Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4921
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dc.contributor.authorAgrawal, P.C.-
dc.contributor.authorMukerjee, K.-
dc.contributor.authorNaik, S.-
dc.contributor.authorPaul, Biswajit-
dc.contributor.authorRao, A.R.-
dc.contributor.authorYadav, J.S.-
dc.contributor.authorKasturirangan, K.-
dc.contributor.authorSeetha, S.-
dc.contributor.authorSingh, K.Y.-
dc.date.accessioned2012-07-14T10:11:08Z-
dc.date.available2012-07-14T10:11:08Z-
dc.date.issued2000-
dc.identifier.citationAdvances in Space Research, 2000, Vol. 25, p357en
dc.identifier.issn0273-1177-
dc.identifier.urihttp://hdl.handle.net/2289/4921-
dc.descriptionRestricted Accessen
dc.description.abstractStudies of several x-ray binaries have been made with the Indian X-ray Astronomy Experiment on the IRS-P3 satellite. We present here results from timing analysis of four of the neutron star and black hole binaries; namely GRS 1915+105, the recently discovered x-ray transient XTE 51748-288 and the x-ray pulsars Cep X-4 and 4U1907+09. New results include detection of a variety of regular and irregular bursts from GRS 1915+105 and detection of irregular intensity variations in the transient source XTE 51748-288. The x-ray pulse profile of 4U1907+09 was found to have changed from a double-peak pulse observed in August 4-7, 1996 to a broad single-peak pulse in May 26 - June 3, 1998 period. Details of these results are presented.en
dc.language.isoenen
dc.publisherElsevier B.V.en
dc.rights2000 Elsevier B.V.en
dc.titleStudies of binary sources with the Indian X-Ray Astronomy Experimenten
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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