Determination of dynamical ages of open clusters through the A$^+$ parameter -- II
Khushboo K. Rao (1), Kaushar Vaidya (1), Manan Agarwal (2), Shanmugha, Balan (1), and Souradeep Bhattacharya (3), ((1) Department of physics, Birla, Institute of Technology, Science-Pilani, 333031 Rajasthan, India, (2), Anton Pannekoek Institute for Astronomy & GRAPPA

TL;DR
This study extends the use of the A+ parameter to estimate the dynamical ages of 23 open clusters using Gaia data, revealing diverse evolutionary stages and identifying the most and least evolved clusters.
Contribution
It applies the A+ parameter methodology to open clusters with Gaia data, classifies their dynamical stages, and compares their evolution to globular clusters, expanding previous research.
Findings
Open clusters show a wide range of dynamical ages.
NGC 2682 and King 2 are highly evolved clusters.
Berkeley 18 is the least evolved open cluster.
Abstract
Blue straggler stars (BSS), one of the most massive members of star clusters, have been used for over a decade to investigate mass segregation and estimate the dynamical ages of globular clusters (GCs) and open clusters (OCs). This work is an extension of our previous study, in which we investigated a correlation between theoretically estimated dynamical ages and the observed values, which represent the sedimentation level of BSS with respect to the reference population. Here, we use the ML-MOC algorithm on \textit{Gaia} EDR3 data to extend this analysis to 23 OCs. Using cluster properties and identified members, we estimate their dynamical and physical parameters. In order to estimate the values, we use the main sequence and main sequence turnoff stars as the reference population. OCs are observed to exhibit a wide range of degrees of dynamical…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research
