RXJ1733.0+4345 (Figure 19) This cluster (around IC1262) has been studied using
BeppoSax by Hudson & Henriksen (2003) and Hudson et al. (2003) who suggest that
there may be diffuse nonthermal emission from a merger shock. They describe the
radio emission as a likely halo, but the combination of images shown here makes
it likely that it is a 400 kpc WAT, with most of the emission resolved away at
the 5" resolution of FIRST.
The observed galaxy (IC 1262) is associated with 4C+43.46.