Theoretical Implications of Diffuse Non-Thermal Emission from Clusters of Galaxies

Simple item page
dc.creatorEnsslin, Torsten A.
dc.date2000-01-25
dc.date.accessioned2026-07-07T01:51:53Z
dc.date.available2026-07-07T01:51:53Z
dc.descriptionA short review on theoretical implications of non-thermal emission (radio, extreme ultraviolet, high energy X-ray) from the intra-cluster medium is given. The origin of cluster radio halos and cluster radio relics is discussed within the framework of a network of processes producing a non-thermal electron population. Emphasis is given to the role of old, remnant, presently invisible relativistic plasma released by former radio galaxies.
dc.description8 pages, 2 figures, LaTeX, uses newpasp.sty, invited talk at IAU 199 `The Universe at Low Radio Frequencies' in Pune, India, 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/0001433
dc.identifierhttp://arxiv.org/abs/astro-ph/0001433
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/444
dc.subjectAstrophysics
dc.titleTheoretical Implications of Diffuse Non-Thermal Emission from Clusters of Galaxies
dc.typetext

Files

Collections

arXiv