Superhumps and Period Variability of V795 Her

Details Superhumps and Period Variability of V795 Her Superhumps and Period Variability of V795 Her

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20913706m&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #137.06; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

Scientific paper

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 0.115487 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.

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