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   71040
   We propose to observe the newly discovered Galactic Jet Source CI Cam
   in its steady state, a possible second example of SS~433. ASCA
   observation of CI Cam in outburst suggests an interesting possibility
   that the X-ray emission originated from the twin jets. Our aim is to
   detect the steady X-ray emission from this symbiotic system, which is
   expected to be highly absorbed. This will enable us to conclude whether
   or not the X-ray emission observed during the outburst was truely
   associated with the jets. Also, the spectrum will lead to the unique
   identification of the compact object in this peculiar system.
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