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   62081
   The broad energy range and imaging capabilities of ASCA have provided a
   new tool to study the evolution and classification of supernova
   remnants (SNRs) in detail. Composite remnants in particular, have
   proven to be one of the most revealing field of study. We propose to
   study 2 composite supernova remnants: G16.7+0.1 and G18.95-1.1. Both
   present indications, deduced from radio data, of an existing compact
   object and have been shown to be X-ray emitters. The proposed
   observations will help to identify unambiguously the compact object
   inferred from the radio profiles and to determine their
   characteristics. In addition, we will analyze the emission from the
   rest of the SNRs to study the parameters of their dynamical evolution.
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