Titlebook: Clusters of Galaxies: Beyond the Thermal View; Jelle Kaastra Book 2008 Springer-Verlag New York 2008 Galaxy.chemical evolution.clusters of

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Nonthermal Radiation Mechanisms,value of the magnetic field and energy of relativistic electrons. This model requires a low value of the magnetic field which is far from the equipartition value. We briefly review the possibilities of gamma-ray emission and prospects for . observations. We also present a toy model of the non-therma

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有花

混合物

,The Chemical Enrichment of the ICM from?Hydrodynamical Simulations,function, on the stellar life-times and on the stellar yields. We will then overview the comparisons presented so far between X-ray observations of the ICM enrichment and model predictions. We will show how the most recent chemo-dynamical models are able to capture the basic features of the observed

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Book 2008thermal, in which case several emission mechanisms have been proposed. Interestingly, some of the non-thermal mechanisms suggested to account for soft excess emission can also explain the hard X-ray emission detected in some clusters, for example by RXTE and BeppoSAX (also see Petrosian et al. 2008—

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anesthesia

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Teratogene Sch?den Durch Narkotikaopic temperatures and a large differences in ion and electron temperatures. We discuss the ion and electron heating by the collisionless shocks and then review the plasma processes responsible for the Coulomb equilibration and collisional ionisation equilibrium of oxygen ions in the WHIM. MHD-turbul

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Zur Lebersch?digung Durch Halothanvalue of the magnetic field and energy of relativistic electrons. This model requires a low value of the magnetic field which is far from the equipartition value. We briefly review the possibilities of gamma-ray emission and prospects for . observations. We also present a toy model of the non-therma