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   52049
   We propose to observe the X-ray binary pulsars 1E1024.0-5732 and
   2S0114+650 whose origins are controversial. These are the only
   persistent X-ray binary pulsars which are listed in the catalogue by
   van Paradijs (1995) and have not been observed with ASCA. 1E1024.0-
   5732/WACK 2134 may be the first X-ray selected Wolf-Rayet Star or a
   high mass X-ray binary system having the shortest spin-period (61
   msec). 2S0114+650 exhibits marginal 850 sec coherent pulsations and
   periodic X-ray flares accompanying iron line intensity variations.
   Using the unique timing and spectral capabilities of ASCA, we will try
   to resolve origins of these mysterious sources.
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