The Cluster of Galaxies Surrounding Cygnus A II: New Velocities and a   Dynamical Model
  We have spectroscopically identified 77 new members of the Cygnus A cluster, bringing the total to 118 galaxies consistent with cluster membership. We use these data combined with the results from X-rays to deduce a dynamical model for the system. The data are consistent with a cluster-cluster merger viewed at a projection angle of 30-45 degrees, 0.2-0.6 Gyr prior to core passage. We estimate the richness of the combined cluster system at Abell richness class 2 or greater, suggesting the merger of two richness class 1 clusters. 
M. J. Ledlow (Gemini), F. N. Owen (NRAO), N. A. Miller (NRAO)