Reclassification of gamma-ray bursts based on their brightness distributions

dc.contributor.author	Shanthi, K
dc.contributor.author	Bhat, C. L
dc.date.accessioned	2008-06-23T11:38:36Z
dc.date.available	2008-06-23T11:38:36Z
dc.date.issued	2002
dc.identifier.citation	BASI, Vol. 30, No. 1, pp. 445 - 448	en
dc.identifier.uri	http://hdl.handle.net/2248/2490
dc.description.abstract	A reclassification of the cosmic gamma-ray bursts has been done into two distinct classes on the basis of their brightness distributions. While one (majority) class is found to be compatible with a homogeneous and monoluminosity source population with simple cosmological effects folded into the brightness distribution function, the other, smaller population is not consistent with such a scenario and may need a consideration of source evolutionary effects.	en
dc.format.extent	409530 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002BASI...30..445S	en
dc.subject	Cosmic Gamma Ray Bursts	en
dc.title	Reclassification of gamma-ray bursts based on their brightness distributions	en
dc.type	Article	en