Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. VLA Radio Observations of the HST Frontier Fields Cluster Abell 2744: The Discovery of New Radio Relics
 

VLA Radio Observations of the HST Frontier Fields Cluster Abell 2744: The Discovery of New Radio Relics

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2017
Author(s)
Pearce, C. J. J.
•
van Weeren, R. J.
•
Andrade-Santos, F.
•
Jones, C.
•
Forman, W. R.
•
Brüggen, M.
•
Bulbul, E.
•
Clarke, T. E.
•
Kraft, R. P.
•
Medezinski, E.
•
Mroczkowski, T.
•
NONINO, Mario  
•
Nulsen, P. E. J.
•
Randall, S. W.
•
Umetsu, K.
DOI
10.3847/1538-4357/aa7e2f
Description
M.N. acknowledges PRIN-INAF 2014 1.05.01.94.02
Abstract
Cluster mergers leave distinct signatures in the intracluster medium (ICM) in the form of shocks and diffuse cluster radio sources that provide evidence for the acceleration of relativistic particles. However, the physics of particle acceleration in the ICM is still not fully understood. Here we present new 1-4 GHz Jansky Very Large Array (VLA) and archival Chandra observations of the HST Frontier Fields Cluster Abell 2744. In our new VLA images, we detect the previously known ∼2.1 Mpc radio halo and ∼1.5 Mpc radio relic. We carry out a radio spectral analysis from which we determine the relic’s injection spectral index to be {α }{inj}=-1.12+/- 0.19. This corresponds to a shock Mach number of { M }={2.05}-0.19+0.31 under the assumption of diffusive shock acceleration. We also find evidence for spectral steepening in the post-shock region. We do not find evidence for a significant correlation between the radio halo’s spectral index and ICM temperature. In addition, we observe three new polarized diffuse sources and determine two of these to be newly discovered giant radio relics. These two relics are located in the southeastern and northwestern outskirts of the cluster. The corresponding integrated spectral indices measure -1.81 ± 0.26 and -0.63 ± 0.21 for the SE and NW relics, respectively. From an X-ray surface brightness profile we also detect a possible density jump of R={1.39}-0.22+0.34 co-located with the newly discovered SE relic. This density jump would correspond to a shock front Mach number of { M }={1.26}-0.15+0.25.
Volume
845
Issue
1
Start page
81
Uri
http://hdl.handle.net/20.500.12386/26775
Url
https://iopscience.iop.org/article/10.3847/1538-4357/aa7e2f
Issn Identifier
0004-637X
Ads BibCode
2017ApJ...845...81P
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

Pearce_2017_ApJ_845_81.pdf

Description
PDF editoriale
Size

6.26 MB

Format

Adobe PDF

Checksum (MD5)

85e6c2dfe80b2b44971f5bc938be3c06

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback