We present the results of a Chandra observation of the cooling core cluster Abell 2063 .
Spectral analysis shows that there is cool gas ( 2 keV ) associated with the cluster core , which is more than a factor of 2 cooler than the outer cluster gas ( 4.1 keV ) .
There also is spectral evidence for a weak cooling flow , \dot { M } \approx 20 \mbox { $M _ { \odot } $ } yr ^ { -1 } .
The cluster exhibits a complex structure in the center that consists of several bright knots of emission , a depression in the emission to the north of the center of the cluster , and a shell of emission surrounding it .
The depression in the X-ray emission is coincident with the position of the north-eastern radio lobe of the radio source associated with the cluster-central galaxy .
The shell surrounding this region appears to be hotter , which may be the result of a shock that has been driven into the gas by the radio source .
The power output of the radio source appears to be sufficient to offset the cooling flow , and heating of the gas through shocks is a possible explanation of how the energy transfer is established .