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   72051
   The non-thermal nebula associated with the EGRET source GEV 1417-6100
   is an excellent candidate for a pulsar wind nebula. ASCA spectra can
   constrain the age and field strength of the particle accelerator
   powering the synchrotron emission. The data will set the stage for the
   detection of a central pulsar: while a period search is not guaranteed
   of success, the data set should allow a Pdot measurement that will help
   in detection of gamma-ray pulsations.
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