On the polarimetric variability of Y Cygni

Details On the polarimetric variability of Y Cygni On the polarimetric variability of Y Cygni

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..370f&link_type=abstract

Publications of the Astronomical Society of the Pacific, vol. 106, no. 698, p. 370-375

Astronomy and Astrophysics

Astronomy

3

Astronomical Polarimetry, Eclipsing Binary Stars, Cygnus Constellation, Stellar Envelopes, Stellar Winds, Variable Stars

Scientific paper

The behavior of the B-band polarimetric data of Y Cygni is analyzed. A period search of the data indicates that the only significant periods arise due to the frequency with which the system had been observed. Around the eclipsing phases there is evidence to suggest that the primary star possesses a stellar wind. speculations regarding the possible envelope geometry are also commented upon.

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