An illuminating dark halo

被引：0
|
作者：
Stéphane Colombi
机构：
[1] Stéphane Colombi is at the Institut d'Astrophysique de Paris,
[2] CNRS UMR 7095/Université Pierre et Marie Curie,undefined
[3] 98 bis boulevard Arago,undefined
[4] 75014 Paris,undefined
[5] France. colombi@iap.fr ,undefined
来源：
Nature | 2008年 / 456卷
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学科分类号：
摘要：
A large simulation reveals that most of the detectable signal from dark matter in our Milky Way probably comes from the main, smooth Galactic halo, rather than from small clumps.
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页码：44 / 45
页数：1
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