Diffuse Cluster-wide Radio Halos

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dc.creatorLiang, Haida
dc.date2000-12-07
dc.date.accessioned2026-07-07T01:56:55Z
dc.date.available2026-07-07T01:56:55Z
dc.descriptionWe will discuss the properties and origins of halos and relics including estimates of the cluster magnetic fields, and present results for a few recently discovered halos and relics. The electrons in the suprathermal high energy tail of the thermal gas distribution are likely to provide the seed particles for acceleration through mergers and turbulences to relativistic energies. These relativistic particles are then responsible for the synchrotron emission of the halos.
dc.description3 pages, 2 postscript figures, use newpasp.sty; invited talk, 24th meeting at the IAU, Joint Discussion 10 on `Cluster Mergers and their Connection to Radio sources', Auguest 2000, Manchester, England, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0012166
dc.identifierhttp://arxiv.org/abs/astro-ph/0012166
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2181
dc.subjectAstrophysics
dc.titleDiffuse Cluster-wide Radio Halos
dc.typetext

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