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    Spectral and morphological signatures of cluster merger shocks: CIZA J2242.8+5301

    Access Status
    Open access via publisher
    Authors
    Stroe, Andra
    Weeren, Reinout J van
    Sobral, David
    Rumsey, Clare
    Intema, Huib
    Röttgering, Huub JA
    Harwood, Jeremy J
    Saunders, Richard
    Brüggen, Marcus
    Hoeft, Matthias
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Stroe, A. and Weeren, R.J.V. and Sobral, D. and Rumsey, C. and Intema, H.T. and Röttgering, H.J.A. and Harwood, J.J. et al. 2014. Spectral and morphological signatures of cluster merger shocks: CIZA J2242.8+5301. Astronomical Society of India Conference Series. BASI. 13 (1): pp. 201-204.
    Additional URLs
    https://astron-soc.in/bulletin/asics_vol013/
    Faculty
    Faculty of Science and Engineering
    School
    School of Electrical Engineering, Computing and Mathematical Sciences (EECMS)
    URI
    http://hdl.handle.net/20.500.11937/76025
    Collection
    • Curtin Research Publications
    Abstract

    The CIZA J2242.8+5301 cluster hosts an extraordinary, narrow, Mpc-wide, diffuse patch of radio emission tracing travelling shock waves, called a relic. We perform a multi-wavelength of observations of the cluster. We discover radio spectral steepening and increasing spectral curvature in the shock downstream area, indicative of emission produced by spectrally-aged electrons, following a JP ageing model. The curved integrated spectrum towards $16$ GHz challenges the favoured relic formation model. Further, we find a boosting the number density of H$\alpha$ emitters by a factor of $10$, possibly caused by interactions of the galaxies with the shock wave.

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