1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1939
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBarman, S. K-
dc.date.accessioned2007-10-31T08:57:31Z-
dc.date.available2007-10-31T08:57:31Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 217 - 220en
dc.identifier.urihttp://hdl.handle.net/2248/1939-
dc.description.abstractThis paper presents a method for calculating linear polarization from binaries whose surfaces are distorted due to tidal and rotational forces. The atmospheres in stars are grey, plane-parallel and pure scattering. The polarization as high as 3.51% is calculated for a single star and 2.89% for a binary with a mass ration q=0.3. The method has been applied to some early type binaries to calculate polarizations in them.en
dc.format.extent259026 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..217Ben
dc.subjectBinaryen
dc.subjectGrey atmosphereen
dc.subjectPure scatteringen
dc.subjectLinear polarizationen
dc.titleLinear polarization in binaries with grey atmosphere I. Conservative Rayleigh scatteringen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
barman.pdf252.96 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.