Astronomy:Abell 2067
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Short description: Galaxy cluster in Corona Borealis
| Abell 2067 | |
|---|---|
 Abell 2067 seen by DESI Legacy Survey DR11 | |
| Observation data (Epoch J2000) | |
| Constellation(s) | Corona Borealis |
| Right ascension | 15h 23m 21.9s |
| Declination | +30° 58′ 18″ |
| Redshift | 0.0740[1] |
| Distance (co-moving) | 426 MPC |
| Other designations | |
| Abell 2067; ABELL 2067; SCL 158 NED04; MCXC J1523.1+3050; [YSS2008] 274[2] | |
Abell 2067 is a galaxy cluster in the Abell catalogue[3] and is located in the constellation of Corona Borealis. On a larger scale, Abell 2067, along with Abell 2061, Abell 2065, Abell 2079, Abell 2089, and Abell 2092, make up the Corona Borealis Supercluster.[4][5] Abell 2061 lies 1.8 megaparsecs south of it and the two are likely interacting.[6]
References
- ↑ 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. doi:10.1093/mnras/stu693. Bibcode: 2014MNRAS.441.1601P.
- ↑ "NED results for Abell 2067". California Institute of Technology. https://ned.ipac.caltech.edu/byname?objname=Abell+2067.
- ↑ Abell, G. O. (1958). "The Distribution of Rich Clusters of Galaxies". The Astrophysical Journal Supplement Series 3: 211. doi:10.1086/190036. Bibcode: 1958ApJS....3..211A.
- ↑ Postman, M.; Geller, M. J.; Huchra, J. P. (1988). "The dynamics of the Corona Borealis supercluster". Astronomical Journal 95: 267–83. doi:10.1086/114635. Bibcode: 1988AJ.....95..267P.
- ↑ Einasto, M.; Einasto, J.; Tago, E.; Müller, V.; Andernach, H. (2001). "Optical and X-Ray Clusters as Tracers of the Supercluster-Void Network. I. Superclusters of Abell and X-Ray Clusters". The Astronomical Journal 122 (5): 2222–2242. doi:10.1086/323707. Bibcode: 2001AJ....122.2222E.
- ↑ van Weeren, R. J.; Brüggen, M.; Röttgering, H. J. A.; Hoeft, M.; Nuza, S. E.; Intema, H. T. (2011). "Radio continuum observations of new radio halos and relics from the NVSS and WENSS surveys. Relic orientations, cluster X-ray luminosity, and redshift distributions". Astronomy & Astrophysics 533 (A35): 20. doi:10.1051/0004-6361/201117149. Bibcode: 2011A&A...533A..35V.
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