*************************************************************************
   72079
   We continue our study of the supernova remnants in the Large Magellanic
   Cloud with the goal of studying their dynamcal states and mean
   metallicities. New ASCA observations of five remnants with radii from
   16 pc to 28 pc are proposed. These remnants are among the
   largest/oldest in the sample and as such will provide a test of the
   effects of differing evolutionary states on the derivation of
   abundances from SNR X-ray spectroscopy.
 *************************************************************************