Distribution of the gas density as a function of the radial distance from the center of the cluster (black curve) and the radial distribution of accelerated particles at different energies (solid, 10 GeV; dotted, 100 GeV), considering propagation in Bohm (blue), Kraichnan (green), or Kolmogorov (red) turbulence. The highest value for the wind luminosity, L_w, 2, was assumed in the calculations.