UBVRI photometry and polarimetry binary V1696 Cyg

  • K.A. Antonyuk Crimean Astrophysical Observatory, Nauchny, 298409

Abstract

The results of multi-polarimetric and photometric observations of a binary system V1696 CYG, obtained in the Crimean Astrophysical Observatory in 2006 is present. We show that the observed changes in the linear polarization in V1696 Cyg is well correlated with the phase of the orbital period. Changes in the brightness (~ 0.1m ) in the UBVRI bands was found. The correlation between changes in brightness with the phase of the orbital period is expressed weakly. We show the existence of the rapid photometric variability.

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Published
2009-06-01
How to Cite
Antonyuk K., 2009. Izvestiya Krymskoi Astrofizicheskoi Observatorii, vol. 105, no. 1, pp. 91-96. Available at: https://jn.craocrimea.ru/index.php/izvcrao/article/view/884 (Accessed: 3December2020)
Section
Research articles