Abell 2067

Abell 2067 is a galaxy cluster 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.[2] Abell 2061 lies 1.8 megaparsecs south of it and the two are likely interacting.[3]

Abell 2067
Observation data (Epoch J2000)
Constellation(s)Corona Borealis
Right ascension15h 23m 21.9s
Declination+30° 58′ 18″
Redshift0.0740[1]

References
  1. 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.
  2. 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.
  3. 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. arXiv:1107.5597. Bibcode:2011A&A...533A..35V. doi:10.1051/0004-6361/201117149. S2CID 55747728.


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