In this paper, an analysis of observational data on rich galaxy clusters is presented. Based on the collected observational data, the values of the concentration degree and the anisotropy parameter are determined for 40 rich galaxy clusters. The relationships between the anisotropy parameter and the concentration degree with the main physical characteristics of rich galaxy clusters are studied. The corresponding empirical formulas between the anisotropy parameter and the concentration degree with the physical parameters of rich galaxy clusters are found.
Kutlimuratov et al. (Mon,) studied this question.