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T.G. Pannuti, G.E. Allen, K.A. Flanagan (MIT Center for Space Research), M.D. Filipovic (ATCA), J.R. Dickel (Illinois)
In order to search for non-thermal X-ray emission from the Large Magellanic Cloud supernova remnants N103B and N132D, we have analyzed Chandra observations of these remnants and compared them to radio observations made using the Australia Telescope Compact Array (ATCA). We have extracted Advanced CCD Imaging Spectrometer (ACIS) spectra from regions in both remnants which are coincident with radio emission, and compared these against spectra taken from regions which are devoid of radio emission. Initial results and preliminary conclusions will be presented.
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