X-ray spectroscopy of SN(R)1987A with RGS

Physics

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Scientific paper

Our XMM-Newton monitoring program of the remnant of SN 1987A with yearly observations since January 2007 provided us with EPIC and RGS spectra of unprecedented quality. The soft X-ray light curve shows a significant flattening after 2005. The RGS spectra allow us to study the time evolution of the shock conditions and abundance profiles of, e.g., N, O, Fe and Ne. I'll present the results of a detailed analysis of the available RGS spectra.

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