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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1927
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dc.contributor.authorYadav, J. S-
dc.contributor.authorAgrawal, P. C-
dc.contributor.authorPaul, B-
dc.contributor.authorRao, A. R-
dc.contributor.authorVahia, M. N-
dc.contributor.authorSeetha, S-
dc.contributor.authorKasturirangan, K-
dc.date.accessioned2007-10-27T11:00:37Z-
dc.date.available2007-10-27T11:00:37Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 177 - 179en
dc.identifier.urihttp://hdl.handle.net/2248/1927-
dc.description.abstractThe light curves of the galactic superluminal X-ray transient source GRS1915+105 observed with the pointed proportional counters (PPC) of Indian X-ray Astronomy Experiment (IXAE)on board IRS-P3 have revealed the presence of four types of intense X-ray bursts : regular persistent bursts, quasi-regular bursts and irregular bursts. Two of the four types of bursts are regular in occurrence and persist over extended durations. All the observed bursts have a slow exponential rise and a sharp linear decay. The regular bursts show two peak structure while the other type of bursts show multi-peak structure. The burst spectrum is hardest at the end of the decay.en
dc.format.extent252152 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..177Yen
dc.subjectX-ray burstsen
dc.subjectIndian S-ray Astronomy Experiment (IXAE)en
dc.titleX-ray bursts from GRS 1915+105 observed with IXAEen
dc.typeArticleen
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