Relations of Physical Properties for a Large Sample of X-Ray Galaxy Clusters
Astrophysics
2007-05-23 v1
Abstract
One hundred and six galaxy clusters have been studied in detail using X-ray data and important global physical properties have been determined. Correlations between these properties are studied with respect to the description of clusters as a self-similar class of objects. The results support the self-similar picture only partly and significant deviations are found for some correlations.
Keywords
Cite
@article{arxiv.astro-ph/9909071,
title = {Relations of Physical Properties for a Large Sample of X-Ray Galaxy Clusters},
author = {Thomas H. Reiprich and Hans Boehringer},
journal= {arXiv preprint arXiv:astro-ph/9909071},
year = {2007}
}
Comments
4 pages; to be published in the Proceedings of the Ringberg Workshop on Diffuse Thermal and Relativistic Plasma in Galaxy Clusters, Ringberg Castle (1999); also available at http://www.xray.mpe.mpg.de/~reiprich/act/publi.html