Volume 555, July 2013
|Number of page(s)||19|
|Section||Cosmology (including clusters of galaxies)|
|Published online||09 July 2013|
Leiden Observatory, Leiden University,
PO Box 9513
2 Harvard Smithsonian Center for Astrophysics (CfA – SAO), 60, Garden Street Cambridge, MA 02138, USA
3 Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, 7990 AA Dwingeloo, The Netherlands
4 Jansky Fellow of the National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA
5 National Radio Astronomy Observatory, Pete V. Domenici Science Operations Center, 1003 Lopezville Road, Socorro, NM 87801-0387, USA
6 Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany
7 Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany
Accepted: 29 April 2013
Context. Giant cluster radio relics are thought to form at shock fronts in the course of collisions between galaxy clusters. Via processes that are still poorly understood, these shocks accelerate or re-accelerate cosmic-ray electrons and might amplify magnetic fields. The best object to study this phenomenon is the galaxy cluster CIZA J2242.8+5301 as it shows the most undisturbed relic. By means of Giant Metrewave Radio Telescope (GMRT) and Westerbork Synthesis Radio Telescope (WSRT) data at seven frequencies spanning from 153 MHz to 2272 MHz, we study the synchrotron emission in this cluster.
Aims. We aim at distinguishing between theoretical injection and acceleration models proposed for the formation of radio relics. We also study the head-tail radio sources to reveal the interplay between the merger and the cluster galaxies.
Methods. We produced spectral index, curvature maps, and radio colour–colour plots and compared our data with predictions from models.
Results. We present one of the deepest 153 MHz maps of a cluster ever produced, reaching a noise level of 1.5 mJy beam-1. We derive integrated spectra for four relics in the cluster, discovering extremely steep spectrum diffuse emission concentrated in multiple patches. We find a possible radio phoenix embedded in the relic to the south of the cluster. The spectral index of the northern relic retains signs of steepening from the front towards the back of the shock also at the radio frequencies below 600 MHz. The spectral curvature in the same relic also increases in the downstream area. The data is consistent with the Komissarov-Gubanov injection models, meaning that the emission we observe is produced by a single burst of spectrally-aged accelerated radio electrons.
Key words: acceleration of particles / radio continuum: galaxies / galaxies: clusters: individual: CIZA J2242.8+530 / galaxies: clusters: intracluster medium / large-scale structure of Universe
Appendices are available in electronic form at http://www.aanda.org
Images as FITS files are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (220.127.116.11) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/555/A110
© ESO, 2013
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