中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Molecular hydrogen as dark mass in dwarf galaxies

文献类型:期刊论文

作者Williams, PR; Marzok, C; Myers, S; Nelson, AH; Ryder, SD; Pisano, DJ; Walker, MA; Freeman, KC
刊名DARK MATTER IN GALAXIES
出版日期2004
期号220页码:251-252
英文摘要We report here an example of a series of computer simulations of the formation of disk galaxies, including a standard cold dark matter component, gas, and star formation, which result in objects which closely resemble observed giant galaxies, with a population of long-lived dwarf satellites which contain little or no non-baryonic dark matter.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]GAS
收录类别SCI ; ISTP
语种英语
WOS记录号WOS:000223027300050
源URL[http://119.78.226.72/handle/331011/18309]  
专题上海天文台_星系宇宙学重点实验室
作者单位Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
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GB/T 7714
Williams, PR,Marzok, C,Myers, S,et al. Molecular hydrogen as dark mass in dwarf galaxies[J]. DARK MATTER IN GALAXIES,2004(220):251-252.
APA Williams, PR.,Marzok, C.,Myers, S.,Nelson, AH.,Ryder, SD.,...&Freeman, KC.(2004).Molecular hydrogen as dark mass in dwarf galaxies.DARK MATTER IN GALAXIES(220),251-252.
MLA Williams, PR,et al."Molecular hydrogen as dark mass in dwarf galaxies".DARK MATTER IN GALAXIES .220(2004):251-252.

入库方式: OAI收割

来源:上海天文台

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