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   51125
   The SMC is an edge-on galaxy with depleted abundance. So far Asca
   observed E0102 which is half degree away from the galactic center. No
   observation on the center has been done by Asca. There is a clear
   enhancement between E0102 and the galactic center suggesting the tail
   part of the hot component in the center. We propose to observe the hot
   gas structure from the center to the norther part with which we can
   study the correlation between the possible halo component and the hot
   gas around the galactic plane. The hot component may be related to the
   possible low luminosity active galactic nucleous in the SMC.
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