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Extended radio emission in clusters of galaxies: recent Westerbork observations

  • E.A. Valentijn (a1) and H. van der Laan (a1)
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Whether galaxy clusters, in addition to a number of radio sources associated with individual cluster members, have an extended radio emitting region designated as cluster halo is in an interesting way related to several questions concerning cluster characteristics:

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References
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Breugel, W.J.M. van and Valentijn, E.A.: 1978, in preparation.
Bridle, A.H. and Fomalont, E.B.: 1976, “Astron. and Astrophys.” 52, 107.
Bridle, A.H., Fomalont, E.B., Miley, G.K.: 1978, in preparation.
Gisler, G.R. and Miley, G.K.: in preparation.
Jaffe, W.J., Perola, G.C. and Valentijn, E.A.: 1976, “Astron. and Astrophys.” 49, 179.
Miley, G.K. and Perola, G.C.: 1977, “Astron. and Astrophys.” in press.
Valentijn, E.A. and Perola, G.C.: 1977, “Astron. and Astrophys.” in press.
Valentijn, E.A., in preparation.
Vallée, J.P. and Wilson, A. S.: 1976, “Nature” 259, 451.
Vallée, J.P.: 1977, in press.
Wilson, A. S. and Vallée, J.P.: 1977, “Astron. and Astrophys.” 58, 79.
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0074-1809
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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