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Photoelectric observations of flares on UV Ceti

Published online by Cambridge University Press:  23 September 2016

N.D. Melikian  and
V.S. Shevchenko
N.D. Melikian
Affiliation:
Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR
V.S. Shevchenko
Affiliation:
Tashkent Astronomical Institute, Uzbek Academy of Sciences, USSR

Abstract

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Synchronous observations of the UV Cet flares were carried out in 1987. Two 60-cm telescopes in U-band were used. Accuracy of syncronous registration on two telescopes is 0.001s. 15 flares were registered simultaneously during observations. Single short-time (up to 2s) light increases were observed in quiescent state and flares, which are the result of observation errors. No light increase with duration shorter than 10s was registered simultaneously on two telescopes.

Type
I Flare Stars Optical Observations and Flare Statistics
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 31 - 32
Copyright
Copyright © Kluwer 1990 

References

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