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Title: Chandra and JVLA Observations of HST Frontier Fields Cluster MACS J0717.5+3745

Journal Article · · The Astrophysical Journal (Online)
ORCiD logo [1]; ORCiD logo [2];  [1]; ORCiD logo [1];  [1];  [3];  [4];  [4]; ORCiD logo [5]; ORCiD logo [6];  [7];  [1];  [8]; ORCiD logo [9];  [10];  [1];  [11];  [12]; ORCiD logo [13]; ORCiD logo [14] more »;  [15];  [16]; ORCiD logo [1];  [17]; ORCiD logo [18]; ORCiD logo [1]; ORCiD logo [17] « less
  1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  2. Stanford Univ., CA (United States). Dept. of Physics
  3. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Univ. of Southampton (United Kingdom). Dept. of Physics and Astronomy
  4. Univ. of Hamburg (Germany). Hamburger Sternwarte
  5. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Kavli Inst. for Astrophysics and Space Research
  6. Naval Research Lab. (NRL), Washington, DC (United States)
  7. Max Planck Inst. for Astrophysics, Garching (Germany); Space Research Inst., Moscow (Russia)
  8. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  9. Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy
  10. Princeton Univ., NJ (United States). Dept. of Astrophysical Sciences
  11. National Radio Astronomy Observatory, Charlottesville, VA (United States)
  12. Univ. of Oxford (United Kingdom). Dept. of Physics
  13. European Organization for Astronomical Research in the Southern Hemisphere (ESO), Munchen (Germany)
  14. Harvard-Smithsonian Center for Astrophysics, Crawley WA (United States). International Centre for Radio Astronomy Research (ICRAR)
  15. Univ. degli Studi di Ferrara (Italy). Dipartimento di Fisica e Scienze della Terra
  16. Univ. of Hull, Cottinton Road, Hall (United States)
  17. California Inst. of Technology (CalTech), Pasadena, CA (United States). Cahill Center for Astronomy and Astrophysics
  18. Academia Sinica, Taipei (Taiwan). Inst. of Astronomy and Astrophysics

To investigate the relationship between thermal and non-thermal components in merger galaxy clusters, we present deep JVLA and Chandra observations of the HST Frontier Fields cluster MACS J0717.5+3745. The Chandra image shows a complex merger event, with at least four components belonging to different merging subclusters. Northwest of the cluster, ~0.7 Mpc from the center, there is a ram-pressure-stripped core that appears to have traversed the densest parts of the cluster after entering the intracluster medium (ICM) from the direction of a galaxy filament to the southeast. Here, we detect a density discontinuity north-northeast of this core, which we speculate is associated with a cold front. Our radio images reveal new details for the complex radio relic and radio halo in this cluster. In addition, we discover several new filamentary radio sources with sizes of 100–300 kpc. A few of these seem to be connected to the main radio relic, while others are either embedded within the radio halo or projected onto it. A narrow-angled-tailed (NAT) radio galaxy, a cluster member, is located at the center of the radio relic. The steep spectrum tails of this active galactic nucleus lead into the large radio relic where the radio spectrum flattens again. This morphological connection between the NAT radio galaxy and relic provides evidence for re-acceleration (revival) of fossil electrons. The presence of hot ≳20 keV ICM gas detected by Chandra near the relic location provides additional support for this re-acceleration scenario.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
Sponsoring Organization:
National Aeronautic and Space Administration (NASA); USDOE
Grant/Contract Number:
AC52-07NA27344
OSTI ID:
1431004
Report Number(s):
LLNL-JRNL--748246
Journal Information:
The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 835; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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$Suzaku$ X-ray study of the double radio relic galaxy cluster CIZA J2242.8+5301 text January 2015
Strong-Lensing Analysis of MACS,J0717.5+3745 from Hubble Frontier Fields observations: How well can the mass distribution be constrained? text January 2015
LOFAR, VLA, and Chandra observations of the Toothbrush galaxy cluster text January 2016
A shock front at the radio relic of Abell 2744 text January 2016
Constraining the efficiency of cosmic ray acceleration by cluster shocks text January 2016
The Case for Electron Re-Acceleration at Galaxy Cluster Shocks text January 2017
Collisional Plasma Models with APEC/APED: Emission Line Diagnostics of Hydrogen-like and Helium-like Ions text January 2001
A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E0657-56 text January 2001
The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton text January 2003
The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections text January 2005
ASMOOTH: A simple and efficient algorithm for adaptive kernel smoothing of two-dimensional imaging data text January 2006
Giant Ringlike Radio Structures Around Galaxy Cluster Abell 3376 text January 2006
Shocks and cold fronts in galaxy clusters text January 2007
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