Magnetic Fields in Galaxy Clusters

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dc.creatorGovoni, Federica
dc.creatorMurgia, Matteo
dc.date2003-11-17
dc.date.accessioned2026-07-07T02:11:13Z
dc.date.available2026-07-07T02:11:13Z
dc.descriptionMagnetic fields in galaxy clusters can be investigated using a variety of techniques. Recent studies including radio halos, Inverse Compton hard X-ray emissions and Faraday rotation measure, are briefly outlined. A numerical approach for investigating cluster magnetic fields strength and structure is presented. It consists of producing simulated rotation measure, radio halo images, and radio halo polarization, obtained from 3-dimensional multi-scale cluster magnetic field models, and comparing with observations.
dc.description5 pages, 2 Postscript figures. To be published by the Astronomical Society of the Pacific in Highlights of Astronomy, Vol 13, as part of the Proceedings of IAU JD10, Evolution in Galaxy Clusters: A Multiwavelength Approach
dc.identifierhttps://arxiv.org/abs/astro-ph/0311385
dc.identifierhttp://arxiv.org/abs/astro-ph/0311385
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7005
dc.subjectAstrophysics
dc.titleMagnetic Fields in Galaxy Clusters
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