Cosmological Aspects of X-Ray Clusters of Galaxies

The NATO Advanced Study Institute "Cosmological Aspects of X-Ray Clus­ ters of Galaxies" took place in Vel en , Westphalia, Germany, from June 6 to June 18, 1993. It addressed the fruitful union of two topics, cosmology and X-ray clus­ ters, both of which carry substantial scientific weigh...

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Bibliographic Details
Other Authors: Seitter, W.C. (Editor)
Format: eBook
Language:English
Published: Dordrecht Springer Netherlands 1994, 1994
Edition:1st ed. 1994
Series:Nato Science Series C:, Mathematical and Physical Sciences
Subjects:
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
Table of Contents:
  • Inflation and the Origin of Large-Scale Potential Perturbations
  • Einstein Observatory Evidence for a Widespread Baryon Overdensity in Clusters of Galaxies
  • Evidence for High? From Large scale Structure
  • X-Ray Clusters: Constraints on Cosmological Parameters
  • Cosmological Implications of the Distribution of Quasar Forest Lines
  • Author Index
  • Object Index
  • Constraint on Galaxy Formation Theories from X-Ray Clusters
  • Evolution of the X-Ray Properties of Clusters of Galaxies
  • The Structure and Evolution of Clusters
  • Galaxy Formation in Galaxy Clusters: A Phenomenological Approach
  • X-Ray Clusters in the Sculptor Supercluster
  • Constraints on Models of Large-Scale Structure Formation
  • A2163: An Exceptionally Hot Cluster of Galaxies
  • X-Ray Clusters of Galaxies in CDM Cosmogony
  • 7. Large-Scale Structure
  • So Many Galaxies, so Little Time
  • A Census of Optically-Selected Clusters
  • The Spatial Correlation Function of Galaxy Clusters: Optical to X-Ray
  • A Search for Galaxy Alignment in the Hercules Supercluster
  • A Redshift Survey of the Corona Borealis Supercluster
  • 8. Structure and Cosmological Parameters
  • A Map with a Scale: The Las Campanas Redshift Survey
  • Large-Scale Structures from Low-Resolution Redshift Surveys
  • The Muenster Redshift Project
  • A Model-Independent Method to Determine the Mass in Clusters of Galaxies
  • Simulating the Dynamics of the Virgo Cluster
  • ROSAT Observation of Abell 1795: Temperature Profile — Gravitating, Gas, and Galaxy Mass Distribution — Cooling Flow
  • 4. Cooling Flows and Chemical Abundances
  • Cluster Cooling Flows
  • The Optical Properties of Central Cluster Galaxies in Cooling Flows
  • 2-D Numerical Simulations of Hot Gas Deposition in Cooling Flows
  • X-Ray Spectroscopy of Galaxy Clusters
  • 5. Cluster Lensing and Sunyaev-ZePdovich Effect
  • Cluster Lenses and Dark Matter Distribution in Clusters of Galaxies
  • Using Gravitational Lensing to Test the Pressure-Supported Hot Intracluster Gas Hypothesis in A2218
  • PRONAOS-SPM: A Balloon-Borne Experiment Well Adapted to Measure the Short Wavelength Part of the Sunyaev-Zel’dovich Effect
  • 6.Cluster Formation and Evolution
  • Formation and Evolution of Clusters as Dynamical Structures
  • 1. The Present and the Past of X-Ray Astronomy
  • ROSAT Three Years in Orbit
  • X-Ray Emission from Clusters of Galaxies
  • The First Decade of X-Ray Astronomy — A Personal View
  • 2. X-Ray Clusters and Cluster Environments
  • Galaxy Environment and Clusters of Galaxies
  • X-Ray Imaging Observations of Clusters of Galaxies
  • X-Ray Studies of Compact Galaxy Groups
  • Combined X-Ray/Radio/Optical Observations of ROSAT Clusters of Galaxies
  • ROSAT Detections at High Redshift
  • X-Ray Emission from a Complete Sample of Abell Clusters of Galaxies
  • Substructure in ABCG 2256: Wavelet Analysis of ROSAT Image
  • Pointed ROSAT Observations of Clusters of Galaxies
  • Dark Matter Distribution in X-Ray Clusters of Galaxies
  • X-Ray Emission from a Simulated Cluster of Galaxies
  • Luminosity Segregation in cD Clusters and Relevant Implications
  • 3. Cluster Masses and Dynamics
  • The Masses of Clusters of Galaxies
  • The Mass Distribution(s) in Clusters of Galaxies