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Slow flares and eruptive phenomena in early stages of stellar evolution

Published online by Cambridge University Press:  23 September 2016

M.A. Ibrahimov  and
V.S. Shevchenko
M.A. Ibrahimov
Affiliation:
Astronomical Institute Uzbek Academy of Sciences USSR
V.S. Shevchenko
Affiliation:
Astronomical Institute Uzbek Academy of Sciences USSR

Abstract

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Correlations between different eruptive phenomena (fast and slow flares, large-scale eruptive variations up to fuor phenomenon) in stellar instability during stage of evolution are analysed A conclusion is drawn on the difference in natures of eruptive phenomena lasting some ten minutes and slower variations lasting more than one day.

Type
III Flare Stars and Related Objects Fuors and Other Non-Stable Objects
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 257 - 260
Copyright
Copyright © Kluwer 1990 

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