| The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE): Core Growth, Cluster Contraction, and Primordial Mass Segregation | |
Xu, Fengwei1,2; Wang, Ke1; Liu, Tie3; Tang, Mengyao4; II, Neal J. Evans5; Palau, Aina6; Morii, Kaho7,8; He JH(何金华)9,10,11 ; Sanhueza, Patricio8,12; Liu, Hong-Li13; Stutz, Amelia14; Zhang, Qizhou15; Chen, Xi3,16,17; Li, Pak Shing3; Gómez, Gilberto C.6; Vázquez-Semadeni, Enrique6; Li, Shanghuo18; Mai, Xiaofeng3; Lu, Xing3; Liu, Meizhu13; Chen, Li13; Li, Chuanshou13; Shi, Hongqiong13; Ren, Zhiyuan19; Li, Di19,20,21; Garay, Guido11; Bronfman, Leonardo11; Dewangan, Lokesh22; Juvela, Mika23; Lee, Chang Won24,25; Zhang, S.1; Yue, Nannan1; Wang, Chao1,2; Ge, Yifei1,2; Jiao, Wenyu1,2,18; Luo, Qiuyi3; Zhou, J.-W.26; Tatematsu, Ken'ichi8,12; Chibueze, James O.27,28,29; Su, Keyun1; Sun, Shenglan1; Ristorcelli, I.30; Toth, L. Viktor31,32
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| 发表期刊 | ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
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| 2024 | |
| 卷号 | 270期号:1 |
| DOI | 10.3847/1538-4365/acfee5 |
| 产权排序 | 第9完成单位 |
| 收录类别 | SCI |
| 摘要 | The Atacama Large Millimeter/submillimeter Array (ALMA) Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE) aims to investigate the process of mass assembly and its connection to high-mass star formation theories in protoclusters in a dynamic view. We observed 11 massive (M clump greater than or similar to 103 M circle dot), luminous (L bol greater than or similar to 104 L circle dot), and blue-profile (infall signature) clumps by ALMA with resolution of similar to 2200-5500 au (median value of 3500 au) at 350 GHz (870 mu m). We identified 248 dense cores, including 106 cores showing protostellar signatures and 142 prestellar core candidates. Compared to early stage infrared dark clouds (IRDCs) by ASHES, the core mass and surface density within the ASSEMBLE clumps exhibited a significant increment, suggesting concurrent core accretion during the evolution of the clumps. The maximum mass of prestellar cores was found to be 2 times larger than that in IRDCs, indicating that evolved protoclusters have the potential to harbor massive prestellar cores. The mass relation between clumps and their most massive core (MMCs) is observed in ASSEMBLE but not in IRDCs, which is suggested to be regulated by multiscale mass accretion. The mass correlation between the core clusters and their MMCs has a steeper slope compared to that observed in stellar clusters, which can be due to fragmentation of the MMC and stellar multiplicity. We observe a decrease in core separation and an increase in central concentration as protoclusters evolve. We confirm primordial mass segregation in the ASSEMBLE protoclusters, possibly resulting from gravitational concentration and/or gas accretion. |
| 资助项目 | National Science Foundation of China; National Key RAMP;D Program of China; China Manned Space Project; High-Performance Computing Platform of Peking University; China-Chile Joint Research Fund (CCJRF); Chinese academy of sciences; Shanghai Pujiang Program; Yunnan provincial Department of Science and Technology; JSPS; Yunnan Fundamental Research Project; UNAM-PAPIIT; Sistema Nacional de Investigadores of CONAHCyT; CONAHCyT; ANID through the BASAL project; Fondecyt Regular; Chinese Academy of Sciences (CAS); Academy of Finland; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[11973013]; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[12033005]; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[11721303]; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[12073061]; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[12122307]; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[12203011]; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[12103045]; Korea Astronomy and Space Science Institute - Korea government (MSIT)[2022YFA1603100]; Korea Astronomy and Space Science Institute - Korea government (MSIT)[2019YFA0405100]; JSPS KAKENHI |
| 项目资助者 | National Science Foundation of China ; National Key RAMP ; D Program of China ; China Manned Space Project ; High-Performance Computing Platform of Peking University ; China-Chile Joint Research Fund (CCJRF) ; Chinese academy of sciences ; Shanghai Pujiang Program ; Yunnan provincial Department of Science and Technology ; JSPS ; Yunnan Fundamental Research Project ; UNAM-PAPIIT ; Sistema Nacional de Investigadores of CONAHCyT ; CONAHCyT ; ANID through the BASAL project ; Fondecyt Regular ; Chinese Academy of Sciences (CAS) ; Academy of Finland ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[11973013, 12033005, 11721303, 12073061, 12122307, 12203011, 12103045] ; Korea Astronomy and Space Science Institute - Korea government (MSIT)[2022YFA1603100, 2019YFA0405100] ; JSPS KAKENHI[CMS-CSST-2021-A09, CMS-CSST-2021-B06] ; [2211] ; [114231KYSB20200009] ; [20PJ1415500] ; [202101BA070001-261] ; [22J21529] ; [JP22H01271] ; [JP23H01221] ; [202301AT070118] ; [IG100223] ; [IN10382] ; [86372] ; [FB210003] ; [1220610] ; [348342] ; [NRF- 2019R1A2C1010851] ; [2023-1-84000] ; [JP20H05645] |
| 语种 | 英语 |
| 学科领域 | 天文学 |
| 文章类型 | Article |
| 出版者 | IOP Publishing Ltd |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0067-0049 |
| URL | 查看原文 |
| WOS记录号 | WOS:001132952700001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | INFRARED DARK CLOUD ; COMPACT SOURCE CATALOG ; SCALE GREATER-THAN-OR-EQUAL-TO-10 PC ; RADIATION-HYDRODYNAMIC SIMULATIONS ; VELOCITY-COHERENT FILAMENTS ; THERMAL JEANS FRAGMENTATION ; LARGE ARRAY OBSERVATIONS ; INNER GALACTIC PLANE ; FORMING REGIONS ; HIERARCHICAL FRAGMENTATION |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 版本 | 出版稿 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/26479 |
| 专题 | 其他 |
| 作者单位 | 1.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China; [email protected]; 2.Department of Astronomy, School of Physics, Peking University, Beijing, 100871, People's Republic of China; 3.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, People's Republic of China; 4.Institute of Astrophysics, School of Physics and Electronic Science, Chuxiong Normal University, Chuxiong 675000, People's Republic of China; 5.Department of Astronomy, The University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712-1205, USA; 6.Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Antigua Carretera a Pátzcuaro 8701, Ex-Hda. San José de la Huerta, 58089 Morelia, Michoacán, Mexico; 7.Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan; 8.National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; 9.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China; 10.Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, CAS, Beijing 100101, People's Republic of China; 11.Departamento de Astronomía, Universidad de Chile, Las Condes, 7591245 Santiago, Chile; 12.Astronomical Science Program, The Graduate University for Advanced Studies, SOKENDAI, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; 13.Department of Astronomy, Yunnan University, Kunming 650091, People's Republic of China; 14.Departamento de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción, Chile; 15.Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA; 16.Center for Astrophysics, Guangzhou University, Guangzhou 510006, People's Republic of China; 17.Peng Cheng Lab, Shenzhen, 518066, People's Republic of China; 18.Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany; 19.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China; 20.Research Center for Intelligent Computing Platforms, Zhejiang Laboratory, Hangzhou 311100, People's Republic of China; 21.NAOC-UKZN Computational Astrophysics Centre (NUCAC), University of KwaZulu-Natal, Durban, 4000, South Africa; 22.Physical Research Laboratory, Navrangpura, Ahmedabad-380 009, India; 23.Department of Physics, University of Helsinki, PO Box 64, FI-00014 Helsinki, Finland; 24.Korea Astronomy and Space Science Institute, 776 Daedeok-daero, Yuseong-gu, Daejeon 34055, Republic of Korea; 25.University of Science and Technology, 217 Gajeong-ro, Yuseong-gu, Daejeon 34113, Republic of Korea; 26.Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany; 27.Department of Mathematical Sciences, University of South Africa, Cnr Christian de Wet Rd and Pioneer Avenue, Florida Park, 1709, Roodepoort, South Africa; 28.Centre for Space Research, Physics Department, North-West University, Potchefstroom 2520, South Africa; 29.Department of Physics and Astronomy, Faculty of Physical Sciences, University of Nigeria, Carver Building, 1 University Road, Nsukka 410001, Nigeria; 30.Univ. Toulouse, CNRS, IRAP, 9 Av. du colonel Roche, BP 44346, F-31028, Toulouse, France; 31.Eötvös University Budapest, Institute of Physics and Astronomy, Pazmany P.s. 1/A, H-1117 Budapest, Hungary; 32.University of Debrecen, Faculty of Science and Technology, Egyetem tér 1, H-4032 Debrecen, Hungary |
| 推荐引用方式 GB/T 7714 | Xu, Fengwei,Wang, Ke,Liu, Tie,et al. The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE): Core Growth, Cluster Contraction, and Primordial Mass Segregation[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2024,270(1). |
| APA | Xu, Fengwei.,Wang, Ke.,Liu, Tie.,Tang, Mengyao.,II, Neal J. Evans.,...&Toth, L. Viktor.(2024).The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE): Core Growth, Cluster Contraction, and Primordial Mass Segregation.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,270(1). |
| MLA | Xu, Fengwei,et al."The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE): Core Growth, Cluster Contraction, and Primordial Mass Segregation".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 270.1(2024). |
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