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On two possible groups of flare stars in Pleiades

Published online by Cambridge University Press:  23 September 2016

A.L. Mirzoyan
Affiliation:
Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR
M.A. Mnatsakanian
Affiliation:
Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR

Abstract

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The correlation between the magnitude of the proper motion and the mean frequency of flares for flare stars in the Pleiades cluster region is discussed. The magority of them are physical members of this star cluster. It is shown that there exist probably two groups of flare stars which differ each other by their parameters, in particular by the magnitude of proper motions. A possible explanation of this phenomenon is suggested.

Type
I Flare Stars Optical Observations and Flare Statistics
Copyright
Copyright © Kluwer 1990 

References

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