作者
Doris Arzoumanian, Ray S Furuya, Tetsuo Hasegawa, M Tahani, S Sadavoy, Charles LH Hull, D Johnstone, Patrick M Koch, S-i Inutsuka, Yasuo Doi, Thiem Hoang, Takashi Onaka, Kazunari Iwasaki, Yoshito Shimajiri, Tsuyoshi Inoue, Nicolas Peretto, P André, Pierre Bastien, David Berry, H-RV Chen, J Di Francesco, Chakali Eswaraiah, Lapo Fanciullo, Laura M Fissel, Jihye Hwang, J-h Kang, Gwanjeong Kim, K-T Kim, F Kirchschlager, Woojin Kwon, CW Lee, H-L Liu, A-R Lyo, Kate Pattle, Archana Soam, X Tang, Anthony Whitworth, T-C Ching, Simon Coudé, J-W Wang, D Ward-Thompson, S-P Lai, Keping Qiu, TL Bourke, D-Y Byun, M Chen, Zhiwei Chen, Wen Ping Chen, Jungyeon Cho, Yunhee Choi, Minho Choi, A Chrysostomou, Eun Jung Chung, Sophia Dai, Pham Ngoc Diep, H-Y Duan, Yan Duan, D Eden, J Fiege, Erica Franzmann, P Friberg, G Fuller, T Gledhill, S Graves, J Greaves, Matt Griffin, Qilao Gu, Ilseung Han, J Hatchell, S Hayashi, M Houde, I-G Jeong, M Kang, S-j Kang, A Kataoka, K Kawabata, F Kemper, M-R Kim, KH Kim, J Kim, S Kim, J Kirk, MIN Kobayashi, V Könyves, T Kusune, J Kwon, K Lacaille, C-Y Law, C-F Lee, Y-H Lee, S-S Lee, H Lee, J-E Lee, H-b Li, Dalei Li, DL Li, J Liu, T Liu, S-Y Liu, X Lu, S Mairs, M Matsumura, B Matthews, G Moriarty-Schieven, T Nagata, F Nakamura, H Nakanishi, NB Ngoc, N Ohashi, G Park, H Parsons, T-S Pyo, L Qian, R Rao, J Rawlings, M Rawlings, B Retter, J Richer, A Rigby, H Saito, G Savini, A Scaife, M Seta, H Shinnaga, M Tamura, Y-W Tang, K Tomisaka, LN Tram, Y Tsukamoto, S Viti, H Wang, J Xie, H-W Yen, H Yoo, J Yuan, H-S Yun, T Zenko, G Zhang, C-P Zhang, Y Zhang, J Zhou, L Zhu, I De Looze, CD Dowell, S Eyres, S Falle, R Friesen, J-F Robitaille, S Van Loo
发表日期
2021/3/1
期刊
Astronomy & Astrophysics
卷号
647
页码范围
A78
出版商
EDP Sciences
简介
Context
Molecular filaments and hubs have received special attention recently thanks to new studies showing their key role in star formation. While the (column) density and velocity structures of both filaments and hubs have been carefully studied, their magnetic field (B-field) properties have yet to be characterized. Consequently, the role of B-fields in the formation and evolution of hub-filament systems is not well constrained.
Aims
We aim to understand the role of the B-field and its interplay with turbulence and gravity in the dynamical evolution of the NGC 6334 filament network that harbours cluster-forming hubs and high-mass star formation.
Methods
We present new observations of the dust polarized emission at 850 μm toward the 2 pc × 10 pc map of NGC 6334 at a spatial resolution of 0.09 pc obtained with the James Clerk Maxwell Telescope (JCMT) as part of the B-field In STar-forming Region Observations …
引用总数