Abstract
AbstractThe arguments in favour of that the primary heating of the gas at the impulsive phase of stellar flares is caused by charged particles of higher energies than in the solar flares are given. It is shown that the model of the deep heating by high energy protons (E ≃ 10 MeV) or electrons (E ≃ 100 keV) with taken into account of the radiative transfer in flare region explane the main properties of the optical continuum of the flare.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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1. Review of the Theoretical Models of Flares of the UV CETI-Type Stars;Flare Stars in Star Clusters, Associations and the Solar Vicinity;1990