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Title: Method of description and the properties of the Fourier components of periodically variable linear polarization

Journal Article · · Sov. Astron. (Engl. Transl.); (United States)
OSTI ID:6591133

When interpreting observations of variable polarization of the emission of binary stars and other objects the problem arises of comparing the observed and calculated polarization curves. A description of the shape of the polarization phase curve in the (Q x U) plane independent of the choice of the zero-point of the polarization position angle is proposed for periodically variable, linearly polarized radiation on the basis of the expansion of the Stokes parameters Q and U in Fourier series. In the (Q x U) plane each Fourier component of the Stokes parameters Q and U consists of an ellipse characterized by four geometrical parameters. Several examples of the description of calculated curves of polarization of the optical emission of binary x-ray systems are given for cases when the scattering takes place in optically thick media: for scattering of the light of a tidally deformed star in its atmosphere and of the light of a star of an accretion disk, both for one lying in the orbital plane and an inclined and precessing disk. Certain properties of the polarization phase curves in the (Q x U) plane resulting from the symmetry properties of rotating systems are pointed out.

Research Organization:
Astronomical Council, USSR Academy of Sciences
OSTI ID:
6591133
Journal Information:
Sov. Astron. (Engl. Transl.); (United States), Vol. 27:5
Country of Publication:
United States
Language:
English