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arXiv · astro-ph/9909035

The Empirical X-Ray Luminosity - Gravitational Mass Relation for Clusters of Galaxies

Thomas H. Reiprich·Hans Boehringer
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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.

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Thomas H. Reiprich, Hans Boehringer. 1999-09-02. The Empirical X-Ray Luminosity - Gravitational Mass Relation for Clusters of Galaxies. https://doi.org/10.1002/1521-3994(199908)320%3A4%2F5%3C296%3A%3Aaid-asna296%3E3.0.co%3B2-8

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