| dc.contributor.author | Barman, S. K | |
| dc.date.accessioned | 2007-10-31T08:57:31Z | |
| dc.date.available | 2007-10-31T08:57:31Z | |
| dc.date.issued | 1999 | |
| dc.identifier.citation | BASI, Vol. 27, No. 1, pp. 217 - 220 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/1939 | |
| dc.description.abstract | This 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.extent | 259026 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/1999BASI...27..217B | en |
| dc.subject | Binary | en |
| dc.subject | Grey atmosphere | en |
| dc.subject | Pure scattering | en |
| dc.subject | Linear polarization | en |
| dc.title | Linear polarization in binaries with grey atmosphere I. Conservative Rayleigh scattering | en |
| dc.type | Article | en |