The Lx-T Relation and Temperature Function for Nearby Clusters Revisited
arXiv:astro-ph/9802059 · doi:10.1086/306080
Abstract
The X-ray luminosity-temperature relation for nearby T=3.5-10 keV clusters is rederived using new ASCA temperatures and ROSAT luminosities. Both quantities are derived by directly excluding the cooling flow regions. This correction results in a greatly reduced scatter in the Lx-T relation; cooling flow clusters are similar to others outside the small cooling flow regions. For a fit of the form L_bol ~ T^alpha, we obtain alpha=2.64+-0.27 (90%) and a residual rms scatter in log L_bol of 0.10. The derived relation can be directly compared to theoretical predictions that do not include radiative cooling. It also provides an accurate reference point for future evolution searches and comparison to cooler clusters. The new temperatures together with a newly selected cluster sample are used to update the temperature function at z~0.05. The resulting function is generally higher and flatter than the previous estimates by Edge et al (1990) and Henry & Arnaud (1991, corrected). For a qualitative estimate of constraints that the new data place on the density fluctuation spectrum, we apply the Press-Schechter formalism for Omega=1 and 0.3. For Omega=1, assuming cluster isothermality, the temperature function implies sigma_8=0.55+-0.03, while taking into account the observed cluster temperature profiles, sigma_8=0.51+-0.03, consistent with the previously derived range. The dependence of sigma_8 on Omega differs from earlier findings, because of our treatment of n as a free parameter. We find n=-(2.0-2.3)+-0.3, somewhat steeper than derived from the earlier temperature function data, in agreement with the local slope of the galaxy fluctuation spectrum from the APM survey, and significantly steeper than the standard CDM prediction.
Accepted for ApJ. Significand additions: Omega=0.3 model for the TF; a discussion of the TF derivation method; a comparison with recent Allen & Fabian L-T results. Latex, 8 pages, uses emulateapj.sty
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- Evaluating Tests of Virialization and Substructure Using Galaxy Clusters in the ORELSE Survey
- Large-scale variations of the cosmic X-ray background and the X-ray emissivity of the local Universe
- Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
- Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
- Relativistic Corrections to the Sunyaev-Zeldovich Effect for Clusters of Galaxies. V. Effect of the Motion of the Observer
- Chandra Observations of the X-ray Environment of BL Lacs
- The phase-diagram of the IGM and the entropy floor of groups and clusters: are clusters born warm?
- The X-ray-Optical Relations for Nine Clusters at z = 0.7-1.1
- Temperature and total mass profiles of the A3571 cluster of galaxies
- Star formation activity of intermediate redshift cluster galaxies out to the infall regions
- The Effect of Formation Redshifts on the Cluster Mass-Temperature Relation
- MCXC-II: Second release of the Meta-Catalogue of X-Ray detected Clusters of galaxies
- An X-ray underluminous cluster of galaxies in the 4Ms CDFS observations
- A low-redshift galaxy cluster X-ray Temperature Function incorporating Suzaku data
- Cosmological constraints from the cluster contribution to the power spectrum of the soft X-ray background. New evidence for a low sigma_8
- Measuring Ω_0 from the Entropy Evolution of Clusters
- Evidence for new physics from clusters ?
- Radial structure, inflow & central mass of stationary radiative galaxy clusters
- Spectroscopic confirmation of a cluster of galaxies at z=1 in the field of the gravitational lens MG2016+112
- Chandra Observations of the Gravitationally Lensed System 2016+112
- Lens or Binary? Chandra Observations of the Wide Separation Broad Absorption Line Quasar Pair UM425
- Mechanical heating by active galaxies
- The SZ Effect as a Probe of Non-Gravitational Entropy in Groups and Clusters of Galaxies
- Core Structure of Intracluster Gas: Isothermal Hydrostatic Equilibrium
- Intracluster Entropy from Joint X-ray and Sunyaev-Zel'dovich Observations
- Multi-fluid shocks in clusters of galaxies: entropy, sigma_ v-T, M-T and L_x-T scalings
- On cooling flows and the Sunyaev-Zel'dovich effect
- Chandra Observation of 3C288 - Reheating the Cool Core of a 3 keV Cluster from a Nuclear Outburst at z = 0.246
- The Universal Gas Mass Fraction in Clusters of Galaxies
- I. Analysis of candidates for interacting galaxy clusters
- Expectations for SZ cluster counts: mass function versus X-ray luminosity function
- Structure and evolution of magnetized clusters: entropy profiles, S-T and L_X-T relations
- ICM properties and AGN distribution in high-z RCS clusters
- The WARPS Survey. VIII. Evolution of the Galaxy Cluster X-ray Luminosity Function
- Constraints on the winds of hot subdwarf stars from X-ray observations of two sdB binaries with compact companions: CD -30 11223 and PG 1232-136
- X-ray Clusters of Galaxies as Cosmological Tools
- Serendipitous XMM-Newton discovery of a cluster of galaxies at z=0.28
- A metal-rich elongated structure in the core of the group NGC4325
- Halo Concentrations and the New Baseline X-ray Luminosity-Temperature and Mass Relations of Galaxy Clusters
- Dark matter distribution in galaxy groups from combined strong lensing and dynamics analysis
- The Halo Mass-Temperature Relation for Clusters, Groups, and Galaxies
- Preheating in the Universe Suppressing High Energy Gamma-rays from Structure Formation
- XMM-Newton observation of the cluster ZW 1305.4+2941 in the field SA 57
- Chandra Observation of the Cluster of Galaxies MS 0839.9+2938 at z=0.194: the Central Excess Iron and SN Ia Enrichment
- Implications of the Universal Temperature Profile for Galaxy Clusters
- Detecting preheating in proto-clusters with Lyman- Forest Tomography
- AXES-2MRS: A new all-sky catalogue of extended X-ray galaxy groups
- Excess entropy and energy feedback from within cluster cores up to r
- Cosmological Implications and Physical Properties of an X-Ray Flux-Limited Sample of Galaxy Clusters
- Cooling flows and the entropy of the intragroup medium
- Suppression of thermal conduction in non-cooling flow clusters
- Discovery of an absorbed cluster of galaxies (XMMU J183225.4-103645) close to the Galactic plane with XMM-Newton
- Constraints on structure formation models from Sunyaev-Zel'dovich Effect
- Scaling relations of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program Field
- An Evolving Entropy Floor in the Intracluster Gas?
- X-ray cluster cosmology
- Zw 1718.1-0108: a highly disturbed galaxy cluster at low Galactic latitude
- A Cluster of Galaxies hiding behind M31: XMM-Newton observations of RX J0046.4+4204
- The XMM Large-Scale Structure Survey: An initial sample of galaxy groups and clusters to a redshift z<0.6
- Extended X-ray emission in the radio loud galaxy 3C 382
- The X-Ray Zurich Environmental Study (X-ZENS). II. X-ray Observations of the Diffuse Intragroup Medium in Galaxy Groups
- Peering Into the Extended X-ray Emission on Megaparsec Scale in 3C 187
- Magnetic fields and Sunyaev-Zel'dovich effect in galaxy clusters
- The baryon mass function for galaxy clusters
- The Disturbed 17 keV Cluster Associated with the Radio Galaxy 3C 438
- Scaling Relation between Sunyaev-Zel'dovich Effect and X-ray Luminosity and Scale-Free Evolution of Cosmic Baryon Field
- Influence of AGN Outbursts on the Surrounding Galaxies
- Monte-Carlo Modeling of Non-Gravitational Heating Processes in Galaxy Clusters
- Chandra and HST Snapshots of Fossil System Progenitors
- Evolution of X-ray galaxy Cluster Properties in a Representative Sample (EXCPReS). Optimal binning for temperature profile extraction
- Joint cluster reconstructions: Combining free-form lensing and X-rays
- RXJ1648.7+6109: Witnessing the Formation of a Massive Group/Poor Cluster and its Brightest Galaxy
- SZ scaling relations in Galaxy Clusters: results from hydrodynamical N-body simulations
- Impact of supermassive black hole growth on star formation
- Average energy of the X-ray spectrum as a model-independent proxy for the mass of galaxy clusters
- Cooling and Clusters: When Is Heating Needed?
- X-ray Temperatures, Luminosities, and Masses From XMM-Newton Follow-up of the First Shear-selected Galaxy Cluster Sample
- Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
- The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to
- The Cluster LX-sigma Relation Has Implications for Scale-Free Cosmologies
- A test of linearity of the ratio of dark matter to baryonic matter in galaxy clusters
- Hydrostatic equilibrium of a porous intracluster medium: implications for mass fraction and X-ray luminosity
- The largest virialized dark halo in the universe
- Clusters of Galaxies: New Results from the CLEF Hydrodynamics Simulation
- Determination of the Linear Mass Power Spectrum From the Mass Function of Galaxy Clusters
- The impact of AGN on their host galaxies
- ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
- Fundamental parameters of FR II radio galaxies and their impact on groups and clusters' environments
- XMM-Newton view of MS0735+7421: the most energetic AGN outburst in a galaxy cluster
- The XMM-BCS galaxy cluster survey: I. The X-ray selected cluster catalog from the initial 6 deg
- The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the -- relation of early-type galaxies