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020 _a9780387788753
_99780387788753
024 7 _a10.1007/9780387788753
_2doi
035 _avtls000332966
039 9 _a201509030222
_bVLOAD
_c201404122319
_dVLOAD
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040 _aMX-SnUAN
_bspa
_cMX-SnUAN
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050 4 _aQB460-466
100 1 _aKaastra, Jelle.
_eeditor.
_9303429
245 1 0 _aClusters of Galaxies :
_bBeyond the Thermal View /
_cedited by Jelle Kaastra.
264 1 _aNew York, NY :
_bSpringer New York,
_c2008.
300 _brecurso en línea.
336 _atexto
_btxt
_2rdacontent
337 _acomputadora
_bc
_2rdamedia
338 _arecurso en línea
_bcr
_2rdacarrier
347 _aarchivo de texto
_bPDF
_2rda
500 _aSpringer eBooks
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.
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9780387788746
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-0-387-78875-3
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999 _c279228
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