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   61103
   So far ASCA observed E0102-72 which is half degree away from the center
   of the Small Magellanic Cloud(SMC). The clear enhancement was detected
   between E0102-72 and the center of the SMC, and it suggests the tail
   part of the hot component in the center. It may correspond to the
   Galacitc Ridge X-ray emission observed in the Galaxy. We propose to
   observe the hot gas structure from the center to the north part of the
   SMC.
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