2005/02/23 by Yasuhiro Hashimoto, J. Patrick Henry, G. Hasinger +4
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.1051/0004-6361:20042112
Accepted for publication in A&A. 5 pages, 4 figures
arxiv created 2005/02/23 · openalex publication_date 2005/07/22 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31
We present a study of the galaxy population in the cluster RX J1053.7+5735, one of the most distant X-ray selected clusters of galaxies and one which also shows an unusual double-lobed X-ray morphology, indicative of a possible equal-mass cluster merger. The cluster was discovered during the ROSAT deep pointings in the direction of the Lockman Hole. Using Keck-DEIMOS spectroscopic observations of galaxies in the 20 15 region surrounding RX J1053.7+5735, we secured redshifts for six galaxies in the range , with a mean redshift . This mean redshift agrees well with the cluster X-ray redshift previously estimated from the cluster X-ray Fe-K line, confirming the presence of a cluster at . Galaxies with concordant redshifts are located in both eastern and western sub-clusters of the double cluster structure, which indicates that both sub-clusters are at similar redshifts. This result is also consistent with a previous claim that both eastern and western X-ray lobes have similar X-ray redshifts. Based on their separation of ~250 kpc, these results support the interpretation that RX J1053.7+5735 is an equal-mass cluster merger taken place at , although further direct evidence for a dynamical state of the cluster is needed to make a more definitive statement about the cluster merging state. The six galaxies have a line-of-sight velocity dispersion ~ 650 km s-1, and all six show clear absorption features of CaII H and K and several Balmer lines that are typical of early galaxies at the present epoch, in agreement with their colors. A color–magnitude diagram, constructed from deep optical/NIR observations of the RX J1053.7+5735 field, shows a clear red color sequence. There is an indication that the red sequence in RX J1053.7+5735 lies ~0.3 to the blue of the Coma line, qualitatively consistent with previous studies investigating other clusters at .