Место издания:Astronomical Society of the Pacific. [Provo, Utah, etc.], United States San Francisco
Первая страница:495
Последняя страница:496
Аннотация: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.