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   51094
   We propose to observe two SNRs that are newly discovered with Rosat.
   They are G69.7+1.0 and G7.7-3.7. G69.7+1.0 shows an extended structure
   parallel to the galactic plane suggesting the hot bubble prevailing in
   the galaxy. G7.7-3.7 shows a shell structure with asymmetric X-ray
   brightness. Since they are dim in radio, they have not been observed
   before the Rosat era. They may form a new type of SNR groups.
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