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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Numerical Simulations of the Warm-Hot Intergalactic Medium,ch as . and . do not have enough sensitivity to detect the hotter WHIM. However, future missions such as . and . might be able to detect both emission lines and absorption systems from highly ionised atoms such as O?., O?. and Fe?..

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Book 2008emission from hot intracluster gas (hereafter the ICM) has been claimed since 1996. Soft excesses are particularly - portant to detect because they may (at least partly) be due to thermal emission from the Warm-Hot Intergalactic Medium, where as much as half of the baryons of the Universe could be.

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Zahlenwerte zur Physiologie der Atmunglatest progress in using the abundance patterns in clusters to put constraints on theoretical models of supernovae and we show how cluster abundances provide new insights into the star-formation history of the Universe.

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