NGC 5291 explained
NGC 5291 |
Credit: | ESO. |
Epoch: | J2000 |
Type: | E pec[1] |
Z: | 4378 ± 6 km/s |
Appmag V: | 15.1 |
Size V: | 1′.1× 0′.7 |
Constellation Name: | Centaurus |
Names: | PGC 48893 |
NGC 5291 is a system of interacting galaxies in the constellation Centaurus. It is surrounded by a collisional ring, containing a young and star-forming tidal dwarf galaxy,[2] where dark matter has been detected.[3]
See also
External links
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 5291 . 2007-04-03.
- Médéric Boquien . 4 . Pierre-Alain Duc . Jonathan Braine . Elias Brinks . Ute Lisenfeld . Vassilis Charmandaris. amp. Polychromatic view of intergalactic star formation in NGC 5291. Astronomy & Astrophysics. 2007. 467 . 1. 93–106. 2007A&A...467...93B. 10.1051/0004-6361:20066692. astro-ph/0703002 . 5822678 .
- Frédéric Bournaud . 4 . Pierre-Alain Duc . Elias Brinks . Médéric Boquien . Philippe Amram . Ute Lisenfeld . Bärbel S. Koribalski . Bärbel Koribalski. Fabian Walter. Vassilis Charmandaris. amp. Missing Mass in Collisional Debris from Galaxies. Science. 2007. 316. 1166–1169. 2007Sci...316.1166B. 10.1126/science.1142114 . 17495138 . 5828. 0705.1356. 20946839 .