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

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 ∼10 5 M ⊙ , 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 × 2 pc area of the hub with 5 σ 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 ∼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 ∼180 M ⊙ , and the cluster is currently forming stars at a rate of ∼330 M ⊙ Myr −1 , with an efficiency of ∼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.

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Publication Details

Journal
The Astronomical Journal
Published
2024-08-30
DOI
https://doi.org/10.3847/1538-3881/ad630d
Citations
2
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
0.66

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article

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

Saurabh Sharma, M. R. Samal, Jessy Jose, Vineet Rawat et al.
2 citations
The Astronomical Journal
Astrophysics and Star Formation Studies
0.66
article

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

Saurabh Sharma, M. R. Samal, Jessy Jose, Vineet Rawat, Brajesh Kumar, D. K. Ojha, Ram Kesh Yadav, R. Sagar
article en
2 citations

Abstract

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 ∼10 5 M ⊙ , 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 × 2 pc area of the hub with 5 σ 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 ∼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 ∼180 M ⊙ , and the cluster is currently forming stars at a rate of ∼330 M ⊙ Myr −1 , with an efficiency of ∼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.

The Astronomical JournalVol. 168(3)
Tata Institute of Fundamental Research (IN), Physical Research Laboratory (IN), Indian Institute of Astrophysics (IN), Yunnan University (CN), Indian Institute of Technology Gandhinagar (IN), Aryabhatta Research Institute of Observational Sciences (IN), Indian Institute of Science Education and Research, Tirupati (IN), National Astronomical Research Institute of Thailand (TH)
National Aeronautics and Space Administration, California Institute of Technology, Tata Institute of Fundamental Research, Department of Atomic Energy, Government of India, Jet Propulsion Laboratory
Openalex Percentile: Top 28%
Astrophysics and Star Formation Studies
0.66
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