As Fig. 6, but for model C. The diffuse X-ray emission observed by Chandra is produced by the hot spots, and there are no lobes. We also show how the flux of the western hot spot would appear if there were no CMB. This shows that most of the X-ray diffuse flux is the result of external Compton process with the CMB photons, while the SSC component is very weak. At high energies the flux is dominated by the second-order Compton scatterings (second IC). The parameters adopted for the hot spots are given in Table 2.