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.
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Parsamian, E.S., Mujica, R. & Corral, L. Spectroscopic Observations of Subfuors (Exors). I. V1118 Ori. Astrophysics 45, 393–399 (2002). https://doi.org/10.1023/A:1021865909178
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DOI: https://doi.org/10.1023/A:1021865909178