KOR

e-Article

A detection of the layered structure of nearby open clusters
Document Type
Working Paper
Source
A&A 672, A12 (2023)
Subject
Astrophysics - Astrophysics of Galaxies
Astrophysics - Solar and Stellar Astrophysics
Language
Abstract
We applied the newly developed rose diagram overlay method to detect the layered structure of 88 nearby open clusters ($\leq$500~pc) on the three projections after the distance correction of their member stars, based on the catalog in literature. The results show that with the rose diagram overlay method, a total of 74 clusters in our sample have a layered structure, while the remaining clusters are without a clear layered structure. We for the first time defined the layered structure parameters for the sample clusters. Meanwhile, we found that the layered circle core area ($s$) has a strong positive correlation with the number of cluster members, while the kernel instability index ($\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.
Comment: 11 pages, 9 figures, 6 tables, accepted for publication in A&A