High-resolution radio imaging of young supernovae

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dc.creatorPerez-Torres, M. A.
dc.creatorMarcaide, J. M.
dc.creatorAlberdi, A.
dc.creatorRos, E.
dc.creatorGuirado, J. C.
dc.creatorLara, L.
dc.creatorMantovani, F.
dc.creatorStockdale, C. J.
dc.creatorWeiler, K. W.
dc.creatorDiamond, P. J.
dc.creatorVan Dyk, S. D.
dc.creatorLundqvist, P.
dc.creatorPanagia, N.
dc.creatorShapiro, I. I.
dc.creatorSramek, R.
dc.date2004-03-11
dc.date2004-03-12
dc.date.accessioned2026-07-07T02:12:36Z
dc.date.available2026-07-07T02:12:36Z
dc.descriptionThe high resolution obtained through the use of VLBI gives an unique opportunity to directly observe the interaction of an expanding radio supernova with its surrounding medium. We present here results from our VLBI observations of the young supernovae SN 1979C, SN 1986J, and SN 2001gd.
dc.description8 pages, 3 figures. Uses svmult.cls. To appear in proceedings of IAU Colloquium 192 "Supernovae (10 years of SN 1993J)", April 2003, Valencia, Spain, eds. J. M. Marcaide and K. W. Weiler
dc.identifierhttps://arxiv.org/abs/astro-ph/0403273
dc.identifierhttp://arxiv.org/abs/astro-ph/0403273
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7505
dc.subjectAstrophysics
dc.titleHigh-resolution radio imaging of young supernovae
dc.typetext

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