| Abell 2067 | |
|---|---|
| Observation data ( Epoch J2000) | |
| Constellation(s) | Corona Borealis |
| Right ascension | 15h 23m 21.9s |
| Declination | +30° 58′ 18″ |
| Redshift | 0.0740 [1] |
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]
- ^ 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.
- ^ 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.
| Abell 2067 | |
|---|---|
| Observation data ( Epoch J2000) | |
| Constellation(s) | Corona Borealis |
| Right ascension | 15h 23m 21.9s |
| Declination | +30° 58′ 18″ |
| Redshift | 0.0740 [1] |
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]
- ^ 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.
- ^ 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.