A shock front at the radio relic of Abell 2744

D. Eckert*, M. Jauzac, F. Vazza, M. S. Owers, J. P. Kneib, C. Tchernin, H. Intema, K. Knowles

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    56 Citations (Scopus)

    Abstract

    Radio relics are Mpc-scale diffuse radio sources at the peripheries of galaxy clusters which are thought to trace outgoing merger shocks. We present XMM-Newton and Suzaku observations of the galaxy cluster Abell 2744 (z = 0.306), which reveal the presence of a shock front 1.5 Mpc east of the cluster core. The surface-brightness jump coincides with the position of a known radio relic. Although the surface-brightness jump indicates a weak shock with a Mach number M=1.7-0.3+0.5, the plasma in the post-shock region has been heated to a very high temperature (~13 keV) by the passage of the shock wave. The low-acceleration efficiency expected from such a weak shock suggests that mildly relativistic electrons have been re-accelerated by the passage of the shock front.

    Original languageEnglish
    Pages (from-to)1302-1307
    Number of pages6
    JournalMonthly Notices of the Royal Astronomical Society
    Volume461
    Issue number2
    DOIs
    Publication statusPublished - 11 Sept 2016

    Keywords

    • Galaxies: clusters: individual: A2744
    • X-rays: galaxies: clusters

    Fingerprint

    Dive into the research topics of 'A shock front at the radio relic of Abell 2744'. Together they form a unique fingerprint.

    Cite this