NGC 5907
From Wikipedia, the free encyclopedia
NGC5907 | |
Observation data | |
---|---|
Constellation | Draco |
Right ascension | 15h 15m 53.8s[1] |
Declination | ±56° 19′ 44″[1] |
Distance | 3.9×106 |
Type | Sb+ |
Other designations | |
H II.759, GC 4087, h 1917, Splinter Galaxy | |
See also: Galaxy, List of galaxies |
NGC 5907 is a spiral galaxy located approximately 39 million light years from Earth. It has an anomalously low metallicity and few detectable giant stars, being apparently composed almost entirely of dwarf stars.[2]
The galaxy was discovered in 1788 by William Herschel. It is a member of the NGC 5866 Group. Supernova 1940A occurred in this galaxy.[3]
[edit] References
- ^ a b NASA/IPAC Extragalactic Database. Results for various galaxies. Retrieved on 2006-10-17.
- ^ Liu, M. C.; Marleau, F. R.; Graham, J. R.; Charlot, S.; Sackett, P.; Zepf, S. E. (12 1998). "Weighing the Stellar Content of NGC 5907's Dark Matter Halo". Bulletin of the American Astronomical Society 30: 1258.
- ^ NGC 5907