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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1415
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dc.contributor.authorPandey, U. S-
dc.date.accessioned2007-03-14T06:23:11Z-
dc.date.available2007-03-14T06:23:11Z-
dc.date.issued1990-
dc.identifier.citationBASI, Vol. 18, pp. 211-214en
dc.identifier.urihttp://hdl.handle.net/2248/1415-
dc.description.abstractIt 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 subjecteden
dc.format.extent122149 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectStellar orbitsen
dc.subjectX-ray binariesen
dc.titleX-ray orbital modulations in low-mass X-ray binariesen
dc.typeArticleen
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