中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Loops formed by tidal tails as fossil records of a major merger

文献类型:期刊论文

作者Wang, J.1,2; Hammer, F.1; Athanassoula, E.3; Puech, M.1; Yang, Y.1,2; Flores, H.1
刊名ASTRONOMY & ASTROPHYSICS
出版日期2012-02-01
卷号538
关键词galaxies: evolution galaxies: spiral galaxies: individual: NGC 5907 galaxies: interactions
英文摘要Context. Many haloes of nearby disc galaxies contain faint and extended features, including loops, which are often interpreted as relics of satellite infall in the main galaxy's potential well. In most cases, however, the residual nucleus of the satellite is not seen, although it is predicted by numerical simulations.
收录类别SCI
语种英语
WOS记录号WOS:000300614100121
源URL[http://ir.bao.ac.cn/handle/114a11/6585]  
专题国家天文台_光学天文研究部
作者单位1.Univ Paris Diderot, Lab GEPI, Observ Paris, CNRS UMR8111, F-92195 Meudon, France
2.Chinese Acad Sci, NAOC, Beijing 100012, Peoples R China
3.Observ Astron Marseille Provence, Lab Astrophys Marseille, F-13388 Marseille 13, France
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GB/T 7714
Wang, J.,Hammer, F.,Athanassoula, E.,et al. Loops formed by tidal tails as fossil records of a major merger[J]. ASTRONOMY & ASTROPHYSICS,2012,538.
APA Wang, J.,Hammer, F.,Athanassoula, E.,Puech, M.,Yang, Y.,&Flores, H..(2012).Loops formed by tidal tails as fossil records of a major merger.ASTRONOMY & ASTROPHYSICS,538.
MLA Wang, J.,et al."Loops formed by tidal tails as fossil records of a major merger".ASTRONOMY & ASTROPHYSICS 538(2012).

入库方式: OAI收割

来源:国家天文台

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