Search for a fine-time structure in flares of UV Cet-type stars

Details Search for a fine-time structure in flares of UV Cet-type stars Search for a fine-time structure in flares of UV Cet-type stars

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285..179p&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Reconnection in Space Plasma, Volume 2 p 179-181 (SEE N89-24974 1

Physics

Fine Structure, Stellar Flares, Time Series Analysis, Brightness Distribution, Stellar Spectrophotometry

Scientific paper

The results of electrophotometrical investigations of the 65 flares with a time resolution of 0.0000005 in 8 flare stars are presented. Analysis shows no fine time structure within the scale 0.000001 to 0.1 sec. The shortest times of brightness variations are 0.3 to 0.8 s and inherent in a phase in front of flares. In four stars (UV Cet, CN Leo, Wolf 424AB, V577 Mon) very fast flare events are observed.

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