NGC 3370


'NGC 3370' (also known as '''UGC 5887''', nicknamed '''Silverado Galaxy''') is a spiral galaxy about 98 million light-years away in the constellation Leo. It is similar in size to our own Milky Way. It was probably discovered by William Herschel between September 7, 1782 and his death in 1822. NGC 3370 exhibits intricate spiral arm structure that is sprinkled with hot areas where new stars are forming. NGC 3370's center has well defined dust lanes and an unusually ill-defined nucleus. This galaxy contains a combination of young stars in the bluer regions and older stars in the yellowish core. The mass of NGC 3370 is estimated to be about the same as our own Milky Way at around 1011 solar masses. NGC 3370 is sometimes referred to as the 'Silverado galaxy'.
NGC 3370 was observed (probably discovered) by William Herschel who gave it the designation 'II 81' and John Herschel who gave it the designation 750. The object has a surface brightness of 13 and a position angle of 140°. William Herschel cataloged 'II 80' to NGC 3348 before and 'II 82' to NGC 3455 after NGC 3370.



Contents
History
See also
External links
References

History


On November 14 1994, S. Van Dyk and the Leuschner Observatory Supernova Search took an image that led to their discovery of a bright supernova in NGC 3370. This was well before the maximal light of the supernova which has been estimated to have occurred in the range November 30 to December 1. This stellar outburst briefly outshone all of the tens of billions of other stars in its galaxy. Although supernova are common, with one exploding every few seconds somewhere in the universe, this one was special. Designated SN 1994ae, this supernova was one of the nearest and best observed supernova since the advent of modern digital detectors. The supernova was also a member of a special subclass of supernovae, the type Ia, the best tool astronomers have to chart the growth rate of the expanding universe. The supernova was located at 10h 44m 21.52s +17° 32′ 20.7′′.

See also



New General Catalogue (NGC)

Spiral Galaxy NGC 1365

External links



'HST': Celestial Composition

Ho et al., BVRI Photometry of Supernovae

NGC 3370 at ESA/Hubble

References




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