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   71039
   We discovered a new varible X-ray source with 1530-s cohelent period in
   ASCA Galactic Plane Survey. Since the pulsation period of 1530s is
   between those of typical white dwarfs and typical neutron stars, we
   cannot determine directly whether it is a white dwarf or a neutron
   star. If it is a neutron star, it becomes the slowest X-ray pulsar in
   our galaxy. We tried a spectral analysis, but could not get a
   statistically sufficient result because the flux is weak and the source
   position is near the edge of the field of view. However, we found a
   sign of eccentric structures in the spectrum above 4 keV, which might
   represent strong iron-line, partial covering absorption, multi-
   temperature plasma, or cyclotron absorption. Then, we propose a follow-
   up observation to study this ASCA new source.
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