Suzaku observations of the merging galaxy cluster Abell 2255: The northeast radio relic

We present the results of deep 140 ks Suzaku X-ray observations of the north-east (NE) radio relic of the merging galaxy cluster Abell 2255. The temperature structure of Abell 2255 is measured out to 0.9 times the virial radius (1.9 Mpc) in the NE direction for the first time. The Suzaku temperature map of the central region suggests a complex temperature distribution, which agrees with previous work. Additionally, on a larger-scale, we confirm that the temperature drops from 6 keV around the cluster center to 3 keV at the outskirts, with two discontinuities at r similar to 5' (450 kpc) and similar to 12' (1100 kpc) from the cluster center. Their locations coincide with surface brightness discontinuities marginally detected in the XMM-Newton image, which indicates the presence of shock structures. From the temperature drop, we estimate the Mach numbers to be M-inner similar to 1.2 and, M-outer similar to 1:4. The first structure is most likely related to the large cluster core region (similar to 350-430 kpc), and its Mach number is consistent with the XMM-Newton observation (M similar to 1.24: Sakelliou & Ponman 2006, MNRAS, 367, 1409). Our detection of the second temperature jump, based on the Suzaku key project observation, shows the presence of a shock structure across the NE radio relic. This indicates a connection between the shock structure and the relativistic electrons that generate radio emission. Across the NE radio relic, however, we find a significantly lower temperature ratio (T-1/T-2 similar to 1.44 +/- 0.16 corresponds to M-X (ray) similar to 1.4) than the value expected from radio wavelengths, based on the standard diffusive shock acceleration mechanism (T-1/T-2 > 3.2 or M-Radio > 2.8). This may suggest that under some conditions, in particular the NE relic of A2255 case, the simple diffusive shock acceleration mechanism is unlikely to be valid, and therefore, more a sophisticated mechanism is required.