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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2125
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dc.contributor.authorGupta, V-
dc.contributor.authorGupta, P. D-
dc.contributor.authorBhat, P. N-
dc.date.accessioned2008-03-05T11:14:26Z-
dc.date.available2008-03-05T11:14:26Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 371 - 373en
dc.identifier.urihttp://hdl.handle.net/2248/2125-
dc.description.abstractIn this paper, we study a sample of short duration bursts contained in the 3B BATSE catalogue. We fit the time profiles of these GRBs with lognormal functions and study various temporal properties of these objects. In most of the mutipeaked bursts, we find that the temporal asymmetry of individual pulses evolves with time i.e. subsequent pulses tend to be more symmetric.en
dc.format.extent230529 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..371Gen
dc.subjectGRBsen
dc.subjectLognormal functionsen
dc.subjectRise and decay timesen
dc.titleMorphological properties of short duration Gamma Ray Burstsen
dc.typeArticleen
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