中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The Spatial Distributions of Blue Main-sequence Stars in Magellanic Cloud Star Clusters

文献类型:期刊论文

作者Yang,Yujiao1,3,4,6,8; Li,Chengyuan1,4,7,8; de Grijs,Richard1,4; Deng,Licai2,5,8
刊名The Astrophysical Journal
出版日期2021-04-30
卷号912期号:1
关键词Magellanic Clouds Young star clusters HST photometry Stellar populations Binary stars
ISSN号0004-637X
DOI10.3847/1538-4357/abec4b
英文摘要Abstract The color–magnitude diagrams of young star clusters show that, particularly at ultraviolet wavelengths, their upper main sequences (MSs) bifurcate into a sequence comprising the bulk population and a blue periphery. The spatial distribution of stars is crucial to understanding the reasons for these distinct stellar populations. This study uses high-resolution photometric data obtained with the Hubble Space Telescope to study the spatial distributions of the stellar populations in seven Magellanic Cloud star clusters. The cumulative radial number fractions of blue stars within four clusters are strongly anticorrelated with those of the high mass ratio binaries in the bifurcated region, with negative Pearson coefficients
语种英语
WOS记录号IOP:0004-637X-912-1-ABEC4B
出版者The American Astronomical Society
源URL[http://ir.bao.ac.cn/handle/114a11/59189]  
专题中国科学院国家天文台
通讯作者Yang,Yujiao
作者单位1.Research Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia
2.School of Astronomy and Space Science, University of the Chinese Academy of Sciences, Huairou 101408, People's Republic of China
3.Kavli Institute for Astronomy & Astrophysics, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, People's Republic of China yujiaoyang@pku.edu.cn
4.Department of Physics and Astronomy, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia
5.Department of Astronomy, China West Normal University, Nanchong 637002, People's Republic of China
6.Department of Astronomy, School of Physics, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, People's Republic of China
7.School of Physics and Astronomy, Sun Yat-sen University, Zhuhai 519082, People's Republic of China; lichengy5@mail.sysu.edu.cn
8.Key Laboratory for Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China
推荐引用方式
GB/T 7714
Yang,Yujiao,Li,Chengyuan,de Grijs,Richard,et al. The Spatial Distributions of Blue Main-sequence Stars in Magellanic Cloud Star Clusters[J]. The Astrophysical Journal,2021,912(1).
APA Yang,Yujiao,Li,Chengyuan,de Grijs,Richard,&Deng,Licai.(2021).The Spatial Distributions of Blue Main-sequence Stars in Magellanic Cloud Star Clusters.The Astrophysical Journal,912(1).
MLA Yang,Yujiao,et al."The Spatial Distributions of Blue Main-sequence Stars in Magellanic Cloud Star Clusters".The Astrophysical Journal 912.1(2021).

入库方式: OAI收割

来源:国家天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。