Abstract
Distant powerful radio galaxies are useful tracers of galaxy groups and clusters, since through their very existence they point to gaseous atmospheres on scales of at least the radio source diameter. We present new results from XMM-Newton observations of three luminous radio galaxies, where evidence for both radiorelated and cluster mission is seen.
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Belsole, E., Worrall, D.M., Hardcastle, M.J. (2004). High Redshift Radio Galaxies as Tracers of Galaxy Clusters. XMM-Newton Observations. In: Plionis, M. (eds) Multiwavelength Cosmology. Astrophysics and Space Science Library, vol 301. Springer, Dordrecht. https://doi.org/10.1007/0-306-48570-2_31
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DOI: https://doi.org/10.1007/0-306-48570-2_31
Publisher Name: Springer, Dordrecht
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