Relations of Physical Properties for a Large Sample of X-Ray Galaxy Clusters

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dc.creatorReiprich, Thomas H.
dc.creatorBoehringer, Hans
dc.date1999-09-03
dc.date.accessioned2026-07-07T02:33:04Z
dc.date.available2026-07-07T02:33:04Z
dc.descriptionOne 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.
dc.description4 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9909071
dc.identifierhttp://arxiv.org/abs/astro-ph/9909071
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14698
dc.subjectAstrophysics
dc.titleRelations of Physical Properties for a Large Sample of X-Ray Galaxy Clusters
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