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   51086
   Kes 32 is the shell type radio SNR. We can see that this SNR has "jet",
   like plume, in radio map. We found the X-ray from Kes 32 by analyzing
   the asca data of PSR 1610-50, which is located near Kes 32. This is
   first detection in X-ray. Althouth only little part of the rim is
   detected in SIS ield of view, we can find the Si, S, Ar emission lines,
   which shows the very high temperature of the hot gas in SNR. Because of
   poor statistics, We could not restrict the physical parameters of hot
   gas well. Farthermore, the "jet" is out of field of view of both
   detector. We propose the observation of Kes 32 and its "jet" to reveal
   the origin of the "jet".
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