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   PR # 11027
    It has long been a matter of debate why the soft X-ray luminosity far
    exceeds the hard X-ray luminosity in Magnetic Catalysmic Variables
    (MCVs), although the soft X-ray is considered to be emitted as a
    reprocessed emission of the hard X-ray emission. Since the hard X-ray
    luminosity of the sources which are doubted to have excessive soft X-
    ray emission is so low in general that the hard X-ray luminosity has
    been measured only for the small number of sources, which prevents
    quantitative analysis of the soft X-ray excess problem.Using the high
    sensitivity and wide energy band of ASCA, we propose to observe MCVs
    which probably have excessive soft X-ray emission. In order to obtain
    soft X-ray information, we have also been planning simultaneous
   observations with other energy
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