Circular polarization through accretion by a star with a strong magnetic field

Details Circular polarization through accretion by a star with a strong magnetic field Circular polarization through accretion by a star with a strong magnetic field

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sval....1..189g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 1, Sept. 1975, p. 34-39.) Soviet Astronomy Letters, vol. 1, Sept.-Oct. 1975, p. 189-191

Astronomy and Astrophysics

Astronomy

Binary Stars, Circular Polarization, Stellar Magnetic Fields, Stellar Rotation, Field Strength, Light Curve, Luminous Intensity, Magnetic Effects, Mass Transfer, X Ray Sources

Scientific paper

Spin phase dependence of polarization curves is found for radiation of
hot regions that appears as a result of accretion onto a strongly
magnetized star in a binary system. Curves obtained are essentially
different for various configurations of radiating region (spot,
symmetric or asymmetric column, etc.).

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