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   PR #     9
   PV Observation of CapellaCapella is a bright nearby G-K binary system.
   Like RS CVn systems, Capellaexhibits flaring behavior and hot coronal
   emission. This coronal emission isnot isothermal, and may come from
   two predominant temperatures (possiblyassociated with two sets of loop
   structures: flares on one star, and loopsextending between stars), or
   from a continuous distribution of temperatures.This observation may
   help to resolve this issue.
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