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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2281
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dc.contributor.authorSingh, N. S-
dc.contributor.authorSingh, K. Y-
dc.contributor.authorNaik, S-
dc.contributor.authorPaul, B-
dc.contributor.authorAgrawal, P. C-
dc.date.accessioned2008-05-09T08:15:40Z-
dc.date.available2008-05-09T08:15:40Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 351 - 354en
dc.identifier.urihttp://hdl.handle.net/2248/2281-
dc.description.abstractThe X-ray binary Cygnus X-3 was observed with the Indian X-ray Astronomy Experiment (IXAE) on Board the Indian Remote Sensing Satellite IRS-P3 during July 3-13, 1999 and October 11-24, 1999 with total useful exposure time of 31244.64 seconds in 1 sec integration mode. The short and long time variability of this X-ray source has been studied. We have found the orbital period to be 17254.273 ± 0.890 seconds.en
dc.format.extent323425 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..351Sen
dc.subjectCygnus X-3en
dc.subjectBinary systemen
dc.subjectOrbital perioden
dc.subjectLight curveen
dc.subjectCross-correlationen
dc.titleObservation of X-ray binary Cygnus X-3 by Indian X-ray Astronomy Experimenten
dc.typeArticleen
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