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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2282
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dc.contributor.authorManchanda, R. K-
dc.date.accessioned2008-05-09T08:24:57Z-
dc.date.available2008-05-09T08:24:57Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 355 - 360en
dc.identifier.urihttp://hdl.handle.net/2248/2282-
dc.description.abstractHard X-ray observations of the binary X-ray pulsars were made using a balloon-borne large area scintillation counter telescope in the 20-200 keV band. Apart from many other galactic and extragalactic X-ray sources, three X-ray pulsars namely Her X-1, GS 1843+00 and 4U 1907+09 were tracked during two flights launched in March 1997 and Nov. 1998. The observations of the transient sources GS 1843+00 correspond to near intensity maximum in its burst phase. We discuss the morphology of the pulse profiles in terms of geometrical constraints and the X-ray emission mechanism.en
dc.format.extent554132 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..355Men
dc.subjectBinary systemsen
dc.subjectX-ray pulsarsen
dc.titlePulse profiles of binary X-ray pulsars in 20-200 keV banden
dc.typeArticleen
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