Light Curves of Radio Supernovae

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dc.creatorKelley, Matthew T.
dc.creatorStockdale, Christopher J.
dc.creatorWeiler, Kurt W.
dc.creatorWilliams, Christopher L. M.
dc.creatorPanagia, Nino
dc.creatorSramek, Richard A.
dc.creatorMarcaide, J. M.
dc.creatorVan Dyk, Schuyler D.
dc.date2007-08-08
dc.date.accessioned2026-07-07T10:57:04Z
dc.date.available2026-07-07T10:57:04Z
dc.descriptionWe present the results from the on-going radio monitoring of recent type II supernovae (SNe), including SNe 2004et, 2004dj, 2002hh, 2001em, and 2001gd. Using the Very Large Array to monitor these supernovae, we present their radio light-curves. From these data we are able to discuss parameterizations and modeling and make predictions of the nature of the progenitors based on previous research. Derived mass loss rates assume wind-established circumstellar medium, shock velocity ~10,000 km/s, wind velocity ~10 km/s, and CSM Temperature ~10,000 K.
dc.description3 pages, 6 figures Conference Proceedings: "Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters" AIP, New York, eds. S. Immler, K.W. Weiler, and R. McCray
dc.identifierhttps://arxiv.org/abs/0708.1180
dc.identifierhttp://arxiv.org/abs/0708.1180
dc.identifierAIPConf.Proc.937:269-271,2007
dc.identifierdoi:10.1063/1.2803574
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186627
dc.subjectAstrophysics
dc.titleLight Curves of Radio Supernovae
dc.typetext

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