Optical observations and multiband modelling of the

dc.contributor.author	Misra, K.
dc.contributor.author	Resmi, L.
dc.contributor.author	Pandey, S. B.
dc.contributor.author	Bhattacharya, D.
dc.contributor.author	Sagar, R.
dc.date.accessioned	2009-10-27T04:36:36Z
dc.date.available	2009-10-27T04:36:36Z
dc.date.issued	2005-12
dc.identifier.uri	http://hdl.handle.net/123456789/321
dc.description.abstract	We 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) confined to a narrow cone of opening angle ϴ ~ 2.3̊. The associated supernova is compared with SN1998bw and is found to be brighter.	en_US
dc.language.iso	en	en_US
dc.publisher	Optical observations and multiband modelling of the	en_US
dc.relation.ispartofseries	basi33-487
dc.subject	Gamma-Ray Bursts, GRB afterglows, Spectral Index	en_US
dc.title	Optical observations and multiband modelling of the	en_US
dc.type	Article	en_US