AO Cassiopeiae - Phase-locked polarization and the geometry of the gas stream

Details AO Cassiopeiae - Phase-locked polarization and the geometry of the gas stream AO Cassiopeiae - Phase-locked polarization and the geometry of the gas stream

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207l.125r&link_type=abstract

Astrophysical Journal, vol. 207, July 15, 1976, pt. 2, p. L125-L128.

Astronomy and Astrophysics

Astrophysics

31

Eclipsing Binary Stars, O Stars, Polarization Characteristics, Stellar Mass Ejection, Astronomical Models, Flow Geometry, Gas Streams, Light Scattering

Scientific paper

Variable linear polarization in this O-star close binary has been found
to be accurately synchronous with the orbital motion over a span of 20
cycles. The polarization is explained by light scattered from a gas
stream. Our analysis indicates that the main scaterring region is on the
advancing side of the secondary star.

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