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   PR #   140
   The 5.57 hr LMXRB X1822-371 is an eclipsing binary. The eclipse is
   partial, indicating the X-ray source is hidden behind an accretion
   disk coronae. The ASCA observation will study the spectrum as a
   function of binary phase.A large fluorescent iron K line is expected
   because the X-ray emission is scattered to the observer via the
   corona.
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