X-ray orbital modulations in low-mass X-ray binaries

dc.contributor.author	Pandey, U. S
dc.date.accessioned	2007-03-14T06:23:11Z
dc.date.available	2007-03-14T06:23:11Z
dc.date.issued	1990
dc.identifier.citation	BASI, Vol. 18, pp. 211-214	en
dc.identifier.uri	http://hdl.handle.net/2248/1415
dc.description.abstract	It is suggested that structure in the outer parts of the accretion disk of low-mass X-ray binaries may be due to tidal action of the secondary which is overflowing its Roche lobe. These structures at various phases may result from inhomogeneous tidal forces to which the matter in the outer parts of the disk is subjected	en
dc.format.extent	122149 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Stellar orbits	en
dc.subject	X-ray binaries	en
dc.title	X-ray orbital modulations in low-mass X-ray binaries	en
dc.type	Article	en