Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6557
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dc.contributor.authorYadav, N-
dc.contributor.authorRay, A-
dc.contributor.authorChakraborti, S-
dc.contributor.authorStockdale, C-
dc.contributor.authorChandra, P-
dc.contributor.authorSmith, R-
dc.contributor.authorRoy, R-
dc.contributor.authorDwarkadas, V-
dc.contributor.authorSutaria, F. K-
dc.contributor.authorPooley, D-
dc.contributor.authorKumar, B-
dc.contributor.authorBose, S-
dc.date.accessioned2014-03-12T09:47:45Z-
dc.date.available2014-03-12T09:47:45Z-
dc.date.issued2014-01-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 296, pp. 112-115en
dc.identifier.isbn978-1-107-04477-7-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/2248/6557-
dc.descriptionRestricted Accessen
dc.description.abstractSN 2012AW is a type-IIP supernova which exploded in M95. In this paper we discuss the radio observations of this supernova and model them to determine the important parameters relevant to the explosion and the evolution of blast wave. We also determine the dominant cooling process important to this source.en
dc.language.isoenen
dc.publisherCambridge University Pressen
dc.relation.ispartofseriesInternational Astronomical Union Symposium;296-
dc.relation.urihttp://dx.doi.org/10.1017/S1743921313009320en
dc.rights© International Astronomical Unionen
dc.subjectRadio continuum: generalen
dc.subjectSupernovae: individual (SN 2012aw)en
dc.subjectMethods: data analysisen
dc.subjectTechniques: image processingen
dc.subjectInterferometricen
dc.titleRadio observations of a nearby type IIP SN 2012awen
dc.typeArticleen
Appears in Collections:IIAP Publications

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