Lynx Supercluster

The Lynx Supercluster was discovered in 1999[1] as ClG J0848+4453, a name now used to describe the western cluster, with ClG J0849+4452 being the eastern one.[2] It contains at least two clusters, designated RXJ 0848.9+4452 (at redshift z=1.26) and RXJ 0848.6+4453 (redshift z=1.27) . At the time of discovery, it was the most distant known supercluster[3] with a comoving distance of 9 billion light years. Additionally, seven smaller groups of galaxies are associated with the supercluster.[4] Through electromagnetic radiation and how it reacts with matter, we have been able to find three groupings of stars and two x-ray clusters within the Lynx.[5]

The observation of the Lynx Supercluster has allowed other locations in proximity to be found. These locations are of special interest because of their high density, which has turned into the discovery of the seven smaller groups of galaxies mentioned above.[6]

A study has been conducted between the clusters in the Lynx, to examine and compare their color and shift.

References
  1. Rosati, P.; et al. (1999). "An X-Ray-Selected Galaxy Cluster at z = 1.26". The Astronomical Journal. 118 (1): 76–85. arXiv:astro-ph/9903381. Bibcode:1999AJ....118...76R. doi:10.1086/300934. S2CID 2560006.
  2. "Lynx Supercluster". SIMBAD.
  3. Nakata, F.; et al. (2004). "Discovery of a large-scale clumpy structure of the Lynx supercluster at z~1.27". Proceedings of the International Astronomical Union. Cambridge University Press. 2004: 29–33. Bibcode:2004ogci.conf...29N. doi:10.1017/S1743921304000080. ISBN 0-521-84908-X.
  4. Ohta, K.; et al. (2003). "Optical Identification of the ASCA Lynx Deep Survey: An Association of Quasi-Stellar Objects and a Supercluster at z = 1.3?". The Astrophysical Journal. 598 (1): 210–215. arXiv:astro-ph/0308066. Bibcode:2003ApJ...598..210O. doi:10.1086/378690. S2CID 117171639.
  5. Kim, Jae-Woo; Im, Myungshin; Lee, Seong-Kook; Edge, Alastair C.; Hyun, Minhee; Kim, Dohyeong; Choi, Changsu; Jueun Hong; Jeon, Yiseul (2016). "Discovery of a Supercluster at z 0.91 and Testing the ΛCDM Cosmological Model". The Astrophysical Journal Letters. 821 (1): L10. arXiv:1604.03254. Bibcode:2016ApJ...821L..10K. doi:10.3847/2041-8205/821/1/L10. ISSN 2041-8205. S2CID 118568359.
  6. Nakata, F.; Kodama, T.; Shimasaku, K.; Doi, M.; Furusawa, H.; Hamabe, M.; Kimura, M.; Komiyama, Y.; Miyazaki, S. (2005-03-11). "Discovery of a large-scale clumpy structure around the Lynx supercluster at z 1.27". Monthly Notices of the Royal Astronomical Society. 357 (4): 1357–1362. arXiv:astro-ph/0412460. Bibcode:2005MNRAS.357.1357N. doi:10.1111/j.1365-2966.2005.08756.x. ISSN 0035-8711. S2CID 15053608.

[1]

  1. Mei, Simona (2006). "Evolution of the Color-Magnitude relation in High-Redshift Clusters: Early-type Galaxies in the Lynx Supercluster at z~1.26". Astrophys. J. 644 (2): 759–768. arXiv:astro-ph/0604082. Bibcode:2006ApJ...644..759M. doi:10.1086/503826. S2CID 18666447.
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