August 11-15, 2014


Analysis of eclipses in V1032 Ophiuchi

Karolina Bakowska (N. Copernicus Astronomical Center )

Arkadiusz Olech N. Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18 00-716 Warsaw, Poland

We present results of the photometric observations of V1032 Ophiuchi made on SALT telescope. Data were obtained during two runs in 2012 (July 11 and 15). V1032 Oph was classified as a variable star of RR Lyr type, but this object is a typical example of a cataclysmic variable. The analysis of eclipses observed in light curves of V1032 Oph was conducted, i.e. we used the decomposition method (Smak, 1994) to obtain separate light curves of the hot spot and the disk.

Mode of presentation: poster