On the Initial Phase of the Flares of the Uv-Ceti Type Stars

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Arguments for the proton heating of the optical emission region in the
flares of UV Ceti-type stars are given. The electron temperature and
number density of atoms in this region are evaluated: T ≅ 7000 -
13000K and nH ≅ 1016cm-3 at an
proton energy of E ≅ 10 MeV.

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