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...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Άλλοι συγγραφείς: Kaastra, Jelle (Επιμελητής έκδοσης)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: New York, NY : Springer New York, 2008.
Θέματα:
Διαθέσιμο Online:Full Text via HEAL-Link
LEADER 03174nam a22004335i 4500
001 978-0-387-78875-3
003 DE-He213
005 20151204185129.0
007 cr nn 008mamaa
008 100301s2008 xxu| s |||| 0|eng d
020 |a 9780387788753  |9 978-0-387-78875-3 
024 7 |a 10.1007/978-0-387-78875-3  |2 doi 
040 |d GrThAP 
050 4 |a QB460-466 
072 7 |a PHVB  |2 bicssc 
072 7 |a SCI005000  |2 bisacsh 
082 0 4 |a 523.01  |2 23 
245 1 0 |a Clusters of Galaxies  |h [electronic resource] :  |b Beyond the Thermal View /  |c edited by Jelle Kaastra. 
264 1 |a New York, NY :  |b Springer New York,  |c 2008. 
300 |a IV, 418 p.  |b online resource. 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
347 |a text file  |b PDF  |2 rda 
505 0 |a 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. 
520 |a 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 this thermal view. It covers topics such as the warm-hot intergalactic medium outside the clusters, non-thermal radiation components, shocks, equilibration processes and the chemical evolution of these structures. The topics are covered from an observational, theoretical and numerical point of view. This volume provides a useful reference for astronomers and graduate students, in particular for those who are working in high-energy astrophysics and extra-galactic astronomy. 
650 0 |a Physics. 
650 0 |a Astrophysics. 
650 0 |a Space sciences. 
650 1 4 |a Physics. 
650 2 4 |a Astrophysics and Astroparticles. 
650 2 4 |a Extraterrestrial Physics, Space Sciences. 
700 1 |a Kaastra, Jelle.  |e editor. 
710 2 |a SpringerLink (Online service) 
773 0 |t Springer eBooks 
776 0 8 |i Printed edition:  |z 9780387788746 
856 4 0 |u http://dx.doi.org/10.1007/978-0-387-78875-3  |z Full Text via HEAL-Link 
912 |a ZDB-2-PHA 
950 |a Physics and Astronomy (Springer-11651)