Optical analysis of the poor clusters Abell 610, Abell 725, and Abell 796, containing diffuse radio sources

2008/05/15 by W. Boschin, R. Barrena, M. Girardi +2 · 1 citation
Physics and Astronomy · #Abell 2744 #Astronomy #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy group #Physics #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809620

18 pages, 20 figures, 7 tables. Astronomy & Astrophysics, in press

openalex publication_date 2008/05/15 · arxiv created 2008/06/18 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. We study the dynamical status of the poor, low X-ray luminous galaxy clusters Abell 610, Abell 725, and Abell 796 (at , 0.09, and 0.16, respectively), containing diffuse radio sources (relic, relic, and possible halo, respectively).

Citations

• A study of the core of the Shapley Concentration - I. The sample
• A comparison of radio and X-ray morphologies of four clusters of galaxies containing radio halos
• Radio Halo and Relic Candidates from the Westerbork Northern Sky Survey
• Radio halo and relic candidates from the NRAO VLA Sky Survey
• Internal dynamics of the massive cluster Abell 697: a multiwavelength analysis
• An analysis of variance test for normality (complete samples)

Cited by

• Abell 315: reconciling cluster mass estimates from kinematics, X-ray, and lensing

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