Abstract
We have isolated Mg II k emission line profiles arising solely from the flaring region during flares on AR Lac and V 711 Tau. From several high-resolution spectra obtained during the lifetime of the flare, we have determined the size and position of the flaring regions and studied the decay of the emission line width, radial velocity, and integrated line flux.
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References
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© 1988 Kluwer Academic Publishers
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Neff, J.E., Linsky, J.L. (1988). Spatially Resolved Flares in RS CVn Systems. In: Havnes, O., Pettersen, B.R., Schmitt, J.H.M.M., Solheim, J.E. (eds) Activity in Cool Star Envelopes. Astrophysics and Space Science Library, vol 143. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2951-7_29
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DOI: https://doi.org/10.1007/978-94-009-2951-7_29
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7827-6
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