We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
The paper presents the basic ideas of pinch-model for UV Cet star flares. The observational consequences and predictions are discussed.
Type
IV Theoretical Problems and Interpretation of Observations
1.Gershberg, R.E., Mogilevskii, E.I., Obridko, V.W. (1987) ‘Energetics of activity of flare stars and the Sun. A synergetical approach’, Fiz. i Kinem.neb.tel, 3(5), 3–17Google Scholar
2
2.Hayrapetyan, V.S., Nikoghossian, A.G., Vikhrev, V.V. (1988) ‘Pinch-effect and stellar flares physics’, in Guyenne, T.D. and Hunt, J.J. (eds.), Reconnection in Space PlasmaESA SP-285, II, 163–167Google Scholar
3
3.Hayrapetyan, V.S. (1989) ‘Gamma-bursts and flares on red dwarfs’, Astr.Tsirk., 1337, 17–18Google Scholar
4
4.Buslavskii, V.G., Severny, A.B. (1969) ‘Asymmetry effect of solar flares emission’, in Sobolev, V.V. (ed.), Stars, Nebulae, Galaxies, pp.129–134.Google Scholar
5
5.Grinin, V.P., Sobolev, V.V. (1977) ‘On the theory of flare stars’, Astrofisika, 13, 587–603Google Scholar
6
6.Harutyunian, H.A., Hayrapetyan, V.S. (1989) ‘On the gamma activity of stellar flares’, this volumeCrossRefGoogle Scholar
7
7.Kodaira, K. (1983) ‘Empirical models of stellar flares: constraints on flare theories’, in Byrne, P. B. and Rodono, M. (eds.), Activity in Red Dwarf Stars, pp. 561–578.Google Scholar