NGC 2997
From Wikipedia, the free encyclopedia
NGC 2997 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Antlia |
Right ascension | 09h 45m 38.8s[1] |
Declination | −31° 11′ 28″[1] |
Distance | 39.8 Mly[2] |
Type | SA(s)c[1] |
Apparent dimensions (V) | 8′.9 × 6′.8[1] |
Apparent magnitude (V) | 10.1[1] |
Other designations | |
ESO 434- G 35,[1] PGC 27978[1] | |
See also: Galaxy, List of galaxies |
NGC 2997 is a face-on unbarred spiral galaxy about 40 million light-years away in the constellation Antlia.[2] It is the brightest galaxy of the NGC 2997 group of galaxies.
NGC 2997 is particularly notable for a nucleus surrounded by a chain of hot giant clouds of ionized hydrogen. It is featured on the cover of the first edition of Galactic Dynamics by James Binney and Scott Tremaine.[3]
Other resources
See also
External links
- APOD: Grand Design Spiral Galaxy NGC 2997 (10/30/1996)
- NGC 2997 in Antlia
- NGC 2997 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "NASA/IPAC Extragalactic Database". Results for NGC 2997. Retrieved 2006-11-25.
- ↑ 2.0 2.1 Hess K. M., Pisano D. J., Wilcots E. M., Chengular J. N. "Anomalous HI in NGC 2997". Retrieved 2006-11-25.
- ↑ "Binney, J. and Tremaine, S.: Galactic Dynamics.". Princeton University Press. Retrieved 2007-04-09.
Coordinates: 09h 45m 38.8s, −31° 11′ 28″
|
This article is issued from Wikipedia. The text is available under the Creative Commons Attribution/Share Alike; additional terms may apply for the media files.