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19 April 2024
 
  » arxiv » astro-ph/0304027

 Article overview


XMM observation of the dynamically young galaxy cluster CL 0939+4713
E. De Filippis ; S. Schindler ; A. Castillo-Morales ;
Date 1 Apr 2003
Journal Astron.Astrophys. 404 (2003) 63-74
Subject astro-ph
Affiliation1 and 2), S. Schindler (3 and 1), A. Castillo-Morales (4 and 1) ( A.R.I. John Moores University, MIT, University of Innsbruck, University of Granada
AbstractWe present an XMM observation of the distant galaxy cluster CL 0939+4713. The X-ray image shows pronounced substructure, with two main subclusters forming the cluster core. This is an indication that the cluster is a dynamically young system. This conclusion is supported by the temperature distribution: a hot region is found between the two main subclusters indicating that they are at the beginning of a major merger, and that they will collide in a few hundreds of Myr. The intra-cluster gas of CL 0939+4713 shows inhomogeneities in the metal distribution, with the optically richer subcluster having a higher metallicity.
Source arXiv, astro-ph/0304027
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