中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Deep near-infrared imaging of W3 Main: constraints on stellar cluster formation

文献类型:期刊论文

作者Bik, A.1; Stolte, A.2; Gennaro, M.1,3; Brandner, W.1; Gouliermis, D.1,4; Hussmann, B.2; Tognelli, E.5; Rochau, B.1; Henning, Th.1; Adamo, A.1
刊名ASTRONOMY & ASTROPHYSICS
出版日期2014
卷号561期号:0页码:0
关键词stars: luminosity function, mass function infrared: stars open clusters and associations: individual: W3 Main stars: pre-main sequence
ISSN号0004-6361
英文摘要Context. Embedded clusters like W3 Main are complex and dynamically evolving systems that represent an important phase in the star formation process.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]INITIAL MASS FUNCTION ; STAR-FORMING REGION ; GIANT MOLECULAR CLOUD ; H-II REGIONS ; INTERSTELLAR EXTINCTION LAW ; PROTOPLANETARY DISKS ; MAGELLANIC-CLOUD ; RADIO-CONTINUUM ; ARCHES CLUSTER ; SEGREGATION
收录类别SCI
原文出处10.1051/0004-6361/201321957
语种英语
WOS记录号WOS:000330584000012
公开日期2014-11-20
源URL[http://libir.pmo.ac.cn/handle/332002/10618]  
专题紫金山天文台_南极天文中心
作者单位1.Max Planck Inst Astron, D-69117 Heidelberg, Germany
2.Argelander Inst Astron, D-53121 Bonn, Germany
3.Space Telescope Sci Inst, Baltimore, MD 21218 USA
4.Heidelberg Univ, Zentrum Astron, Inst Theoret Astrophys, D-69120 Heidelberg, Germany
5.Univ Pisa, Dept Phys, I-56127 Pisa, Italy
6.Heidelberg Univ, Zentrum Astron, Astronom Rechen Inst, D-69120 Heidelberg, Germany
7.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
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GB/T 7714
Bik, A.,Stolte, A.,Gennaro, M.,et al. Deep near-infrared imaging of W3 Main: constraints on stellar cluster formation[J]. ASTRONOMY & ASTROPHYSICS,2014,561(0):0.
APA Bik, A..,Stolte, A..,Gennaro, M..,Brandner, W..,Gouliermis, D..,...&Wang, Y..(2014).Deep near-infrared imaging of W3 Main: constraints on stellar cluster formation.ASTRONOMY & ASTROPHYSICS,561(0),0.
MLA Bik, A.,et al."Deep near-infrared imaging of W3 Main: constraints on stellar cluster formation".ASTRONOMY & ASTROPHYSICS 561.0(2014):0.

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来源:紫金山天文台

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