Hercules Cluster
Galaxy cluster in the constellation Hercules From Wikipedia, the free encyclopedia
The Hercules Cluster (Abell 2151) is a cluster of about 200 galaxies[4] some 500 million light-years distant in the constellation Hercules. It is rich in spiral galaxies and shows many interacting galaxies.[5] The cluster is part of the larger Hercules Supercluster, which is itself part of the much larger Great Wall super-structure.[6]
Hercules Cluster | |
---|---|
![]() | |
Observation data (Epoch J2000) | |
Constellation(s) | Hercules |
Right ascension | 16h 05m 15.0s[1] |
Declination | +17° 44′ 55″[1] |
Brightest member | NGC 6041 |
Number of galaxies | 300[2] |
Richness class | 2[3] |
Bautz–Morgan classification | III[3] |
Redshift | 0.03660 (10 972 km/s)[1] |
Distance | 156 Mpc (509 Mly) h−1 0.705 [1] |
X-ray flux | (15.00 ± 12.5%)×10−12 erg s−1 cm−2 (0.1—2.4 keV) [1] |
Other designations | |
Abell 2151 |
The cluster's brightest member is the giant elliptical galaxy NGC 6041.[7]
See also
External links
- NASA Astronomy Picture of the Day: The Hercules Cluster of Galaxies (July 19, 2007)
- NASA Astronomy Picture of the Day: The Hercules Cluster of Galaxies (July 16, 2009)
- Hercules Cluster — University of Alabama
- The Hercules Cluster on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
References
Wikiwand - on
Seamless Wikipedia browsing. On steroids.