Warm-Hot Intergalactic Medium
Warm-Hot Intergalactic Medium
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DOI：
10.1017/9781108781596.011
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发表时间：
2005-02
期刊：
影响因子：
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通讯作者：
J. Hayes
中科院分区：
文献类型：
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作者：
J. Hayes
该补助金与LTSA的一项为期5年的补助金有关，该补助金的主题是“研究宇宙中最大的重子库：温热的星系际介质”。该方案第一年的工作非常丰富，已经产生了几项重要成果，详见本文。我们最初的提案理由表2列出了计划的逐年计划，分为两个子领域：（A）z=0（或本地组WHIM）系统的研究，以及（B）z大于0（即干预WHIM）系统的研究。对于这两个子领域中的每一个，我们计划在第一年分析一些存档（Chandra，XMM和FUSE）和新的（如果观察到）视线。此外，z=0系统的计划包括寻找新的有趣的视线。我们已经完成了所有这些任务。
This grant is associated to a 5-year LTSA grant, on "Studying the Largest Reservoir of Baryons in the Universe: The Warm-Hot Intergalactic Medium". The first year of work within this program has been very rich, and has already produced several important results, as detailed in this paper. Table 2 of our original proposal justification, listed the planned year-by-year program, divided into two sub-fields: (A) the study of the z=0 (or Local Group WHIM) system, and (B) the study of the z greater than 0 (i.e- intervening WHIM) systems. For each of the two sub-fields we had planned to analyze, in the first year, a number of archival (Chandra, XMM and FUSE) and new (if observed) sightlines. Moreover, the plan for the z=0 system included the search for new interesting sightlines. We have accomplished all these tasks.