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Flare variability in the close binary FL Vir
Authors:B R Pettersen
Institution:Department of Mathematical Sciences and Technology, University of Environmental and Life Sciences, PO Box 5003, N-1432 Ås, Norway
Abstract:The results of U -filter flare monitoring of the binary flare star FL Vir = Wolf 424 is presented. 57 flares with energies between  2 × 1028  and  2 × 1031 erg  were recorded in 20 h of observation. The properties of flare occurrence and flare time-scales are analysed, and the flare activity level in 1980 April is determined to be   L f( U ) = 8.0 × 1026 erg s?1  . This is larger than previously published results and may indicate a variation in the flare activity level on a time-scale of years. An analysis of existing data indicates that the flare activity level correlates with the relative orbital positions of the stars.
Keywords:techniques: photometric  binaries: close  stars: flare
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