Chandra and XMM-Newton observations of A2256: Cold fronts, merger shocks, and constraint on the IC emission

Chong Ge, Ruo Yu Liu, Ming Sun, Heng Yu, Lawrence Rudnick, Jean Eilek, Frazer Owen, Sarthak Dasadia, Mariachiara Rossetti, Maxim Markevitch, Tracy E. Clarke, Thomas W. Jones, Simona Ghizzardi, Tiziana Venturi, Alexis Finoguenov, Dominique Eckert

Research output: Contribution to journalArticlepeer-review

Abstract

We present the results of deep Chandra and XMM-Newton observations of a complex merging galaxy cluster Abell 2256 (A2256) that hosts a spectacular radio relic (RR). The temperature and metallicity maps show clear evidence of a merger between the western subcluster (SC) and the primary cluster (PC). We detect five X-ray surface brightness edges. Three of them near the cluster centre are cold fronts (CFs): CF1 is associated with the infalling SC; CF2 is located in the east of the PC; and CF3 is located to the west of the PC core. The other two edges at cluster outskirts are shock fronts (SFs): SF1 near the RR in the NW has Mach numbers derived from the temperature and the density jumps, respectively, of MT = 1.62 ± 0.12 and Mρ = 1.23 ± 0.06; SF2 in the SE has MT = 1.54 ± 0.05 and Mρ = 1.16 ± 0.13. In the region of the RR, there is no evidence for the correlation between X-ray and radio substructures, from which we estimate an upper limit for the inverse-Compton emission, and therefore set a lower limit on the magnetic field (450 kpc from PC centre) of B > 1.0 μG for a single power-law electron spectrum or B > 0.4 μG for a broken power-law electron spectrum. We propose a merger scenario including a PC, an SC, and a group. Our merger scenario accounts for the X-ray edges, diffuse radio features, and galaxy kinematics, as well as projection effects.

Original languageEnglish (US)
Pages (from-to)4704-4717
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume497
Issue number4
DOIs
StatePublished - Oct 1 2020

Bibliographical note

Funding Information:
This work was also supported at the University of Minnesota through the Chandra Award Number GO4-15119A with supplementary funding from the NSF grant AST17-14205. Basic research in radio astronomy at the Naval Research Laboratory is funded by 6.1 Base funding.

Publisher Copyright:
© 2020 The Author(s).

Keywords

  • X-rays: galaxies: clusters
  • galaxies: clusters: individual: Abell 2256
  • galaxies: clusters: intracluster medium

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