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ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – V. Hierarchical fragmentation and gas dynamics in IRDC G034.43+00.24

  • 【作者】Hong-Li Liu,Anandmayee Tej,Tie Liu,Namitha Issac,Anindya Saha,Paul F Goldsmith,Jun-Zhi Wang,Qizhou Zhang,Sheng-Li Qin,Ke Wang,Shanghuo Li,Archana Soam,Lokesh Dewangan,Chang Won Lee,Pak-Shing Li,Xun-Chuan Liu,Yong Zhang,Zhiyuan Ren,Mika Juvela,Leonardo Bronfman,Yue-Fang Wu,Ken’ichi Tatematsu,Xi Chen,Di Li,Amelia Stutz,Siju Zhang,L Viktor Toth,Qiu-Yi Luo,Feng-Wei Xu,Jinzeng Li,Rong Liu,Jianwen Zhou,Chao Zhang,Mengyao Tang,Chao Zhang,Tapas Baug,E Mannfors,Eswaraiah Chakali,Somnath Dutta
  • 【刊名】Monthly Notices of the Royal Astronomical Society
  • 【作者单位】1 Department of Astronomy, Yunnan University , Kunming 650091, China; 2 Indian Institute of Space Science and Technology , Thiruvananthapuram 695 547, Kerala, India; 3 Shanghai Astronomical Observatory, Chinese Academy of Sciences , 80 Nandan Road, Shanghai 200030, China; 4 Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences , 80 Nandan Road, Shanghai 200030, China; 5 Jet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Drive, Pasadena, CA 91109, USA; 6 Key Laboratory of Radio Astronomy, Chinese Academy of Sciences , Nanjing 210008, China; 7 Center for Astrophysics | Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USA; 8 Kavli Institute for Astronomy and Astrophysics, Peking University , 5 Yiheyuan Road, Haidian District, Beijing 100871, China; 9 Department of Astronomy, Peking University , Beihing 100871, China; 10 Korea Astronomy and Space Science Institute , 776 Daedeokdaero, Yuseong-gu, Daejeon 34055, Republic of Korea; 11 SOFIA Science Centre , USRA, NASA Ames Research Centre, MS-12, N232, Moffett Field, CA 94035, USA; 12 Physical Research Laboratory , Navrangpura, Ahmedabad-380 009, India; 13 University of Science and Technology , Korea (UST), 217 Gajeong-ro, Yuseong-gu, Daejeon 34113, Republic of Korea; 14 Astronomy Department, University of California , Berkeley, CA 94720, USA; 15 School of Physics and Astronomy , Sun Yat-sen University, 2 Daxue Road, Zhuhai, Guangdong 519082, China; 16 National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, China; 17 Department of Physics , PO box 64, FI- 00014, University of Helsinki, Finland; 18 Departamento de Astronomía, Universidad de Chile , Las Condes, Santiago, Chile; 19 National Astronomical Observatory of Japan, National Institutes of Natural Sciences , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; 20 Center for Astrophysics, GuangZhou University , Guangzhou 510006, China; 21 University of Chinese Academy of Sciences , Beijing 100049, China; 22 NAOC-UKZN Computational Astrophysics Centre, University of KwaZulu-Natal , Durban 4000, South Africa; 23 Departamento de Astronomía, Universidad de Concepción , Av. Esteban Iturra s/n, Distrito Universitario, 160-C, Chile; 24 Max-Planck-Institute for Astronomy , Königstuhl 17, D-69117 Heidelberg, Germany; 25 Eötvös Loránd University, Department of Astronomy , Pázmány Péter sétány 1/A, H-1117 Budapest, Hungary; 26 Department of Physics, Taiyuan Normal University , Jinzhong 030619, China; 27 Institute of Astrophysics, School of Physics and Electronic Science, Chuxiong Normal University, Chuxiong; 28 Satyendra Nath Bose National Centre for Basic Sciences , Block-JD, Sector-III, Salt Lake, Kolkata-700 106, India; 29 Indian Institute of Science Education and Research Tirupati , Rami Reddy Nagar, Karakambadi Road, Mangalam (PO), Tirupati 517 507, India; 30 Institute of Astronomy and Astrophysics, Academia Sinica, Roosevelt Rd, Taipei 10617, Taiwan, R.O.C
  • 【年份】2022
  • 【卷号】Vol.510 No.4
  • 【页码】5009-5022
  • 【ISSN】0035-8711
  • 【关键词】stars: formation stars: kinematics and dynamics ISM: clouds ISM: individual objects: G034.43+00.24 
  • 【摘要】 We present new 3-mm continuum and molecular lines observations from the ATOMS survey towards the massive protostellar clump, MM1, located in the filamentary infrared dark cloud , G034.43+00.24 . The lines observed are the tracers of either dense gas ...
  • 【文献类型】 期刊
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