (Type Ia, mag. 14.9) was discovered by Christian Pollas and the TAROT collaboration on 5 November 2007. SN 2011iv (Type Ia, mag. 12.8) was discovered by Stuart Parker on 2 December 2011.
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References
External links Media related to NGC 1404 at Wikimedia Commons NGC 1404 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images



