Abstract
We present results of multicolor photometric and polarimetric observations of the binary system V1696 CYG obtained in the Crimean Astrophysical Observatory in 2006. It is shown that observed variations of the linear polarization of the V1696 Cyg light are well correlated with the orbital period phase. We also found brightness variations (∼0.1m) in the UBVRI bands. The brightness variations are weakly correlated with the orbital period phase. A rapid photometric variability was found.
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