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   PR # 43016
   We seek ASCA observations of three recently advanced intermediate
   polar candidates to confirm their classification and to secure, for
   the first time, accurate constraints on their basic X-ray emission
   properties (inclusion of these objects will expand the group by about
   20%). In at least one case (probably all cases), coarsely
   phase-resolved spectra will be used to quantify the role of partial
   covering. At the same time, line diagnostics, in particular the iron
   transitions, can be exploited t
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