Abstract
We present equivalent widths and profiles for Hα Hβ, Hγ and He I λ4471 Å emission lines obtained in observations of the flares of EV Lac made at the Crimean Astrophysical Observatory in 1994 and 1995. Our semi-empirical modeling of the flares gives insight into the structure of the emitting regions, including a temperature plateau, and also into the physical parameters, size, and location of the star’s relatively quiescent chromosphere.
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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 78, No. 4, 2001, pp. 359–369.
Original Russian Text Copyright © 2001 by Baranovski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\), Gershberg, Shakhovskoi\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\).
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Baranovskii, É.A., Gershberg, R.E. & Shakhovskoi, D.N. Emission lines of the red-dwarf flare star EV Lac: Stellar flares. Astron. Rep. 45, 309–318 (2001). https://doi.org/10.1134/1.1361323
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DOI: https://doi.org/10.1134/1.1361323