The Evolution of X-ray Clusters of Galaxies

Abstract

Considerable progress has been made over the last decade in the study of the evolutionary trends of the population of galaxy clusters in the Universe. In this review we focus on observations in the X-ray band. X-ray surveys with the ROSAT satellite, supplemented by follow-up studies with ASCA and Beppo-SAX, have allowed an assessment of the evolution of the space density of clusters out to z~1, and the evolution of the physical properties of the intra-cluster medium out to z~0.5. With the advent of Chandra and Newton-XMM, and their unprecedented sensitivity and angular resolution, these studies have been extended beyond redshift unity and have revealed the complexity of the thermodynamical structure of clusters. The properties of the intra-cluster gas are significantly affected by non-gravitational processes including star formation and Active Galactic Nucleus (AGN) activity. Convincing evidence has emerged for modest evolution of both the bulk of the X-ray cluster population and their thermodynamical properties since redshift unity. Such an observational scenario is consistent with hierarchical models of structure formation in a flat low density universe with Omega_m=0.3 and sigma_8=0.7-0.8 for the normalization of the power spectrum. Basic methodologies for construction of X-ray-selected cluster samples are reviewed and implications of cluster evolution for cosmological models are discussed.

40 pages, 15 figures. Full resolution figures can be downloaded from http://www.eso.org/~prosati/ARAA/

References in corpus (21)

• The Mass Function of an X-Ray Flux-Limited Sample of Galaxy Clusters
• The Chandra Deep Field South: the 1 Million Second
• Cosmological Parameter Extraction from the First Season of Observations with DASI
• Measuring ${\Omega }_m$ with the ROSAT Deep Cluster Survey
• A JavaScript Passive Evolution Calculator
• The X-ray virial relations for relaxed lensing clusters observed with Chandra
• Cosmological implications of the MAXIMA-I high resolution Cosmic Microwave Background anisotropy measurement
• The most distant structure of galaxies known: a protocluster at z=4.1
• Regulation of the X-ray luminosity of clusters of galaxies by cooling and supernova feedback
• The New Emerging Model for the Structure of Cooling Cores in Clusters of Galaxies
• A Systematic Study of X-Ray Substructure of Galaxy Clusters Detected in the ROSAT All-Sky Survey
• Detecting Clusters of Galaxies in the Sloan Digital Sky Survey I : Monte Carlo Comparison of Cluster Detection Algorithms
• The Las Campanas Distant Cluster Survey - The Catalog
• Constraining the Matter Power Spectrum Normalization using the SDSS/RASS and REFLEX Cluster surveys
• Pre-heating the ICM in high resolution simulations: the effect on the gas entropy
• The 2dF Galaxy Redshift Survey: A targeted study of catalogued clusters of galaxies
• An X-ray Selected Galaxy Cluster at z=1.11 in the Rosat Deep Cluster Survey
• Distant Cluster Hunting I: A Comparison Between the Optical and X-ray Luminosity Functions from an Optical/X-ray Survey
• Chandra X-Ray Observatory Observation of the High-Redshift Cluster MS 1054-0321
• Heating of Intracluster Gas by Jet Activities of AGN: Is the "Preheating" Scenario Realistic?
• XMM-Newton Observation of a Distant X-ray Selected Cluster of Galaxies at z=1.26 with Possible Cluster Interaction

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