Examination of the X-ray spectrum of the SNR 0509-67.5
Publication date
2009-03-19
Authors
Kosenko, D.
Vink, J M
Editors
Branduardi-Raymont, G.
Blustin, A.
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Abstract
We discuss XMM-Newton observations of the supernova remnant 0509-67.5 in the Large Magellanic Cloud. EPIC and RGS data were studied extensively using SPEX spectral software package. The analysis allowed us to obtain dynamical properties of the SNR and also plasma conditions in the remnant.
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Kosenko, D & Vink, J 2009, Examination of the X-ray spectrum of the SNR 0509-67.5. in G Branduardi-Raymont & A Blustin (eds), Proceedings of the international workshop held at the Mullard Space Science Laboratory of University College London, Holmbury St Mary, Dorking, Surrey, UK, March 19 - 20, 2009. Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey, pp. E24/1-E24/11.