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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/795
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dc.contributor.authorMisra, K-
dc.contributor.authorResmi, L-
dc.contributor.authorPandey, S. B-
dc.contributor.authorBhattacharya, D-
dc.contributor.authorSagar, R-
dc.date.accessioned2006-03-15T11:12:53Z-
dc.date.available2006-03-15T11:12:53Z-
dc.date.issued2005-12-
dc.identifier.citationBASI, Vol. 33, No. 4, pp. 487-497en
dc.identifier.urihttp://hdl.handle.net/2248/795-
dc.description.abstractWe present the CCD Cousins R band photometric observations of the afterglow of GRB 041006. The multiband afterglow evolution is modelled using an underlying `hard' electron energy spectrum with a p1 ~ 1.3. The burst appears to be of very low energy (E ~ 1048 ergs) concerned to a narrow cone of opening angle theta ~ 2.3o The associated supernova is compared with SN1998bw and is found to be brighteren
dc.format.extent211898 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectGamma-ray burstsen
dc.subjectGRB afterglowsen
dc.subjectflux decayen
dc.subjectspectral indexen
dc.titleOptical observations and multiband modelling of the afterglow of GRB041006 : Evidence of a hard electron energy spectrumen
dc.typeArticleen
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