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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2490
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dc.contributor.authorShanthi, K-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2008-06-23T11:38:36Z-
dc.date.available2008-06-23T11:38:36Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 445 - 448en
dc.identifier.urihttp://hdl.handle.net/2248/2490-
dc.description.abstractA 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.extent409530 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..445Sen
dc.subjectCosmic Gamma Ray Burstsen
dc.titleReclassification of gamma-ray bursts based on their brightness distributionsen
dc.typeArticleen
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