Two periods of the variability in V380 Oph

Details Two periods of the variability in V380 Oph Two periods of the variability in V380 Oph

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..330..495s&link_type=abstract

The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference Vol. 330. Edited by J.-M. Hameury a

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

It was shown that the nova-like cataclysmic variable V380 Oph is at the "high" most of the time and sometimes switches over to "low" stage. The "low" state continues through several months. We classified V380 Oph as an "anti-dwarf-nova", or VY Scl-type star. The orbital period was rectified (Porb=0.d14817) and the independent period (P2=4.d513) was found.

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