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   PR # 42077
   We propose an ASCA observation of the Crab-like supernova remnant MSH
   11-62. MSH 11-62 shows distinct evidence of a central engine powering
   a synchrotron nebula. The radio spectrum is relatively flat, the
   X-ray spectrum appears to be nonthermal and an EGRET source has been
   associated with the SNR. The proposed ASCA observation will fully
   characterize the nature of the emission and identify the contribution
   from a central pulsar-driven synchrotron nebula.
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