中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
What X-rays tell us about dark matter halos

文献类型:期刊论文

作者Jing, YP; Ryder, SD; Pisano, DJ; Walker, MA; Freeman, KC
刊名DARK MATTER IN GALAXIES
出版日期2004
期号220页码:455-460
英文摘要We present a detailed non-spherical modeling of dark matter halos on the basis of a careful analysis of state-of-the art N-body simulations. The fitting formulae presented here form a complete and accurate description of the triaxial density profiles of halos in Cold Dark Matter (CDM) models. This modeling allows us to quantitatively discuss implications for shape observations of galactic and cluster halos. The predictions of the concordance ACDM model are confronted with the shape observations from the Milky Way to X-ray clusters.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]DENSITY PROFILES ; CLUSTERS
收录类别SCI ; ISTP
语种英语
WOS记录号WOS:000223027300099
源URL[http://119.78.226.72/handle/331011/18311]  
专题上海天文台_星系宇宙学重点实验室
作者单位MPI Astrophys, Shanghai Astron Observ, Partner Grp, Shanghai 200030, Peoples R China
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GB/T 7714
Jing, YP,Ryder, SD,Pisano, DJ,et al. What X-rays tell us about dark matter halos[J]. DARK MATTER IN GALAXIES,2004(220):455-460.
APA Jing, YP,Ryder, SD,Pisano, DJ,Walker, MA,&Freeman, KC.(2004).What X-rays tell us about dark matter halos.DARK MATTER IN GALAXIES(220),455-460.
MLA Jing, YP,et al."What X-rays tell us about dark matter halos".DARK MATTER IN GALAXIES .220(2004):455-460.

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来源:上海天文台

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