A Chandra X-ray and ATCA Radio Comparison of SNR N103B in the Large Magellanic Cloud

Details A Chandra X-ray and ATCA Radio Comparison of SNR N103B in the Large Magellanic Cloud A Chandra X-ray and ATCA Radio Comparison of SNR N103B in the Large Magellanic Cloud

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..262..339s&link_type=abstract

The High Energy Universe at Sharp Focus: Chandra Science, held in conjunction with the 113th Annual Meeting of the ASP. ASP Conf

Astronomy and Astrophysics

Astronomy

Scientific paper

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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