The Empirical X-Ray Luminosity - Gravitational Mass Relation for Clusters of Galaxies
arXiv:astro-ph/9909035 · doi:10.1002/1521-3994(199908)320:4/5<296::AID-ASNA296>3.0.CO;2-8
Abstract
A sample of one hundred and six X-ray galaxy clusters has been analysed in detail. Here we give the observed X-ray luminosity - gravitational mass relation. Possible future applications include conversion of empirical cluster luminosity functions to mass functions and conversion of simulated mass functions to luminosity functions.
1 page; to be published in the Proceedings of the 4th ASCA Symposium on Heating and Acceleration in the Universe, Tokyo (1999); also available at http://www.xray.mpe.mpg.de/~reiprich/act/publi.html
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