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   71095
   Large and Small Magelanic Clouds have extremely ideal characters for
   the systematic study from the X-ray scope. The aims and expected fruit
   of this survey are 1: Derive the survey of the SNRs which are not
   observed deeply yet with ASCA, get the more completely sample for the
   study of SNR evolution. 2: Find the non-thermal X-ray emission SNRs,
   which will be the proof that these SNRs deals with the cosmic ray
   accerelation. 3: Find out the new X-ray pulsar, to know the reason for
   the difference of the population of X-ray sources among SMC, LMC and
   our galaxy. 4: Study the X-ray spectrum and the spatial structure of
   the star forming region in both galaxies. 5: Get the complete X-ray
   images(2-10keV band), which greately help us for the comparison with
   other wavelength.
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