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We present a radio and X-ray study of PKS 1353-341, the brightest clustergalaxy radio source at the center of a recent Chandra-discovered X-ray cluster.Our multi-frequency VLA images reveal an edge-brightened (FR-II), double-lobedstructure with total ~50 kpc extent and 1.5 GHz power of $1.2\times10^{25}$ WHz$^{-1}$, separated from the bright, arcsecond-scale core. We reanalyzed theChandra data and found the X-ray emitting AGN is offset by ~9 kpc from acompact X-ray cool-core with temperature, $kT=3.1\pm0.5$ keV, and a radius of~22 kpc, surrounded by a hotter $kT=6.3\pm0.7$ keV gas out to ~50 kpc. Theoffset suggests sloshing inside the cool-core induced by a minor merger or apast outburst of the AGN that produced the large-scale radio lobes. Thecomparable spatial scales of the lobes with the interface between the differenttemperature X-ray plasma indicate the lobes are actively heating the outerlayers of what is now a remnant compact cool-core. Our dual-frequency VLBAimages reveal substructure in the central radio source, consisting of a radiocore with double-sided pc-scale jets pointing toward the kpc-scale structures.The northern jet is detected only at 8.4 GHz, indicating its emission is behindan absorbing torus or disk. We also measured faster apparent motions in thesouthern jet up to $1.9\pm1.1c$ than in the northern jet ($0.8\pm0.5c$). Whilethe VLBA observations indicate the southern jet is aligned slightly closer toour line of sight, the asymmetries are overall modest and imply minimalprojection effects in the large-scale radio structures.

Extended Radio Structures and a Compact X-ray Cool-Core in the Cluster Source PKS 1353-341