Buch, Englisch, Band 72, 535 Seiten, Paperback, Format (B × H): 155 mm x 235 mm, Gewicht: 936 g
Buch, Englisch, Band 72, 535 Seiten, Paperback, Format (B × H): 155 mm x 235 mm, Gewicht: 936 g
Reihe: Space Sciences Series of ISSI
ISBN: 978-94-024-1736-4
Verlag: Springer Netherlands
Clusters of galaxies are large assemblies of galaxies, hot gas and dark matter bound together by gravity. Galaxy clusters are now one of the most important cosmological probes to test the standard cosmological models. Constraints on the Dark Energy equation of state from the cluster number density measurements, deviations from the Gaussian perturbation models, the Sunyaev-Zeldovich effect as well as the dark matter proles are among the issues to be studied with clusters. The baryonic composition of clusters is dominated by hot gas that is in quasi-hydrostatic equilibrium within the dark matter-dominated gravitational potential well of the cluster. The hot gas is visible through spatially extended thermal X-ray emission, and it has been studied extensively both for assessing its physical properties and as a tracer of the large-scale structure of the Universe. Magnetic fields as well as a number of non-thermal plasma processes play a role in clusters of galaxies as we observe from radioastronomical observations.
The goal of this volume is to review these processes and to investigate how they are interlinked. Overall, these papers provide a timely and comprehensive review of the multi-wavelength observations and theoretical understanding of clusters of galaxies in the cosmological context. Thus, the volume will be particularly useful to postgraduate students and researchers active in various areas of astrophysics and space science.
Originally published in Space Science Reviews in the Topical Collection "Clusters of Galaxies: Physics and Cosmology"
Zielgruppe
Research
Autoren/Hrsg.
Fachgebiete
- Naturwissenschaften Astronomie Astrophysik
- Naturwissenschaften Astronomie Kosmologie, Urknalltheorie
- Naturwissenschaften Astronomie Astronomische Beobachtung: Observatorien, Instrumente, Methoden
- Naturwissenschaften Physik Thermodynamik Plasmaphysik
- Naturwissenschaften Physik Angewandte Physik Astrophysik
Weitere Infos & Material
Preface.- The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population.- X-Ray Spectroscopy of Galaxy Clusters: Beyond the CIE Modeling.- Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects.- Diffuse Radio Emission from Galaxy Clusters.- Hot Atmospheres, Cold Gas, AGN Feedback and the Evolution of Early Type Galaxies: A Topical Perspective.- Constraining Gas Motions in the Intra-Cluster Medium.- The Physics of Galaxy Cluster Outskirts.- Enrichment of the Hot Intracluster Medium: Observations.- 10. Enrichment of the Hot Intracluster Medium: Numerical Simulations.- Magnetic Field Amplification in Galaxy Clusters and Its Simulation.- Shocks and Non-thermal Particles in Clusters of Galaxies.