We present an X-ray, radio and optical study of the cluster A2717. The
central D galaxy is associated with a Wide-Angled-Tailed (WAT) radio source. A
Rosat PSPC observation of the cluster shows that the cluster has a well
constrained temperature of 2x10^7 K. The pressure of the intracluster medium
was found to be comparable to the mininum pressure of the radio source
suggesting that the tails may in fact be in equipartition with the surrounding
hot gas.Comment: 7 pages, 6 Postscript figures, to appear in Astronomy and
Astrophysics 199
