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Chandra Observations of the Spectacular A3411-12 Merger Event

  • Author(s): Andrade-Santos, F
  • Van Weeren, RJ
  • Di Gennaro, G
  • Wittman, D
  • Ryu, D
  • Lal, DV
  • Placco, VM
  • Fogarty, K
  • Jee, MJ
  • Stroe, A
  • Sobral, D
  • Forman, WR
  • Jones, C
  • Kraft, RP
  • Murray, SS
  • Brüggen, M
  • Kang, H
  • Santucci, R
  • Golovich, N
  • Dawson, W
  • et al.
Abstract

© 2019. The American Astronomical Society. All rights reserved.. We present deep Chandra observations of A3411-12, a remarkable merging cluster that hosts the most compelling evidence for electron reacceleration at cluster shocks to date. Using the YX-M scaling relation, we find r 500 ∼ 1.3 Mpc, M500 =(7.1 ± 0.7) × 1014 M⊙, kT =6.5 ± 0.1 keV, and a gas mass of Mg,500 =(9.7 ± 0.1) × 1013 M⊙. The gas mass fraction within r 500 is fg = 0.14 ± 0.01. We compute the shock strength using density jumps to conclude that the Mach number of the merging subcluster is small (M ≤ 1.15-0.09+0.14). We also present density, temperature, pseudo-pressure, and pseudo-entropy maps. Based on the pseudo-entropy map, we conclude that the cluster is undergoing a mild merger, consistent with the small Mach number. On the other hand, radio relics extend over Mpc scale in the A3411-12 system, which strongly suggests that a population of energetic electrons already existed over extended regions of the cluster.

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