標(biāo)題: Titlebook: Clusters of Galaxies: Beyond the Thermal View; Jelle Kaastra Book 2008 Springer-Verlag New York 2008 Galaxy.chemical evolution.clusters of [打印本頁] 作者: lutein 時間: 2025-3-21 19:16
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書目名稱Clusters of Galaxies: Beyond the Thermal View影響因子(影響力)學(xué)科排名
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書目名稱Clusters of Galaxies: Beyond the Thermal View網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Clusters of Galaxies: Beyond the Thermal View被引頻次
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書目名稱Clusters of Galaxies: Beyond the Thermal View年度引用學(xué)科排名
書目名稱Clusters of Galaxies: Beyond the Thermal View讀者反饋
書目名稱Clusters of Galaxies: Beyond the Thermal View讀者反饋學(xué)科排名
作者: 鬧劇 時間: 2025-3-22 00:15 作者: Mortal 時間: 2025-3-22 02:55 作者: accessory 時間: 2025-3-22 08:15
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.作者: NICHE 時間: 2025-3-22 10:04
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.作者: 引起痛苦 時間: 2025-3-22 13:47
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.作者: 引起痛苦 時間: 2025-3-22 17:36
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.作者: 值得尊敬 時間: 2025-3-23 00:56
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?..作者: SOB 時間: 2025-3-23 04:32
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.作者: genesis 時間: 2025-3-23 09:01 作者: SPASM 時間: 2025-3-23 11:17
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?..作者: Expurgate 時間: 2025-3-23 17:49 作者: 詼諧 時間: 2025-3-23 18:17 作者: 屈尊 時間: 2025-3-23 23:41
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. 作者: 亂砍 時間: 2025-3-24 03:17 作者: 做作 時間: 2025-3-24 10:32 作者: 侵略者 時間: 2025-3-24 14:06
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.作者: altruism 時間: 2025-3-24 18:16 作者: Mercantile 時間: 2025-3-24 21:59 作者: Congruous 時間: 2025-3-25 01:51 作者: BADGE 時間: 2025-3-25 07:02 作者: 拋物線 時間: 2025-3-25 10:48 作者: Seminar 時間: 2025-3-25 13:06 作者: 慷慨援助 時間: 2025-3-25 16:07 作者: 有危險 時間: 2025-3-25 20:58
Schriftenreihe Neurologie‘ Neurology Seriester space. This emission is likely to be nonthermal, probably resulting from Compton scattering of relativistic electrons by the cosmic microwave background (CMB) radiation. Direct evidence for the presence of relativistic electrons in some 50 clusters comes from measurements of extended radio emiss作者: 暴發(fā)戶 時間: 2025-3-26 01:42 作者: 輕快帶來危險 時間: 2025-3-26 06:47
Zur Lebersch?digung Durch Halothannergy of gravitationally accelerated flows to internal energy of the gas. Being the main gas-heating agent, cosmological shocks could amplify magnetic fields and accelerate energetic particles via the multi-fluid plasma relaxation processes. We first discuss the basic properties of standard single-f作者: 剛毅 時間: 2025-3-26 08:46 作者: BLOT 時間: 2025-3-26 15:39 作者: 弓箭 時間: 2025-3-26 19:48 作者: Ballad 時間: 2025-3-26 23:56 作者: Discrete 時間: 2025-3-27 03:46 作者: overrule 時間: 2025-3-27 08:39
https://doi.org/10.1007/978-3-8348-9924-8ing the cosmological history of the hierarchical build up of galaxy clusters. In this paper we review the current status of these simulations and how their predictions fare in reproducing the most recent X-ray observations of clusters. After briefly discussing the shortcomings of the self-similar mo作者: cringe 時間: 2025-3-27 11:21 作者: fibula 時間: 2025-3-27 13:58
Akute Vergiftungen durch sonstige Giftgasescale turbulence are unavoidable in the cluster formation processes. Understanding the amplification and evolution of the magnetic field in galaxy clusters is necessary for modelling both the heat transport and the dissipative processes in the hot intra-cluster plasma. The acceleration, transport an作者: 少量 時間: 2025-3-27 20:57
Zahlenwerte zur Physiologie der Atmungxies. Most of these metals reside in the hot plasma which dominates the baryon content of clusters. This makes them excellent laboratories for the study of the nucleosynthesis and chemical enrichment history of the Universe. Here we review the history, current possibilities and limitations of the ab作者: 鋼盔 時間: 2025-3-27 22:40 作者: 規(guī)范就好 時間: 2025-3-28 06:11
Sch?dliche Nebenwirkungen von Arzneimittelny of star formation, the role of feedback processes and the gas-dynamical processes which determine the evolution of the cosmic baryons. In this paper we review the approaches that have been followed so far to model the enrichment of the ICM in a cosmological context. While our presentation will be 作者: Haphazard 時間: 2025-3-28 09:31 作者: 強行引入 時間: 2025-3-28 13:59
Sch?dliche Nebenwirkungen von ArzneimittelnWe briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.作者: debble 時間: 2025-3-28 14:58 作者: DRILL 時間: 2025-3-28 21:27 作者: 放棄 時間: 2025-3-29 00:36 作者: Entreaty 時間: 2025-3-29 05:28 作者: 格子架 時間: 2025-3-29 07:20
http://image.papertrans.cn/c/image/228569.jpg作者: craven 時間: 2025-3-29 14:18 作者: Banister 時間: 2025-3-29 16:46
Clusters of Galaxies: Setting the Stage,rrelation between the dynamical and morphological properties of irregular clusters and the surrounding large-scale structure increase with redshift..In the current bottom-up scenario for the formation of cosmic structure, where tiny fluctuations of the otherwise homogeneous primordial density field 作者: 割讓 時間: 2025-3-29 22:42 作者: 窒息 時間: 2025-3-30 01:32 作者: 以煙熏消毒 時間: 2025-3-30 04:12
Equilibration Processes in the Warm-Hot Intergalactic Medium,opic 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作者: NORM 時間: 2025-3-30 11:05
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作者: 微塵 時間: 2025-3-30 14:16 作者: 有花 時間: 2025-3-30 20:34 作者: 混合物 時間: 2025-3-31 00:36
,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作者: 特征 時間: 2025-3-31 04:10
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—作者: 配置 時間: 2025-3-31 06:56 作者: anesthesia 時間: 2025-3-31 12:35 作者: 揭穿真相 時間: 2025-3-31 14:04 作者: 牌帶來 時間: 2025-3-31 20:22
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作者: Rejuvenate 時間: 2025-4-1 00:22
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作者: 狂怒 時間: 2025-4-1 02:22
Zur Lebersch?digung Durch Halothanectrons from the background plasma with an initial Maxwellian distribution. For acceleration rates smaller than the Coulomb energy loss rate, the effect of energising the plasma is to primarily heat the plasma with little sign of a distinct non-thermal tail. Such tails are discernible only for accel作者: BLA 時間: 2025-4-1 07:18 作者: 槍支 時間: 2025-4-1 10:14 作者: prolate 時間: 2025-4-1 15:21
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—978-1-4419-2702-6978-0-387-78875-3作者: intolerance 時間: 2025-4-1 22:24
Clusters of Galaxies: Beyond the Thermal View,servational and theoretical status of the non-virialised X-ray emission components in clusters of galaxies. The subject is important for the study of large-scale hierarchical structure formation and to shed light on the “missing baryon” problem. The topics of the team work include thermal emission a
