{ "id": "2403.04532", "version": "v1", "published": "2024-03-07T14:30:04.000Z", "updated": "2024-03-07T14:30:04.000Z", "title": "Exploring NGC 2345: A Comprehensive Study of a Young Open Cluster through Photometric and Kinematic Analysis", "authors": [ "Kuldeep Belwal", "D. Bisht", "Mohit Singh Bisht", "Geeta Rangwal", "Ashish Raj", "Arvind K. Dattatrey", "R. K. S. Yadav", "B. C. Bhatt" ], "comment": "Accepted for publication in A&A and 21 pages, 22 Figures", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "We conducted a photometric and kinematic analysis of the young open cluster NGC 2345 using CCD \\emph{UBV} data from 2-m Himalayan Chandra Telescope (HCT), \\emph{Gaia} Data Release 3 (DR3), 2MASS, and the APASS datasets. We found 1732 most probable cluster members with membership probability higher than 70$\\%$. The fundamental and structural parameters of the cluster are determined based on the cluster members. The mean proper motion of the cluster is estimated to be $\\mu_{\\alpha}cos\\delta$ = ${-1.34}\\pm0.20$ and $\\mu_{\\delta}$= $1.35\\pm 0.21$ mas $yr^{-1}$. Based on the radial density profile, the estimated radius is $\\sim$ 12.8 arcmin (10.37 pc). Using color-color and color-magnitude diagrams, we estimate the reddening, age, and distance to be $0.63\\pm0.04$ mag, 63 $\\pm$ 8 Myr, and 2.78 $\\pm$ 0.78 kpc, respectively. The mass function slope for main-sequence stars is determined as $1.2\\pm 0.1$. The mass function slope in the core, halo, and overall region indicates a possible hint of mass segregation. The cluster's dynamical relaxation time is 177.6 Myr, meaning ongoing mass segregation, with complete equilibrium expected in 100-110 Myr. Apex coordinates are determined as $-40^{\\circ}.89 \\pm 0.12, -44^{\\circ}.99 \\pm 0.15$. The cluster's orbit in the Galaxy suggests early dissociation in field stars due to its close proximity to the Galactic disk.", "revisions": [ { "version": "v1", "updated": "2024-03-07T14:30:04.000Z" } ], "analyses": { "keywords": [ "kinematic analysis", "exploring ngc", "comprehensive study", "mass function slope", "photometric" ], "note": { "typesetting": "TeX", "pages": 21, "language": "en", "license": "arXiv", "status": "editable" } } }