@article{8769126,
  abstract     = {{We present the first results from the B-fields In STar-forming Region Observations (BISTRO) survey, using the Sub-millimetre Common-User Bolometer Array. 2 camera, with its associated polarimeter (POL-2), on the James Clerk Maxwell Telescope in Hawaii. We discuss the survey's aims and objectives. We describe the rationale behind the survey, and the questions that. the survey will aim to answer. The most important of these is the role of magnetic fields in the star formation process on the scale of individual filaments and cores in dense regions. We describe the data acquisition and reduction processes for POL-2, demonstrating both repeatability and consistency with previous data. We present a first-look analysis of the first results from the BISTRO survey in the OMC 1 region. We see that the magnetic field lies approximately perpendicular to the famous "integral filament" in the densest regions of that filament. Furthermore, we see an "hourglass" magnetic field morphology extending beyond the densest region of the integral filament into the less-dense surrounding material, and discuss possible causes for this. We also discuss the more complex morphology seen along the Orion Bar region. We examine the morphology of the field along the lower-density northeastern filament. We find consistency with previous theoretical models that predict magnetic fields lying parallel to low-density, non-self-gravitating filaments, and perpendicular to higher-density, self-gravitating filaments.}},
  articleno    = {{66}},
  author       = {{Ward-Thompson, Derek and Pattle, Kate and Bastien, Pierre and Furuya, Ray S. and Kwon, Woojin and Lai, Shih-Ping and Qiu, Keping and Berry, David and Choi, Minho and Coude, Simon and Di Francesco, James and Hoang, Thiem and Franzmann, Erica and Friberg, Per and Graves, Sarah F. and Greaves, Jane S. and Houde, Martin and Johnstone, Doug and Kirk, Jason M. and Koch, Patrick M. and Kwon, Jungmi and Lee, Chang Won and Li, Di and Matthews, Brenda C. and Mottram, Joseph C. and Parsons, Harriet and Pon, Andy and Rao, Ramprasad and Rawlings, Mark and Shinnaga, Hiroko and Sadavoy, Sarah and Van Loo, Sven and Aso, Yusuke and Byun, Do-Young and Eswaraiah, Chakali and Chen, Huei-Ru and Chen, Mike C. -Y. and Chen, Wen Ping and Ching, Tao-Chung and Cho, Jungyeon and Chrysostomou, Antonio and Chung, Eun Jung and Doi, Yasuo and Drabek-Maunder, Emily and Eyres, Stewart P. S. and Fiege, Jason and Friesen, Rachel K. and Fuller, Gary and Gledhill, Tim and Griffin, Matt J. and Gu, Qilao and Hasegawa, Tetsuo and Hatchell, Jennifer and Hayashi, Saeko S. and Holland, Wayne and Inoue, Tsuyoshi and Inutsuka, Shu-ichiro and Iwasaki, Kazunari and Jeong, Il-Gyo and Kang, Ji-hyun and Kang, Miju and Kang, Sung-ju and Kawabata, Koji S. and Kemper, Francisca and Kim, Gwanjeong and Kim, Jongsoo and Kim, Kee-Tae and Kim, Kyoung Hee and Kim, Mi-Ryang and Kim, Shinyoung and Lacaille, Kevin M. and Lee, Jeong-Eun and Lee, Sang-Sung and Li, Dalei and Li, Hua-bai and Liu, Hong-Li and Liu, Junhao and Liu, Sheng-Yuan and Liu, Tie and Lyo, A-Ran and Mairs, Steve and Matsumura, Masafumi and Moriarty-Schieven, Gerald H. and Nakamura, Fumitaka and Nakanishi, Hiroyuki and Ohashi, Nagayoshi and Onaka, Takashi and Peretto, Nicolas and Pyo, Tae-Soo and Qian, Lei and Retter, Brendan and Richer, John and Rigby, Andrew and Robitaille, Jean-Francois and Savini, Giorgio and Scaife, Anna M. M. and Soam, Archana and Tamura, Motohide and Tang, Ya-Wen and Tomisaka, Kohji and Wang, Hongchi and Wang, Jia-Wei and Whitworth, Anthony P. and Yen, Hsi-Wei and Yoo, Hyunju and Yuan, Jinghua and Zhang, Chuan-Peng and Zhang, Guoyin and Zhou, Jianjun and Zhu, Lei and Andre, Philippe and Dowell, C. Darren and Falle, Sam and Tsukamoto, Yusuke}},
  issn         = {{0004-637X}},
  journal      = {{ASTROPHYSICAL JOURNAL}},
  keywords     = {{APERTURE SUBMILLIMETER TELESCOPE,FILAMENTARY MOLECULAR CLOUDS,MAGNETIC-FIELD STRUCTURE,REGULATED STAR-FORMATION,COLLAPSING DENSE,CORE,JCMT LEGACY SURVEY,H I FLOWS,350 MU-M,IMAGING POLARIMETRY,AMBIPOLAR DIFFUSION,ISM: individual objects (Orion A OMC1),polarization,stars: formation,stars: magnetic field,submillimeter: ISM}},
  language     = {{eng}},
  number       = {{1}},
  pages        = {{10}},
  title        = {{First results from BISTRO : a SCUBA-2 polarimeter survey of the Gould Belt}},
  url          = {{http://doi.org/10.3847/1538-4357/aa70a0}},
  volume       = {{842}},
  year         = {{2017}},
}

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