Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1439
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dc.contributor.authorBarman, S. K-
dc.contributor.authorPeraiah, A-
dc.date.accessioned2007-03-14T10:02:56Z-
dc.date.available2007-03-14T10:02:56Z-
dc.date.issued1991-
dc.identifier.citationBASI, Vol. 19, No. 1&2, pp. 37-46en
dc.identifier.urihttp://hdl.handle.net/2248/1439-
dc.description.abstractTheoretical models are computed for estimating linear polarization from the extended dusty outer layers of the components of a close binary system whose surfaces are distorted by rotation and mutual tidal effects. Plane-parallel layers of the dusty atmospheres of the components are assumed. A wavelength-dependent scattering coefficient and a Rayleigh phase function is used in solving the equation of radiative transfer. Polarization increases with decreasing wavelength and increasing particle size. Polarization for uniform rotation is larger than that for nonuniform rotation. Polarization for single stars is always less than that for a binary component, dependent on the position of the observeren
dc.format.extent629413 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectPolarizationen
dc.subjectRadiative transferen
dc.titlePolarization in binariesen
dc.typeArticleen
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