A detection of the layered structure of nearby open clusters

被引:4
|
作者
Hu, Qingshun [1 ,2 ]
Zhang, Yu [1 ,2 ]
Esamdin, Ali [1 ,2 ]
Wang, Hong [1 ,2 ]
Qin, Mingfeng [1 ,2 ]
机构
[1] Chinese Acad Sci, Xinjiang Astron Observ, 150,Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
[2] Univ Chinese Acad Sci, 19 Yuquan Rd, Beijing 100049, Peoples R China
基金
中国国家自然科学基金; 国家重点研发计划;
关键词
methods: statistical; open clusters and associations: general; galaxies: stellar content; MASS SEGREGATION; EVOLUTION; !text type='PYTHON']PYTHON[!/text; SHAPE; PARAMETERS; MORPHOLOGY; DISTANCES; ASTROPY;
D O I
10.1051/0004-6361/202244199
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We applied the newly developed rose diagram overlay method to detect the layered structure of 88 nearby open clusters (=500pc) on the three projections after the distance correction of their member stars, based on the catalog in literature. The results show that with the rose diagram overlay method, a total of 74 clusters in our sample have a layered structure, while the remaining clusters are without a clear layered structure. We for the first time defined the layered structure parameters for the sample clusters. Meanwhile, we found that the layered circle core area (N) has a strong positive correlation with the number of cluster members, while the kernel instability index ($eta$) has a strong negative correlation with the number of cluster members. Our study provides a novel perspective for the detection of the layered structure of open clusters.
引用
收藏
页数:12
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