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Diffuse Cluster Radio Sources

  • Conference paper
Book cover Extragalactic Radio Sources

Part of the book series: International Astronomical Union ((IAUS,volume 175))

Abstract

Diffuse radio sources in clusters remain a poorly understood phenomenon. They are very extended sources (0.4-0.6 Mpc), of low surface brightness and steep spectrum, which cannot be identified with any active radio galaxy. They are a rare phenomenon, as they have been found so far in few clusters of galaxies. This paper reviews the current findings about this kind of sources, and the suggestions about their formation and evolution.

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Author information

Authors and Affiliations

  1. Istituto di Radioastronomia, CNR, Bologna, Italy

    L. Feretti

  2. Dipartimento di Astronomia dell’Università, Bologna, Italy

    G. Giovannini

Authors
  1. L. Feretti
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  2. G. Giovannini
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Editor information

Editors and Affiliations

  1. Australia Telescope, CSIRO, Epping, Australia

    R. Ekers

  2. Istituto di Radioastronomia, CNR, Bologna, Italy

    C. Fanti  & L. Padrielli  & 

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© 1996 International Astronomical Union

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Feretti, L., Giovannini, G. (1996). Diffuse Cluster Radio Sources. In: Ekers, R., Fanti, C., Padrielli, L. (eds) Extragalactic Radio Sources. International Astronomical Union, vol 175. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0295-4_120

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  • DOI: https://doi.org/10.1007/978-94-009-0295-4_120

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-4122-2

  • Online ISBN: 978-94-009-0295-4

  • eBook Packages: Springer Book Archive

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