Applications of the Doppler Imaging Technique to the Analysis of High Resolution Spectra of the 3 October 1981 Flare on V711 Tauri
An unconstrained four gaussian fit to the Mg II profile near the flare peak indicates that the flare occurred near the central meridian of the K1 IV star, perhaps above a spot. A more likely fit to the same data places the flare at +90±30 km s-1 relative to the K1 IV star, indicating significant downflowing plasma.
The Impact of Very High S/N Spectroscopy on Stellar Physics
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