Clusters of Galaxies: Beyond the Thermal View
Clusters of galaxies are the largest structures in the Universe. Most of the visible matter is in the form of hot gas permeating the volume of the cluster. The bulk of this gas is in thermal equilibrium in the dark matter-dominated potential. This book discusses all aspects of cluster physics beyond...
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| Language: | English |
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New York, NY :
Springer New York : Imprint: Springer,
2008.
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| Edition: | 1st ed. 2008. |
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| Online Access: | https://doi.org/10.1007/978-0-387-78875-3 |
Table of Contents:
- Clusters of Galaxies: Beyond the Thermal View
- Clusters of Galaxies: Setting the Stage
- FUV and X-Ray Absorption in the Warm-Hot Intergalactic Medium
- Soft X-Ray and Extreme Ultraviolet Excess Emission from Clusters of Galaxies
- Nonthermal Phenomena in Clusters of Galaxies
- Observations of Extended Radio Emission in Clusters
- Cosmological Shock Waves
- Equilibration Processes in the Warm-Hot Intergalactic Medium
- Thermal Radiation Processes
- Nonthermal Radiation Mechanisms
- Particle Acceleration Mechanisms
- Simulation Techniques for Cosmological Simulations
- Thermodynamical Properties of the ICM from Hydrodynamical Simulations
- Numerical Simulations of the Warm-Hot Intergalactic Medium
- Non-Thermal Processes in Cosmological Simulations
- Observations of Metals in the Intra-Cluster Medium
- Metal Enrichment Processes
- The Chemical Enrichment of the ICM from Hydrodynamical Simulations
- Future Instrumentation for the Study of the Warm-Hot Intergalactic Medium.