Figure 2 from The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry

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The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry

Authors: Chakali Eswaraiah, Di Li, Ray S. Furuya, Tetsuo Hasegawa, Derek Ward-Thompson, Keping Qiu, Nagayoshi Ohashi, Kate Pattle, Sarah Sadavoy, Charles L. H. Hull, David Berry, Yasuo Doi, Tao-Chung Ching, Shih-Ping Lai, Jia-Wei Wang, Patrick M. Koch, Jungmi Kwon, Woojin Kwon, Pierre Bastien, Doris Arzoumanian, Simon Coudé, Archana Soam, Lapo Fanciullo, Hsi-Wei Yen, Junhao Liu, Thiem Hoang, Wen Ping Chen, Yoshito Shimajiri, Tie Liu, Zhiwei Chen, Hua-bai Li, A-Ran Lyo, Jihye Hwang, Doug Johnstone, Ramprasad Rao, Nguyen Bich Ngoc, Pham Ngoc Diep, Steve Mairs, Harriet Parsons, Motohide Tamura, Mehrnoosh Tahani, Huei-Ru Vivien Chen, Fumitaka Nakamura, Hiroko Shinnaga, Ya-Wen Tang, Jungyeon Cho, Chang Won Lee, Shu-ichiro Inutsuka, Tsuyoshi Inoue, Kazunari Iwasaki, Lei Qian, Jinjin Xie, Dalei Li, Hong-Li Liu, Chuan-Peng Zhang, Mike Chen, Guoyin Zhang, Lei Zhu, Jianjun Zhou, Philippe André, Sheng-Yuan Liu, Jinghua Yuan, Xing Lu, Nicolas Peretto, Tyler L. Bourke, Do-Young Byun, Sophia Dai, Yan Duan, Hao-Yuan Duan, David Eden, Brenda Matthews, Jason Fiege, Laura M. Fissel, Kee-Tae Kim, Chin-Fei Lee, Jongsoo Kim, Tae-Soo Pyo, Yunhee Choi, Minho Choi, Antonio Chrysostomou, Eun Jung Chung, Le Ngoc Tram, Erica Franzmann, Per Friberg, Rachel Friesen, Gary Fuller, Tim Gledhill, Sarah Graves, Jane Greaves, Matt Griffin, Qilao Gu, Ilseung Han, Jennifer Hatchell, Saeko Hayashi, Martin Houde, Koji Kawabata, Il-Gyo Jeong, Ji-hyun Kang, Sung-ju Kang, Miju Kang, Akimasa Kataoka, Francisca Kemper, Mark Rawlings, Jonathan Rawlings, Brendan Retter, John Richer, Andrew Rigby, Hiro Saito, Giorgio Savini, Anna Scaife, Masumichi Seta, Gwanjeong Kim, Kyoung Hee Kim, Mi-Ryang Kim, Florian Kirchschlager, Jason Kirk, Masato I. N. Kobayashi, Vera Konyves, Takayoshi Kusune, Kevin Lacaille, Chi-Yan Law, Sang-Sung Lee, Yong-Hee Lee, Masafumi Matsumura, Gerald Moriarty-Schieven, Tetsuya Nagata, Hiroyuki Nakanishi, Takashi Onaka, Geumsook Park, Xindi Tang, Kohji Tomisaka, Yusuke Tsukamoto, Serena Viti, Hongchi Wang, Anthony Whitworth, Hyunju Yoo, Hyeong-Sik Yun, Tetsuya Zenko, Yapeng Zhang, Ilse de Looze, C. Darren Dowell, Stewart Eyres, Sam Falle, Jean-François Robitaille, and Sven van Loo

2021 The Astrophysical Journal Letters 912 L27.

Provider: AAS Journals

Caption: Figure 2.

Same as Figure 1(b) but now we only show the mean B-field orientation in the three cores K04166, Miz-8b, and K04169, based on the weighted mean of the PAs we measure. The blue and red dashed arrows denote the protostellar outflows (lengths are not to scale) emanating from K04166 and K04169. The red contour around each core is drawn at I = 13 mJy beam⁻¹, corresponding to 10σ in total intensity. The large-scale B-field morphology, as determined from the oversampled Planck 850 μm polarization data (pixel size 1′), is shown as yellow segments. The white contour is as described in Figure 1(b).

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