000			03091nam a22004095i 4500
001			978-0-387-78875-3
003			DE-He213
005			20251006084420.0
007			cr nn 008mamaa
008			100301s2008 xxu| s |||| 0|eng d
020			_a9780387788753
020			_a99780387788753
024	7		_a10.1007/978-0-387-78875-3 _2doi
082	0	4	_a523.01 _223
100	1		_aKaastra, Jelle. _eeditor.
245	1	0	_aClusters of Galaxies _h[electronic resource] : _bBeyond the Thermal View / _cedited by Jelle Kaastra.
264		1	_aNew York, NY : _bSpringer New York, _c2008.
300			_bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
505	0		_aClusters 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			_aClusters 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	_aPHYSICS.
650		0	_aASTROPHYSICS.
650	1	4	_aPHYSICS.
650	2	4	_aASTROPHYSICS.
650	2	4	_aEXTRATERRESTRIAL PHYSICS, SPACE SCIENCES.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9780387788746
856	4	0	_uhttp://dx.doi.org/10.1007/978-0-387-78875-3 _zVer el texto completo en las instalaciones del CICY
912			_aZDB-2-PHA
942			_2ddc _cER
999			_c59117 _d59117