NASA NTRS · 19900031838
Spatially resolved flares in RS CVn systems
Abstract
Mg II k emission-line profiles arising solely from the flaring region during flares on AR Lac and V 711 Tau have been isolated. From several high-resolution spectra obtained during the lifetime of the flare, the size and position of the flaring regions have been determined, and the decay of the emission line width, radial velocity, and integrated line flux has been studied.
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Neff, James E., Linsky, Jeffrey L.. 1988-01-01. Spatially resolved flares in RS CVn systems. https://ntrs.nasa.gov/citations/19900031838
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