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   61077
   We have found the bright X-ray point source in the southern break of
   the Cygnus Loop supernova remnant during the ASCA AO-5 observation
   phase. We performed the timing analysis by using the GISs but failed to
   detect the X-ray pulsation. To detect the X-ray pulsation, we propose
   to observe this point source as soon as possible. This will prove the
   Cygnus Loop to be type II SN in origin.
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