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1994PASP..106..370F - Publ. Astron. Soc. Pac., 106, 370-375 (1994/April-0)
On the polarimetric variability of Y Cygni.
FOX G.K.
Abstract (from CDS):
The behavior of hte B-band polarimetric data of Y Cyg (Koch and Pfeiffer 1989) are 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. The speculations by Koch and Pfeiffer regarding the possible envelope geometry are also commented upon.
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