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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2105
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dc.contributor.authorMukerjee, K-
dc.contributor.authorAgrawal, P. C-
dc.contributor.authorPaul, B-
dc.contributor.authorRao, A. R-
dc.contributor.authorYadav, J. S-
dc.contributor.authorSeetha, S-
dc.contributor.authorKasturirangan, K-
dc.date.accessioned2008-03-03T08:11:47Z-
dc.date.available2008-03-03T08:11:47Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 293 - 294en
dc.identifier.urihttp://hdl.handle.net/2248/2105-
dc.description.abstractThe X-ray pulsars Cep X-4 and 4U 1907+09 were observed with the Indian X-ray Astronomy Experiment (IXAE). Observations of Cep-X4 were made during the declining phase of its latest 30 days outburst in 1997, July-August. The X-ray pulse profiles obtained during IXAE observations show inter-pulse dominated double-peak pulse. The second X-ray pulsar 4U 1907+09 with a period of 440s was observed in August 1996 and again in June 1998. The X-ray profile shows a double-peak pulse shape. The P obtained from these two observations indicate that the pulsar is in monotonically spin-down phase, at the rate of 0.23 s yr-1.en
dc.format.extent168375 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..293Men
dc.subjectX-ray pulsaren
dc.subjectIXAEen
dc.subjectProfileen
dc.titleStudy of two pulsars with the Indian X-ray Astronomy Experimenten
dc.typeArticleen
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