A Photometric Investigation and Examination of Superhumps of V795 Her

We present new photometric data, taken at the Crimean Laboratory of Sternberg Astronomical Institute and University of Dallas, on the suspected intermediate polar V795 Her. Photometry reveals a period of 0.1155 days. This period, when compared with past observations, shows a slight modulation and even a complete disappearance in mid-1990. Light curves of V795 Her are also shown to demonstrate some superhump activity. Superhumps as the possible result of accretion disk precession are discussed.