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dc.contributor.authorWeiler, Kurt W.
dc.contributor.authorPanagia, Nino
dc.contributor.authorStockdale, Christopher
dc.contributor.authorRupen, Michael
dc.contributor.authorSramek, Richard A.
dc.contributor.authorWilliams, Christopher Leigh
dc.date.accessioned2015-02-25T20:40:43Z
dc.date.available2015-02-25T20:40:43Z
dc.date.issued2011-10
dc.date.submitted2011-05
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/1721.1/95632
dc.description.abstractWe present the results of detailed monitoring of the radio emission from the Type Ic supernova SN 1994I from three days after optical discovery on 1994 March 31 until eight years later at age 2927 days on 2002 April 5. The data were mainly obtained using the Very Large Array at the five wavelengths of λλ1.3, 2.0, 3.6, 6.2, and 21 cm and from the Cambridge 5 km Ryle Telescope at λ2.0 cm. Two additional measurements were obtained at millimeter wavelengths. This data set represents the most complete, multifrequency radio observations ever obtained for a Type Ib/c supernova. The radio emission evolves regularly in both time and frequency and is well described by established supernova emission/absorption models. It is the first radio supernova with sufficient data to show that it is clearly dominated by the effects of synchrotron self-absorption at early times.en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-637x/740/2/79en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Astronomical Societyen_US
dc.titleRADIO EMISSION FROM SN 1994I IN NGC 5194 (M 51): THE BEST-STUDIED TYPE Ib/c RADIO SUPERNOVAen_US
dc.typeArticleen_US
dc.identifier.citationWeiler, Kurt W., Nino Panagia, Christopher Stockdale, Michael Rupen, Richard A. Sramek, and Christopher L. Williams. “RADIO EMISSION FROM SN 1994I IN NGC 5194 (M 51): THE BEST-STUDIED TYPE Ib/c RADIO SUPERNOVA.” The Astrophysical Journal 740, no. 2 (October 3, 2011): 79. © 2011 The American Astronomical Societyen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorWilliams, Christopher Leighen_US
dc.relation.journalAstrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsWeiler, Kurt W.; Panagia, Nino; Stockdale, Christopher; Rupen, Michael; Sramek, Richard A.; Williams, Christopher L.en_US
dc.identifier.orcidhttps://orcid.org/0000-0001-7130-208X
mit.licensePUBLISHER_POLICYen_US


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