Issue |
A&A
Volume 672, April 2023
|
|
---|---|---|
Article Number | A12 | |
Number of page(s) | 12 | |
Section | Galactic structure, stellar clusters and populations | |
DOI | https://doi.org/10.1051/0004-6361/202244199 | |
Published online | 23 March 2023 |
A detection of the layered structure of nearby open clusters
1
Xinjiang Astronomical Observatory, Chinese Academy of Sciences, No. 150, Science 1 Street, Urumqi, Xinjiang 830011, PR China
e-mail: zhy@xao.ac.cn; aliyi@xao.ac.cn
2
University of Chinese Academy of Sciences, 19 Yuquan Road, Shijingshan District, Beijing 100049, PR China
Received:
7
June
2022
Accepted:
30
January
2023
We applied the newly developed rose diagram overlay method to detect the layered structure of 88 nearby open clusters (≤500 pc) 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 (s) has a strong positive correlation with the number of cluster members, while the kernel instability index (η) 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.
Key words: methods: statistical / open clusters and associations: general / galaxies: stellar content
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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