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

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

1999-09-02

arxiv.org/abs/astro-ph/9909035v1

Astronomy and Astrophysics

Astrophysics

1 page; to be published in the Proceedings of the 4th ASCA Symposium on Heating and Acceleration in the Universe, Tokyo (1999)

Scientific paper

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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