The Long Period Recurrent Nova RS Oph

Details The Long Period Recurrent Nova RS Oph The Long Period Recurrent Nova RS Oph

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..404...72v&link_type=abstract

The Eighth Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conference Series, Vol. 404, proceed

Astronomy and Astrophysics

Astrophysics

Scientific paper

The new CCD observations of recurrent nova RS Oph were taken in April 2008 in continuation of our study of short-term variability of this star. They were carried out with 50 cm and 60 cm telescopes of Sternberg Astronomical Institute in Crimea. The analysis of all our data obtained in 2007 and 2008 reveals a periodic oscillations with different periods on the time scale of dozens of minutes and flickering with an amplitude of about ˜0m.2 on the time scale of minutes. The consideration properties of detected brightness variations shows that they could be interpret as a quasi-periodic oscillations.

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