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Some physical consequences from the flare statistics of the UV Cet type stars in the solar neighbourhood

Published online by Cambridge University Press:  23 September 2016

N.I. Shakhovskaya
N.I. Shakhovskaya*
Affiliation:
Crimean Astrophysical Observatory Nauchny, Crimea 334413, USSR

Abstract

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The observational data permit us to establish statistical correlations between different parameters of stellar flare activity and the characteristics of quiet stars. We discusss physical consequences following from these relationships.

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. 53
Copyright
Copyright © Kluwer 1990