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Variation in the flare activity of the star UV Ceti
Authors:N D Melikian  V S Tamazian  A L Samsonyan
Institution:1.V. A. Ambartsumyan Byurakan Astrophysical Observatory,Byurakan,Armenia;2.Ramon Maria Aller Astronomical Observatory,University of Santiago de Compostela,Santiago de Compostela,Spain
Abstract:This is an analysis of the dependence of the flare activity of the well known flare star UV Ceti on the linear distance between the components of this binary system. It is shown that its flaring activity clearly depends on the mutual distance of the components, while this kind of variability is not seen in isolated flare stars.
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