FRONTIER FIELDS CLUSTERS: DEEP CHANDRA OBSERVATIONS OF THE COMPLEX MERGER MACS J1149.6+2223

G.A. Ogrean, R.J. Van Weeren, C. Jones, W. Forman, W.A. Dawson, N. Golovich, F. Andrade-Santos, S.S. Murray, Paul Nulsen, E. Roediger, A. Zitrin, E. Bulbul, R. Kraft, A. Goulding, K. Umetsu, T. Mroczkowski, A. Bonafede, S. Randall, J. Sayers, E. ChurazovL. David, J. Merten, M. Donahue, B. Mason, P. Rosati, A. Vikhlinin, H. Ebeling

Research output: Contribution to journalArticle

15 Citations (Scopus)

Abstract

© 2016. The American Astronomical Society. All rights reserved. The Hubble Space Telescope Frontier Fields cluster MACS J1149.6+2223 is one of the most complex merging clusters, believed to consist of four dark matter halos. We present results from deep (365 ks) Chandra observations of the cluster, which reveal the most distant cold front (z = 0.544) discovered to date. In the cluster outskirts, we also detect hints of a surface brightness edge that could be the bow shock preceding the cold front. The substructure analysis of the cluster identified several components with large relative radial velocities, thus indicating that at least some collisions occur almost along the line of sight. The inclination of the mergers with respect to the plane of the sky poses significant observational challenges at X-ray wavelengths. MACS J1149.6+2223 possibly hosts a steep-spectrum radio halo. If the steepness of the radio halo is confirmed, then the radio spectrum, combined with the relatively regular ICM morphology, could indicate that MACS J1149.6+2223 is an old merging cluster.
Original languageEnglish
JournalThe Astrophysical Journal
Volume819
Issue number2
DOIs
Publication statusPublished - 2016

Fingerprint Dive into the research topics of 'FRONTIER FIELDS CLUSTERS: DEEP CHANDRA OBSERVATIONS OF THE COMPLEX MERGER MACS J1149.6+2223'. Together they form a unique fingerprint.

Cite this