中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metalicity gradients

文献类型:期刊论文

作者Pasetto, S.1,2; Grebel, E. K.1; Berczik, P.1,3,4; Spurzem, R.1,3,5; Dehnen, W.6
刊名ASTRONOMY & ASTROPHYSICS
出版日期2010-05-01
卷号514
关键词galaxies: dwarf galaxies: formation galaxies: evolution galaxies: kinematics and dynamics galaxies: abundances
英文摘要The chemodynamical evolution of spherical multi-component self-gravitating models for isolated dwarf galaxies is studied. We compared their evolution with and without feedback effects from star formation processes. We found that initially cuspy dark matter profiles flatten with time without any special tuning conditions as a result of star formation. Thus the seemingly flattened profiles found in many dwarfs do not contradict the cuspy profiles predicted by cosmological models. We also calculated the chemical evolution of stars and gas, to permit comparisons with observational data.
收录类别SCI
语种英语
WOS记录号WOS:000280504800014
源URL[http://ir.bao.ac.cn/handle/114a11/7638]  
专题国家天文台_星系宇宙学研究部
作者单位1.Univ Heidelberg, Zentrum Astron, Astron Rechen Inst, D-69117 Heidelberg, Germany
2.Max Planck Inst Astron, D-69117 Heidelberg, Germany
3.Chinese Acad Sci, NAOC, Beijing 100012, Peoples R China
4.NASU, MAO, UA-03680 Kiev, Ukraine
5.Peking Univ, Kavli Inst Astron & Astrophys, Beijing, Peoples R China
6.Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
推荐引用方式
GB/T 7714
Pasetto, S.,Grebel, E. K.,Berczik, P.,et al. Isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metalicity gradients[J]. ASTRONOMY & ASTROPHYSICS,2010,514.
APA Pasetto, S.,Grebel, E. K.,Berczik, P.,Spurzem, R.,&Dehnen, W..(2010).Isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metalicity gradients.ASTRONOMY & ASTROPHYSICS,514.
MLA Pasetto, S.,et al."Isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metalicity gradients".ASTRONOMY & ASTROPHYSICS 514(2010).

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来源:国家天文台

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