中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Evidences of Two Merging Elongated Filaments Associated with AGAL323.444+0.096 and Star Formation

文献类型:期刊论文

作者Ma, Yingxiu4,5; Zhou, Jianjun4,5,6,7; Esimbek, Jarken4,5,6,7; Li, Dalei4,5,7; Sobolev, Andrej M.4; Tang, Xindi4,5,6,7; Baan, Willem3,4,5; Wu, Gang4,5,7; Gordon, Macleod1,2,4; He, Yuxin4,5,6,7
刊名ASTROPHYSICAL JOURNAL
出版日期2025-11-20
卷号994期号:1页码:118
ISSN号0004-637X
DOI10.3847/1538-4357/ae12f4
产权排序1
英文摘要We study the structure, kinematics, and star-forming activity of filamentary cloud F-NE associated with AGAL323.444+0.096 using 13CO (J = 2-1) molecular line and continuum data from the far-infrared to near-infrared. The cloud comprises two elongated subfilaments, F-NE-north and F-NE-south, each spanning 25 pc, with systemic velocities of -65.25 and -67.38 km s-1, respectively. F-NE-north and F-NE-south seem to be merging by collision. They exhibit signatures of cloud-cloud collisions, including U-shaped and arc-like morphologies, complementary components, and bridge features, suggesting ongoing collisions. The interacting zones show enhanced column densities and elevated velocity dispersion, further supporting the collision scenario. All these features are consistent with the "fray and gather" model. Dense clumps and young stellar objects are predominantly concentrated in these collision regions, implying that filament merging and localized collisions drive the formation of massive dusty clumps capable of nurturing massive stars. These results demonstrate that filament merging by collision is crucial for both filament structural evolution and the formation of massive stars and clusters.
WOS关键词CLOUD-CLOUD COLLISION ; GALACTIC PLANE ; DENSE CORES ; HI-GAL ; CLUSTER FORMATION ; SOURCE CATALOG ; DARK CLOUDS ; SYSTEMS ; I.
资助项目MOST divided by R&D Project of Ministry of Science and Technology of the People's Republic of China[2023YFA1608002] ; MOST divided by National Natural Science Foundation of China (NSFC)[12403033]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001618310200001
出版者IOP Publishing Ltd
资助机构MOST divided by R&D Project of Ministry of Science and Technology of the People's Republic of China ; MOST divided by National Natural Science Foundation of China (NSFC)
源URL[http://ir.xao.ac.cn/handle/45760611-7/8317]  
专题恒星形成与演化研究团组
通讯作者Ma, Yingxiu; Zhou, Jianjun
作者单位1.Open Univ Tanzania, Dar Es Salaam, Tanzania
2.Hartebeesthoek Radio Astron Observ, Krugersdorp, South Africa
3.Netherlands Inst Radio Astron, ASTRON, NL-7991 PD Dwingeloo, Netherlands
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
5.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China
6.State Key Lab Radio Astron & Technol, A20 Datun Rd, Beijing 100101, Peoples R China
7.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
8.Ural Fed Univ, 19 Mira St, Ekaterinburg 620002, Russia
9.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
10.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
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Ma, Yingxiu,Zhou, Jianjun,Esimbek, Jarken,et al. Evidences of Two Merging Elongated Filaments Associated with AGAL323.444+0.096 and Star Formation[J]. ASTROPHYSICAL JOURNAL,2025,994(1):118.
APA Ma, Yingxiu.,Zhou, Jianjun.,Esimbek, Jarken.,Li, Dalei.,Sobolev, Andrej M..,...&Shen, Hailiang.(2025).Evidences of Two Merging Elongated Filaments Associated with AGAL323.444+0.096 and Star Formation.ASTROPHYSICAL JOURNAL,994(1),118.
MLA Ma, Yingxiu,et al."Evidences of Two Merging Elongated Filaments Associated with AGAL323.444+0.096 and Star Formation".ASTROPHYSICAL JOURNAL 994.1(2025):118.

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