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   52029
   A class of tremendous outburst amplitude dwarf novae (TOADs) has been
   identified, which show similar minimum light properties as soft X-ray
   transients (SXTs). We propose to make ASCA observations of three
   quiescent TOADs. These will allow us to make fundamental tests, using
   model fits to the obtained X-ray spectra in quiescence, of the minimum
   state accretion disk, mass transfer rates, and search for spin
   modulations from the white dwarf primary.
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