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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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發(fā)表于 2025-3-21 19:16:04 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Clusters of Galaxies: Beyond the Thermal View
編輯Jelle Kaastra
視頻videohttp://file.papertrans.cn/229/228569/228569.mp4
概述Focuses on the warm-hot intergalactic medium and non-thermal aspects of clusters.Contains a tutorial review about these topics.Takes an approach from observational, theoretical, and numerical modeling
圖書封面Titlebook: Clusters of Galaxies: Beyond the Thermal View; Jelle Kaastra Book 2008 Springer-Verlag New York 2008 Galaxy.chemical evolution.clusters of
描述The existence of soft excess emission originating from clusters of galaxies, de ned as em- sion detected below 1 keV in excess over the usual thermal emission 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. They are therefore of fundamental cosmological importance. Soft excess emission has been observed (and has also given rise to controversy) in a number of clusters, mainly raising the following questions: (1) Do clusters really show a soft excess? (2) If so, from what spatial region(s) of the cluster does the soft excess or- inate? (3) Is this excess emission thermal, originating from warm-hot intergalactic gas (at 6 temperatures of?10 K), or non-thermal, 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—
出版日期Book 2008
關(guān)鍵詞Galaxy; chemical evolution; clusters of galaxies; non-thermal processes; warm hot intergalactic medium; w
版次1
doihttps://doi.org/10.1007/978-0-387-78875-3
isbn_softcover978-1-4419-2702-6
isbn_ebook978-0-387-78875-3
copyrightSpringer-Verlag New York 2008
The information of publication is updating

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Eigene experimentelle Untersuchungen,a and Suzaku) and their corresponding instrumental issues, which are responsible for the fact that this soft excess remains controversial in a number of cases. We then review the evidence for this soft X-ray excess and discuss the possible mechanisms (thermal and non-thermal) which could be responsible for this emission.
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Soft X-Ray and Extreme Ultraviolet Excess Emission from Clusters of Galaxies,a and Suzaku) and their corresponding instrumental issues, which are responsible for the fact that this soft excess remains controversial in a number of cases. We then review the evidence for this soft X-ray excess and discuss the possible mechanisms (thermal and non-thermal) which could be responsible for this emission.
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Einführung in die Sch?delbasischirurgieseries of review papers on this subject. These reviews are intended as introductory text and reference for scientists wishing to work actively in this field. The team consists of sixteen experts in observations, theory and numerical simulations.
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Teratogene Sch?den Durch Narkotikaydrodynamic codes based on both particle methods that discretise mass, and grid-based methods. We briefly describe Eulerian grid methods, and also some variants of Lagrangian smoothed particle hydrodynamics (.) methods.
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https://doi.org/10.1007/978-3-8348-9924-8ch 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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Clusters of Galaxies: Beyond the Thermal View,series of review papers on this subject. These reviews are intended as introductory text and reference for scientists wishing to work actively in this field. The team consists of sixteen experts in observations, theory and numerical simulations.
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