Back to Search Start Over

The temperature structure in the core of Sersic 159-03

Authors :
F. B. S. Paerels
Takayuki Tamura
Mariano Mendez
Johan A. M. Bleeker
Richard Lieu
J. de Plaa
John R. Peterson
Massimiliano Bonamente
Jelle Kaastra
Publication Year :
2005
Publisher :
arXiv, 2005.

Abstract

We present results from a new 120 ks XMM-Newton observation of the cluster of galaxies Sersic 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.<br />Comment: 7 pages and 4 figures. Contribution to the proceedings of the COSPAR Scientific Assembly, session E1.2 "Clusters of Galaxies: New Insights from XMM-Newton, Chandra and INTEGRAL", july 2004, Paris (France). Accepted for publication in Advances in Space Research

Details

Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....ca26e43839d013b7523e09466692ed64
Full Text :
https://doi.org/10.48550/arxiv.astro-ph/0504262