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    PR # 31006                                                                   
     V773 Tau is one of the most active weak-lined T Tauri stars known. It       
      shows variable circularly polarized radio emission, spot modulation        
      of the optical light curve, and X-ray emission. These traits indicat       
     e strong magnetic surface activity. We propose to obtain a 40 ksec  o       
     bservation of V773 Tau that will enable us to obtain emission line  f       
     luxes that are needed to construct a coronal model. In addition,  the       
      observation will allow us to search for slow (1 day) variability in        
     the X-ray emission that may occur as surface features rotate  across        
     the line-of-sight.                                                          
                                                                                 
                                                                                 
                                                                                 
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