| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10694501 | Advances in Space Research | 2005 | 4 Pages |
Abstract
We present results from a new 120Â ks XMM-Newton observation of the cluster of galaxies Sérsic 159-03. In this paper, we focus on the high-resolution X-ray spectra obtained with the Reflection Grating Spectrometer (RGS). The spectra allow us to constrain the temperature structure in the core of the cluster and determine the emission measure distribution as a function of temperature. We also fit the line widths of mainly oxygen and iron lines.
Keywords
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Earth and Planetary Sciences
Space and Planetary Science
Authors
J. de Plaa, J.S. Kaastra, M. Méndez, T. Tamura, J.A.M. Bleeker, J.R. Peterson, F.B.S. Paerels, M. Bonamente, R. Lieu,