How unusual is the cool-core radio halo cluster CL1821+643 ?
  Massive galaxy clusters with cool-cores typically host diffuse radio sources
called mini-haloes, whereas, those with non-cool-cores host radio haloes. We
attempt to understand the unusual nature of the cool-core galaxy cluster
CL1821+643 that hosts a Mpc-scale radio halo using new radio observations and
morphological analysis of its intra-cluster medium. We present the Giant
Metrewave Radio Telescope (GMRT) 610 MHz image of the radio halo. The spectral
index, $\alpha$ defined as $S\propto \nu^{-\alpha}$, of the radio halo is
$1.0\pm0.1$ over the frequency range of 323 - 610 - 1665 MHz. Archival {\it
Chandra} X-ray data were used to make surface brightness and temperature maps.
The morphological parameters Gini, $M_{20}$ and concentration ($C$) were
calculated on X-ray surface brightness maps by including and excluding the
central quasar (H1821+643) in the cluster. We find that the cluster CL1821+643,
excluding the quasar, is a non-relaxed cluster as seen in the morphological
parameter planes. It occupies the same region as other merging radio halo
clusters in the temperature- morphology parameter plane. We conclude that this
cluster has experienced a non-core-disruptive merger.
