Exploring the Small Scale Structure of N103B
K. T. Lewis, D. N. Burrows, J. A. Nousek, G. P. Garmire, P. Slane, J. P. Hughes
Abstract
We present the preliminary results of a 40.8 ks Chandra ACIS observation of the young supernova remnant (SNR) N103B located in the Large Magellanic Cloud. The image reveals structure at the sub-arcsecond level, including several bright knots and filamentary structures. The remnant has the characteristic spectrum of a Type Ia SNR, containing strong lines of Fe, He-and H-like Si and S, Ar, and Ca. Narrow band images reveal non-uniformities in the remnant.
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