Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58..350k&link_type=abstract
Astronomicheskii Zhurnal, vol. 58, Mar.-Apr. 1981, p. 350-354. In Russian.
Astronomy and Astrophysics
Astronomy
1
Atmospheric Heating, Chromosphere, Dynamic Response, Stellar Flares, Stellar Luminosity, Stellar Models, X Ray Sources, Dwarf Stars, Particle Acceleration, Plasma-Electromagnetic Interaction, Stellar Atmospheres, Stellar Coronas, Stellar Evolution, Stellar Magnetic Fields, Stellar Mass Ejection
Scientific paper
It is suggested that the origin of large heating fluxes in intense events on flare stars is associated with the annihilation of magnetic fields; the strength of these fields in the lower corona must be of the order of several hundred oersted. The observed X-ray-to-optical luminosity ratios are consistent with the present theoretical estimates and yield evidence that in soft X-ray flares, the outflowing hot gas is confined by the magnetic field near the surface of the star.
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