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On the gamma-activity of stellar flares

Published online by Cambridge University Press:  23 September 2016

H.A. Harutyunian  and
V.S. Hayrapetyan
H.A. Harutyunian
Affiliation:
Byurakan Astrophysical Observatory, Armenian Academy of Siences, USSR
V.S. Hayrapetyan
Affiliation:
Byurakan Astrophysical Observatory, Armenian Academy of Siences, USSR

Abstract

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The principal possibility of γ-ray manifestation of stellar flares in the framework of pinch-model is shown. Validity of assumption that, γ-bursts are connected with magnetically active dwarfs (MAD) is discussed.

Type
IV Theoretical Problems and Interpretation of Observations
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 333 - 336
Copyright
Copyright © Kluwer 1990 

References

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