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On the gamma-activity of stellar flares
Published online by Cambridge University Press: 23 September 2016
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
- Copyright
- Copyright © Kluwer 1990
References
1.
Hayrapetyan, V.S. (1989) ‘Gamma-bursts and flares on red dwarfs’, Astr.Tsirk., 17–18.Google Scholar
2.
Hayrapetyan, V.S., Nikoghossian, A.G. and Vikhrev, V.V. (1989) ‘Pinch-effect and stellar flares physics’, in Guyenne, T.D. and Hunt, J.J. (eds.), Reconnection in Space Plasma, ESA SP-285, II, 163–167.Google Scholar
3.
Mazets, E.P. and Golenetskii, S.V. (1987) ‘Cosmic gamma-bursts observations’, in Sunyaev, R.A. (ed.), Itogi nauki i tekhniki, ser. Astronomia, Moskva, 16–42.Google Scholar
4.
Vahia, M.N. and Rao, A.R. (1988) ‘Origin of the gamma-ray bursts’, Astron. Astrophys., 207, 55–69.Google Scholar
5.
Montmerle, T., Koch-Miramond, L., Falgarone, E. and Grindlay, J.E. (1983), ‘Einstein observations of the Rho Ophiu-Chi dark cloud: an X-ray Christmas Tree’, Astrophys. J., 269, 182–201.CrossRefGoogle Scholar