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 |