Radio Observations of Supernovae

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dc.creatorPanagia, Nino
dc.creatorWeiler, Kurt W.
dc.creatorVan Dyk, Schuyler D.
dc.creatorSramek, Richard A.
dc.creatorStockdale, Christopher J.
dc.date2007-03-15
dc.date.accessioned2026-07-07T10:36:56Z
dc.date.available2026-07-07T10:36:56Z
dc.descriptionStudy of radio supernovae over the past 25 years includes two dozen detected objects and more than 100 upper limits. From this work it is possible to identify classes of radio properties, demonstrate conformance to and deviations from existing models, estimate the density and structure of the circumstellar material and, by inference, the evolution of the presupernova stellar wind. It is also possible to detect ionized hydrogen along the line of sight, to demonstrate binary properties of the stellar system, to detect clumpiness of the circumstellar material, and to put useful constraints on the progenitors of undetected Type Ia supernovae.
dc.description8 pages, 4 figures. Invited talk at `The Multicoloured Landscape of Compact Objects and their Explosive Origins', Cefalu', 2006 June 11-24 (AIP Conf. Proc.), eds. L. Burderi et al., in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0703411
dc.identifierhttp://arxiv.org/abs/astro-ph/0703411
dc.identifierAIPConf.Proc.924:407-414,2007
dc.identifierdoi:10.1063/1.2774888
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180221
dc.subjectAstrophysics
dc.titleRadio Observations of Supernovae
dc.typetext

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