Observation of X-ray binary Cygnus X-3 by Indian X-ray Astronomy Experiment

dc.contributor.author	Singh, N. S
dc.contributor.author	Singh, K. Y
dc.contributor.author	Naik, S
dc.contributor.author	Paul, B
dc.contributor.author	Agrawal, P. C
dc.date.accessioned	2008-05-09T08:15:40Z
dc.date.available	2008-05-09T08:15:40Z
dc.date.issued	2001
dc.identifier.citation	BASI, Vol. 29, No. 3, pp. 351 - 354	en
dc.identifier.uri	http://hdl.handle.net/2248/2281
dc.description.abstract	The 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.extent	323425 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2001BASI...29..351S	en
dc.subject	Cygnus X-3	en
dc.subject	Binary system	en
dc.subject	Orbital period	en
dc.subject	Light curve	en
dc.subject	Cross-correlation	en
dc.title	Observation of X-ray binary Cygnus X-3 by Indian X-ray Astronomy Experiment	en
dc.type	Article	en