Skip to main navigation Skip to search Skip to main content

The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament

  • Tao Chung Ching
  • , Keping Qiu
  • , Di Li
  • , Zhiyuan Ren
  • , Shih Ping Lai
  • , David Berry
  • , Kate Pattle
  • , Ray Furuya
  • , Derek Ward-Thompson
  • , Doug Johnstone
  • , Patrick M. Koch
  • , Chang Won Lee
  • , Thiem Hoang
  • , Tetsuo Hasegawa
  • , Woojin Kwon
  • , Pierre Bastien
  • , Chakali Eswaraiah
  • , Jia Wei Wang
  • , Kyoung Hee Kim
  • , Jihye Hwang
  • Archana Soam, A. Ran Lyo, Junhao Liu, Valentin J.M. Le Gouellec, Doris Arzoumanian, Anthony Whitworth, James Di Francesco, Frédérick Poidevin, Tie Liu, Simon Coudé, Mehrnoosh Tahani, Hong Li Liu, Takashi Onaka, Dalei Li, Motohide Tamura, Zhiwei Chen, Xindi Tang, Florian Kirchschlager, Tyler L. Bourke, Do Young Byun, Mike Chen, Huei Ru Vivien Chen, Wen Ping Chen, Jungyeon Cho, Yunhee Choi, Youngwoo Choi, Minho Choi, Antonio Chrysostomou, Eun Jung Chung, Y. Sophia Dai, Pham Ngoc Diep, Yasuo Doi, Yan Duan, Hao Yuan Duan, David Eden, Lapo Fanciullo, Jason Fiege, Laura M. Fissel, Erica Franzmann, Per Friberg, Rachel Friesen, Gary Fuller, Tim Gledhill, Sarah Graves, Jane Greaves, Matt Griffin, Qilao Gu, Ilseung Han, Saeko Hayashi, Martin Houde, Charles L.H. Hull, Tsuyoshi Inoue, Shu Ichiro Inutsuka, Kazunari Iwasaki, Il Gyo Jeong, Vera Könyves, Ji Hyun Kang, Miju Kang, Janik Karoly, Akimasa Kataoka, Koji Kawabata, Francisca Kemper, Jongsoo Kim, Mi Ryang Kim, Shinyoung Kim, Hyosung Kim, Kee Tae Kim, Gwanjeong Kim, Jason Kirk, Masato I.N. Kobayashi, Takayoshi Kusune, Jungmi Kwon, Kevin Lacaille, Chi Yan Law, Sang Sung Lee, Hyeseung Lee, Jeong Eun Lee, Chin Fei Lee, Yong Hee Lee, Guangxing Li, Hua Bai Li, Sheng Jun Lin, Sheng Yuan Liu, Xing Lu, Steve Mairs, Masafumi Matsumura, Brenda Matthews, Gerald Moriarty-Schieven, Tetsuya Nagata, Fumitaka Nakamura, Hiroyuki Nakanishi, Nguyen Bich Ngoc, Nagayoshi Ohashi, Geumsook Park, Harriet Parsons, Nicolas Peretto, Felix Priestley, Tae Soo Pyo, Lei Qian, Ramprasad Rao, Mark Rawlings, Jonathan Rawlings, Brendan Retter, John Richer, Andrew Rigby, Sarah Sadavoy, Hiro Saito, Giorgio Savini, Masumichi Seta, Yoshito Shimajiri, Hiroko Shinnaga, Ya Wen Tang, Kohji Tomisaka, Le Ngoc Tram, Yusuke Tsukamoto, Serena Viti, Hongchi Wang, Jintai Wu, Jinjin Xie, Meng Zhe Yang, Hsi Wei Yen, Hyunju Yoo, Jinghua Yuan, Hyeong Sik Yun, Tetsuya Zenko, Chuan Peng Zhang, Yapeng Zhang, Guoyin Zhang, Jianjun Zhou, Lei Zhu, Ilse De Looze, Philippe André, C. Darren Dowell, Stewart Eyres, Sam Falle, Jean François Robitaille, Sven Van Loo
  • Zhejiang Lab
  • National Astronomical Observatories Chinese Academy of Sciences
  • National Radio Astronomy Observatory Socorro
  • Nanjing University
  • University of Chinese Academy of Sciences
  • University of KwaZulu–Natal
  • National Tsing Hua University
  • Academia Sinica, Institute of Astronomy and Astrophysics
  • East Asian Observatory
  • University College London
  • Tokushima University
  • University of Central Lancashire
  • National Research Council Canada
  • University of Victoria
  • Korea Astronomy and Space Science Institute
  • Korea University of Science and Technology
  • National Institutes of Natural Sciences - National Astronomical Observatory of Japan
  • Seoul National University
  • Université de Montréal
  • Indian Institute of Science Education and Research (IISER) Tirupati
  • Ulsan National Institute of Science and Technology
  • Indian Institute of Astrophysics
  • Universities Space Research Association
  • Université Paris-Sud
  • Cardiff University
  • GTC Project
  • Universidad de la Laguna
  • Shanghai Astronomical Observatory Chinese Academy of Sciences
  • Worcester State University
  • Harvard & Smithsonian
  • Stanford University
  • Yunnan University
  • Meisei University
  • University of Tokyo
  • Xinjiang Astronomical Observatory
  • National Institutes of Natural Sciences - AstroBiology Center
  • Purple Mountain Observatory Chinese Academy of Sciences
  • SKA Organisation, UK
  • University of Manchester
  • National Central University
  • Chungnam National University
  • Vietnam Academy of Science and Technology
  • Armagh Observatory
  • National Chung Hsing University
  • University of Manitoba
  • Queen’s University
  • National Radio Astronomy Observatory
  • University of Hertfordshire
  • University of Western Ontario
  • Joint ALMA Observatory
  • NAOJ Fellow
  • Nagoya University
  • Doshisha University
  • Kyungpook National University (KNU)
  • Hiroshima University
  • Institut de Ciéncies de l’Espai (ICE-CSIC)
  • ICREA Catalan Institution for Research and Advanced Studies
  • PMT-UPC
  • Tohoku University
  • McMaster University, Faculty of Science
  • Dalhousie University
  • Chinese University of Hong Kong
  • Chalmers University of Technology
  • Kyung Hee University
  • Kagawa University
  • Graduate School of Science
  • The Graduate University for Advanced Studies
  • Kagoshima University
  • Chinese Academy of Sciences
  • NSF's National Optical-Infrared Astronomy Research Laboratory
  • Cavendish Laboratory
  • Institute of Astronomy
  • University of Tsukuba
  • Kwansei Gakuin University
  • University of Science and Technology of Hanoi (USTH)
  • Beijing Normal University
  • CEA Saclay
  • Jet Propulsion Laboratory
  • Glamorgan University
  • University of Leeds
  • Laboratoire Astrophysique de Grenoble

Research output: Contribution to a Journal (Peer & Non Peer)Articlepeer-review

24 Citations (Scopus)

Abstract

We present 850 μm dust polarization observations of the massive DR21 filament from the B-fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter and the SCUBA-2 camera on the James Clerk Maxwell Telescope. We detect ordered magnetic fields perpendicular to the parsec-scale ridge of the DR21 main filament. In the subfilaments, the magnetic fields are mainly parallel to the filamentary structures and smoothly connect to the magnetic fields of the main filament. We compare the POL-2 and Planck dust polarization observations to study the magnetic field structures of the DR21 filament on 0.1-10 pc scales. The magnetic fields revealed in the Planck data are well-aligned with those of the POL-2 data, indicating a smooth variation of magnetic fields from large to small scales. The plane-of-sky magnetic field strengths derived from angular dispersion functions of dust polarization are 0.6-1.0 mG in the DR21 filament and ∼0.1 mG in the surrounding ambient gas. The mass-to-flux ratios are found to be magnetically supercritical in the filament and slightly subcritical to nearly critical in the ambient gas. The alignment between column density structures and magnetic fields changes from random alignment in the low-density ambient gas probed by Planck to mostly perpendicular in the high-density main filament probed by James Clerk Maxwell Telescope. The magnetic field structures of the DR21 filament are in agreement with MHD simulations of a strongly magnetized medium, suggesting that magnetic fields play an important role in shaping the DR21 main filament and subfilaments.

Original languageEnglish
Article number122
JournalAstrophysical Journal
Volume941
Issue number2
DOIs
Publication statusPublished - 1 Dec 2022
Externally publishedYes

Fingerprint

Dive into the research topics of 'The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament'. Together they form a unique fingerprint.

Cite this