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   62016
   HR5110 is a fundamentally important RS CVn system due to observed
   outbursts (3 and 7 days duration) suggestive of inter-binary flaring.
   ASCA will play a pivotal and essential role in a multi-wavelength
   observing campaign to investigate this system, the brightest RS CVn
   system still to be observed by ASCA. The frequency with which large
   outbursts have previously been observed make it likely that such an
   event will again be observed by ASCA. However although fortuitous, this
   is not essential to this program. High-resolution GIS and SIS spectra
   will determine the X-ray luminosities, and most importantly, coronal
   abundances, helping to provide constraints on temperature and density
   stratification of this system's coronal environment.
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