@misc{10481/29038,
year = {2003},
url = {http://hdl.handle.net/10481/29038},
abstract = {We 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.},
organization = {A. Castillo-Morales acknowledges support by the Marie Curie Training Site grant HPMT-CT-2000-00136 by the European Commission.},
publisher = {EDP Sciences},
keywords = {Galaxies},
keywords = {Clusters},
keywords = {Intergalactic medium},
keywords = {Evolution},
keywords = {Cosmology},
keywords = {X-rays},
title = {XMM observation of the dynamically young galaxy cluster CL 0939+4713},
author = {Filippis, E. de and Schindler, S. and Castillo-Morales, A.},
}