Radio observations of a nearby type IIP SN 2012aw

Yadav, N; Ray, A; Chakraborti, S; Stockdale, C; Chandra, P; Smith, R; Roy, R; Dwarkadas, V; Sutaria, F. K; Pooley, D; Kumar, B; Bose, S

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dc.contributor.author	Yadav, N
dc.contributor.author	Ray, A
dc.contributor.author	Chakraborti, S
dc.contributor.author	Stockdale, C
dc.contributor.author	Chandra, P
dc.contributor.author	Smith, R
dc.contributor.author	Roy, R
dc.contributor.author	Dwarkadas, V
dc.contributor.author	Sutaria, F. K
dc.contributor.author	Pooley, D
dc.contributor.author	Kumar, B
dc.contributor.author	Bose, S
dc.date.accessioned	2014-03-12T09:47:45Z
dc.date.available	2014-03-12T09:47:45Z
dc.date.issued	2014-01
dc.identifier.citation	Proceedings of the International Astronomical Union, Vol. 296, pp. 112-115	en
dc.identifier.isbn	978-1-107-04477-7
dc.identifier.issn	1743-9213
dc.identifier.uri	http://hdl.handle.net/2248/6557
dc.description	Restricted Access	en
dc.description.abstract	SN 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.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.ispartofseries	International Astronomical Union Symposium;296
dc.relation.uri	http://dx.doi.org/10.1017/S1743921313009320	en
dc.rights	© International Astronomical Union	en
dc.subject	Radio continuum: general	en
dc.subject	Supernovae: individual (SN 2012aw)	en
dc.subject	Methods: data analysis	en
dc.subject	Techniques: image processing	en
dc.subject	Interferometric	en
dc.title	Radio observations of a nearby type IIP SN 2012aw	en
dc.type	Article	en