{ "id": "2408.12969", "version": "v1", "published": "2024-08-23T10:35:16.000Z", "updated": "2024-08-23T10:35:16.000Z", "title": "Peering into the Heart of the Giant Molecular Cloud G148.24+00.41: A Deep Near-infrared View of the Newly Hatched Cluster FSR 655", "authors": [ "Vineet Rawat", "M. R. Samal", "D. K. Ojha", "Brajesh Kumar", "Saurabh Sharma", "J. Jose", "Ram Sagar", "R. K. Yadav" ], "comment": "17 pages and 13 figures", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "We present a detailed near-infrared study of an embedded cluster located in the hub of the giant molecular cloud G148.24+00.41 of mass $\\sim$10$^5$ $M_\\odot$, with the TANSPEC instrument mounted on the 3.6 m Devasthal Optical Telescope. The hub is located near the geometric center of the cloud and represents its most massive clump. We studied the central 2 pc $\\times$ 2 pc area of the hub with 5$\\sigma$ limiting magnitudes of 20.5, 20.1, and 18.6 mag in the $J$, $H$, and $K_s$ bands, respectively. Using the $K_s$-band luminosity function and comparing it with the synthetic clusters, we obtained the age of the cluster as $\\sim$0.5 Myr, which was found to corroborate well with the visual extinction versus the age of nearby embedded clusters. We find that the present mass of the cluster is around $\\sim$180 $M_\\odot$, and the cluster is currently forming stars at a rate of $\\sim$330 $M_\\odot$ $\\rm{Myr}^{-1}$, with an efficiency of $\\sim$20%. The cluster is connected to an extended gas reservoir through a filamentary network; thus, we hypothesize that the cluster has the potential to become a richer cluster in a few Myr of time.", "revisions": [ { "version": "v1", "updated": "2024-08-23T10:35:16.000Z" } ], "analyses": { "keywords": [ "giant molecular cloud", "newly hatched cluster fsr", "deep near-infrared view", "embedded cluster", "band luminosity function" ], "note": { "typesetting": "TeX", "pages": 17, "language": "en", "license": "arXiv", "status": "editable" } } }