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Reclassification of gamma-ray bursts based on their brightness distributions

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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


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