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   63007
   Of the 17 intermediate polars bright enough for phase-resolved
   spectroscopy with ASCA, 15 have been observed, and we request time for
   the remaining two in this proposal. We are part-way through a
   systematic and detailed analysis of the spin pulses in these stars,
   aimed at understanding the class as a whole. V1062 Tau has
   exceptionally long spin and orbital periods, allowing as to study
   accretion at one extreme of the class. V709 Cas is the opposite, with
   the shortest spin period accessible to ASCA. Studying the two extremes
   will allow us to test the theory that intermediate polars cycle between
   the extremes as they cycle from diskless to disk-fed states.
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