Abell 2065
(Redirected from Corona Borealis Cluster)
| Abell 2065 | |
|---|---|
 Amateur image taken with 10" telescope | |
| Observation data (Epoch J2000) | |
| Constellation(s) | Corona Borealis |
| Right ascension | 15h 22m 31.8s[1] |
| Declination | +27° 42′ 04″[1] |
| Redshift | (21, 673 km/s)[1] |
Abell 2065 is a highly concentrated galaxy cluster in the constellation of Corona Borealis containing over 400 member galaxies, the brightest of which are 16th magnitude. The cluster is more than one billion light-years from Earth.[citation needed] On a larger scale still, Abell 2065, along with Abell 2061, Abell 2067, Abell 2079, Abell 2089, and Abell 2092, make up the Corona Borealis Supercluster.[2]
References
[edit]- ^ a b c Pearson, David W.; Batiste, Merida; Batuski, David J. (2014). "The Largest Gravitationally Bound Structures: The Corona Borealis Supercluster - Mass and Bound Extent". Mon. Not. R. Astron. Soc. 441 (2): 1601–1614. arXiv:1404.1308. Bibcode:2014MNRAS.441.1601P. doi:10.1093/mnras/stu693.
- ^ Postman, M.; Geller, M. J.; Huchra, J. P. (1988). "The dynamics of the Corona Borealis supercluster". Astronomical Journal. 95: 267–83. Bibcode:1988AJ.....95..267P. doi:10.1086/114635.
