The X-ray Luminosity Function of Nearby Rich and Poor Clusters of Galaxies: A Cosmological Probe
arXiv:astro-ph/9903117 · doi:10.1086/311996
Abstract
In this letter, we present a new determination of the local (z<0.09) X-ray luminosity function (XLF) using a large, statistical sample of 294 Abell clusters and the ROSAT All-Sky-Survey. Given our large sample size, we have reduced errors by a factor of two for L(X)(0.5-2keV)>10^43 ergs/sec. We combine our data with previous work in order to explore possible constraints imposed by the shape of the XLF on cosmological models. A set of currently viable cosmologies is used to construct theoretical XLFs assuming Lx is proportional to M^p and a sigma_8-Omega_0 constraint (from Viana & Liddle 1996) based on the local X-ray temperature function. We fit these models to our observed XLF and verify that the simplest adiabatic, analytic scaling relation (e.g. Kaiser 1986) disagrees strongly with observations. If we assume that clusters can be described by the pre-heated, constant core-entropy models of Evrard & Henry (1991) then the observed XLF is consistent only with 0.1 < Omega_0 < 0.4 if the energy per unit mass in galaxies is roughly equal to the gas energy (ie if beta=1). (abridged)
4 pages, 2 figures, accepted for publication in ApJ Letters. uses emulateapj.sty
References in corpus (9)
- Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
- The ROSAT Brightest Cluster Sample (BCS) - I. The compilation of the sample and the cluster log N-log S distribution
- The Evolution of X-ray Clusters in Low Density Universes
- A Catalog of 200 Galaxy Clusters Serendipitously Detected in the ROSAT PSPC Pointed Observations
- The ROSAT Deep Cluster Survey: the X-ray Luminosity Function out to z=0.8
- The Most Massive Distant Clusters: Determining Omega and sigma_8
- The Age Of Globular Clusters In Light Of Hipparcos: Resolving the Age Problem?
- The WARPS survey - II: The Log(N)-Log(S) relation and the X-ray evolution of low luminosity Clusters of Galaxies
- Cosmological Constraints from the ROSAT Deep Cluster Survey
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- A New Measurement of the X-ray Temperature Function of Clusters of Galaxies
- The Mass-To-Light Function of Virialized Systems and the Relationship Between Their Optical and X-ray Properties
- Mapping Large-Scale Structures Behind the Galactic Plane: The Second CIZA Subsample
- The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II) IV. X-ray Luminosity Function and First Constraints on Cosmological Parameters
- The X-ray Properties of Nearby Abell Clusters from the ROSAT All-Sky Survey: The Sample and Correlations with Optical Properties
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