A non cool-core 4.6-keV cluster around the bright nearby radio galaxy PKS B1416-493

We present new X-ray (Chandra) and radio (ATCA) observations of the z = 0.09 radio galaxy PKSB1416-493, amember of the southern equivalent of the 3CRR sample. We find the source to be embedded in a previously unrecognized bright kT = 4.6-keV non cool-core cluster. The discovery of new clusters of such high temperature and luminosity within z = 0.1 is rare. The radio source was chosen for observation based on its intermediate FR I/II morphology. We identify a cavity coincident with the northeast lobe, and excess counts associated with the southwest lobe that we interpret as inverse-Compton X-ray emission. The jet power, at 5.3 x 10(44) erg s(-1), when weighted by radio source density, supports suggestions that radio sources of intermediate morphology and radio power may dominate radio-galaxy heating in the local Universe.