The X-ray Luminosity Function and Gas Mass Function for Optically-Selected Poor + Rich Clusters of Galaxies

Details The X-ray Luminosity Function and Gas Mass Function for Optically-Selected Poor + Rich Clusters of Galaxies The X-ray Luminosity Function and Gas Mass Function for Optically-Selected Poor + Rich Clusters of Galaxies

1996-06-19

arxiv.org/abs/astro-ph/9606120v1

Astronomy and Astrophysics

Astrophysics

9 pages, LaTex, 1 Postscript table, 2 Postscript figures. Fig. 1 is a GIF, full version at ftp://astro.nmsu.edu/pub/CHRIS/xlum

Scientific paper

10.1086/310198

We present the first X-ray Luminosity Function (XLF) for an optically-selected sample of 49 nearby poor clusters of galaxies and a sample of 67 Abell clusters with z < 0.15. We have extended the measured cluster XLF by more than a factor of 10 in X-ray luminosity. Our poor cluster sample was drawn from an optical catalog of groups with 0.01

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