We study the dynamical status of the poor, low X-ray luminous galaxy clusters Abell 610, Abell 725, and Abell 796 (at z=0.1, 0.09, and 0.16, respectively), containing diffuse radio sources (relic, relic, and possible halo, respectively). Our analysis is based on new spectroscopic data obtained at the William Herschel Telescope for 158 galaxies, new photometry obtained at the Isaac Newton Telescope with the addition of data recovered from the Data Release 5 of the Sloan Digital Sky Survey. We use statistical tools to select 57, 36, and 26 cluster members and to analyze the kinematics of cluster galaxies, as well as to study the 2D cluster structure.
Cone search capability for table J/A+A/487/33/table4 (Velocity catalog of 51 spectroscopically measured galaxies in the field of A725)
Cone search capability for table J/A+A/487/33/table5 (Velocity catalog of 99 spectroscopically measured galaxies in the field of A796)
Cone search capability for table J/A+A/487/33/table1 (Velocity catalog of 165 spectroscopically measured galaxies in the field of A610)