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Paper: A Chandra X-ray and ATCA Radio Comparison of SNR N103B in the Large Magellanic Cloud
Volume: 262, The High Energy Universe at Sharp Focus: Chandra Science
Page: 339
Authors: Scronce, G.; Feng, H.; Keohane, J. W.; Olbert, C. M.
Abstract: We present an X-ray and radio comparison of the Supernova Remnant N103B in the Large Magellanic Cloud. N103B is particularly interesting, because of the strong asymmetry, which is due to the strong density gradient of the surrounding medium. We present archival Chandra data, which are compared to the ATCA radio data of Dickel (1995). In addition, we fit thermal and non-thermal shock models, and discuss the dynamics of this SNR.
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