The NuSTAR and Chandra View of CL 0217+70 and Its Tell-tale Radio Halo

Mergers of galaxy clusters are the most energetic events in the universe, driving shock and cold fronts, generating turbulence, and accelerating particles that create radio halos and relics. The galaxy cluster CL 0217+70 is a remarkable late-stage merger, with a double peripheral radio relic and a giant radio halo. Chandra detects surface brightness (SB) edges that correspond to radio features within the halo. In this work, we present a study of this cluster with Nuclear Spectroscopic Telescope Array and Chandra data using spectro-imaging methods. The global temperature is found to be kT = 9.1 keV. We set an upper limit for the inverse Compton (IC) flux of similar to 2.7x 10(-12) erg s(-1) cm(-2), and a lower limit to the magnetic field of 0.08 mu G. Our local IC search revealed a possibility that IC emission may have a significant contribution at the outskirts of the radio halo emission and on/ near shock regions within similar to 0.6 r(500) of clusters. We detected a hot spot feature in our temperature map coincident with an SB edge, but our investigation on its origin is inconclusive. If the hot spot is the downstream of a shock, we set a lower limit of kT > 21 keV to the plasma that corresponds to M similar to 2. We found three shock fronts within 0.5 r(500). Multiple weak shocks within the cluster center hint at an ongoing merger activity and continued feeding of the giant radio halo. CL 0217+70 is the only example hosting these secondary shocks in multiple form.

Automated summary

Mergers of galaxy clusters are energetic events that generate shock and cold fronts, turbulence, and accelerate particles that create radio halos and relics. The late-stage merger cluster CL 0217+70 is remarkable due to its double peripheral radio relic and giant radio halo. The study using Nuclear Spectroscopic Telescope Array and Chandra data reveals the global temperature, upper limit of inverse Compton flux, and lower limit of magnetic field. Possible significant contributions of IC emission and ongoing merger activity with multiple shocks are found.