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 |
| DOI | 10.3847/1538-4357/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 |
| 推荐引用方式 GB/T 7714 | 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. |
入库方式: OAI收割
来源:新疆天文台
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。

