Quiescent and Flaring Structure in Rs Cvn
نویسنده
چکیده
منابع مشابه
Quiescent and Flaring Structure in Rs Canum Venaticorum Stars
Four of the most active RS CVn stars (V711 Tau, II Peg, Gem, and UX Ari) have been observed for a total of 3Ms with the Extreme Ultraviolet Explorer satellite (EUVE) between 1992 and 2000 January. Flaring and quiescent states of extreme ultraviolet spectra ( 70–740) and light curves ( 75–175) have been analyzed to provide emission measure distributions (EMD) for these systems in the range logTe...
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تاریخ انتشار 2002