Spectropolarimetric observation of RS Oph Authors: * Yanko Nikolov and Radoslav Zamanov Institution: * Institute of Astronomy and National Astronomical Observatory, BAS, Bulgaria Preferred format: * Oral Abstract Text: * RS Oph is a symbiotic recurrent nova which exhibits recurrent nova outbursts approximately every 15-20 years. During the outbursts the brightness rises from an initial value of V ∼ 11 to V ≈ 6 magnitude. We present spectropolarimetric observation of RS Oph, obtained with the 2-Channel Focal Reducer (FoReRo2), attached at the Cassegrian focus of the 2.0m RCC telescope of the Bulgarian National Astronomical Observatory Rozhen.