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Spectroscopic Observations of Subfuors (Exors). I. V1118 Ori
Authors:Elma S. Parsamian  Raul Mujica  Luis Corral
Affiliation:(1) V. A. Ambartsumian Byurakan Astrophysical Observatory, Armenia;(2) National Institute of Astrophysics, Optics, and Electronics, Mexico
Abstract:Spectroscopic observations of the star V1118 Ori during the 1992-94 outburst showed that, as during the 1989 outburst, the spectrum resembles that of a T Tauri star with strong hydrogen and Ca II lines, as well as Fe I, Fe II, He I, and Na I lines of moderate intensity.
Keywords:stars  stars flare  stars individual  V1118 Ori
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