The ALMA-QUARKS Survey. III. Clump-to-core Fragmentation and Searches for High-mass Starless Cores

Abstract The Querying Underlying mechanisms of massive star formation with ALMA-Resolved gas Kinematics and Structures (QUARKS) survey observed 139 infrared-bright (IR-bright) massive protoclusters at 1.3 mm wavelength with the Atacama Large Millimeter/submillimeter Array (ALMA). This study investigates clump-to-core fragmentation and searches for candidate high-mass starless cores within IR-bright clumps using combined ALMA 12 m (C-2) and Atacama Compact Array 7 m data, providing ∼1″ (∼0.02 pc at 3.7 kpc) resolution and ∼0.6 mJy beam −1 continuum sensitivity (∼0.3 M ⊙ at 30 K). We identified 1562 compact cores from 1.3 mm continuum emission using getsf . Observed linear core separations ( λ obs ) are significantly less than the thermal Jeans length ( λ J ), with the λ obs / λ J ratios peaking at ∼0.2. This indicates that thermal Jeans fragmentation has taken place within the IR-bright protocluster clumps studied here. The observed low ratio of λ obs / λ J ≪ 1 could be the result of evolving core separation or hierarchical fragmentation. Based on associated signatures of star formation (e.g., outflows and ionized gas), we classified cores into three categories: 127 starless, 971 warm, and 464 evolved cores. Two starless cores have masses exceeding 16 M ⊙ , and represent high-mass candidates. The scarcity of such candidates suggests that competitive accretion-type models could be more applicable than turbulent core accretion-type models in high-mass star formation within these IR-bright protocluster clumps.

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Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2025-09-01
DOI
https://doi.org/10.3847/1538-4365/adf847
Citations
7
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
8.08
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article

The ALMA-QUARKS Survey. III. Clump-to-core Fragmentation and Searches for High-mass Starless Cores

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7 citations
The Astrophysical Journal Supplement Series
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article

The ALMA-QUARKS Survey. III. Clump-to-core Fragmentation and Searches for High-mass Starless Cores

Dongting Yang, Xiaofeng Mai, Xindi Tang, Tie Liu, Jihye Hwang, Patricio Sanhueza, Xunchuan Liu, Shanghuo Li, Fengwei Xu, L. K. Dewangan, Prasanta Gorai, Chuanshou Li, Tapas Baug, Xianjin Shen, Anandmayee Tej, Chang Won Lee, Ariful Hoque, Anindya Saha, Wenyu Jiao, Yankun Zhang, P. F. Goldsmith, Sami Dib, A. Y. Yang, L. Bronfman, A. Zavagno, James O. Chibueze, Ankan Das, Sheng‐Li Qin, Mengyao Tang, Pablo García, Amelia M. Stutz, L. Viktor Tóth, Kotomi Taniguchi, Aina Palau, Jianjun Zhou, Yichen Zhang, Li Chen, Hongli Liu, Tianwei Zhang, Swagat Ranjan Das, J. H. Zou, Guido Garay, Hafiz Nazeer, Lei Zhu, Siju Zhang, Zhiping Kou
article en
7 citations

Abstract

Abstract The Querying Underlying mechanisms of massive star formation with ALMA-Resolved gas Kinematics and Structures (QUARKS) survey observed 139 infrared-bright (IR-bright) massive protoclusters at 1.3 mm wavelength with the Atacama Large Millimeter/submillimeter Array (ALMA). This study investigates clump-to-core fragmentation and searches for candidate high-mass starless cores within IR-bright clumps using combined ALMA 12 m (C-2) and Atacama Compact Array 7 m data, providing ∼1″ (∼0.02 pc at 3.7 kpc) resolution and ∼0.6 mJy beam −1 continuum sensitivity (∼0.3 M ⊙ at 30 K). We identified 1562 compact cores from 1.3 mm continuum emission using getsf . Observed linear core separations ( λ obs ) are significantly less than the thermal Jeans length ( λ J ), with the λ obs / λ J ratios peaking at ∼0.2. This indicates that thermal Jeans fragmentation has taken place within the IR-bright protocluster clumps studied here. The observed low ratio of λ obs / λ J ≪ 1 could be the result of evolving core separation or hierarchical fragmentation. Based on associated signatures of star formation (e.g., outflows and ionized gas), we classified cores into three categories: 127 starless, 971 warm, and 464 evolved cores. Two starless cores have masses exceeding 16 M ⊙ , and represent high-mass candidates. The scarcity of such candidates suggests that competitive accretion-type models could be more applicable than turbulent core accretion-type models in high-mass star formation within these IR-bright protocluster clumps.

The Astrophysical Journal Supplement SeriesVol. 280(1)
Openalex Percentile: Top 3%
Astrophysics and Star Formation Studies
8.08
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