SPASM
发表于 2025-3-23 11:17:22
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 ..
Expurgate
发表于 2025-3-23 17:49:50
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诙谐
发表于 2025-3-23 18:17:02
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屈尊
发表于 2025-3-23 23:41:03
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.
乱砍
发表于 2025-3-24 03:17:59
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做作
发表于 2025-3-24 10:32:13
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侵略者
发表于 2025-3-24 14:06:04
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.
altruism
发表于 2025-3-24 18:16:52
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Mercantile
发表于 2025-3-24 21:59:15
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Congruous
发表于 2025-3-25 01:51:01
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