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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 3.

(Top panels) Velocity gradient maps for (a) K04166, (b) K04169, and (c) Miz-8b. The length and angle of each black arrow correspond to the magnitude and direction, respectively, of the local velocity gradient. A reference arrow with units of kilometers per second per parsec is shown on each plot. Red segments show the B-field orientations from Figure 1(b). (Bottom panels) Weighted mean B-field geometry (thick red segments; same as Figure 2) in the cores of (d) K04166, (e) K04169, and (f) Miz-8b, overlaid on the Stokes I map (color scale). The large-scale Planck mean B-field direction is shown as a yellow segment on each core. Red and blue contours show the redshifted and blueshifted 12CO (2–1) emission tracing the bipolar outflow in the center of each core. These were obtained with the ALMA 7 m array by Tokuda et al. (2020). The cyan line denotes the mean PA of each outflow (33° for K04166 and 58° for K04169). The thin black line represents the PA of the core rotation axis. The integrated velocity ranges are −10 to 0 and 10 to 20 km s−1 for the blue- and redshifted outflows of K04166 and −5 to 4 and 11 to 17 km s−1 for the blue- and redshifted outflows of K04169. The lowest and subsequent contour steps are 0.4 and 1.2 K km s−1 , respectively. The angular resolution of the ALMA data is 6.″8 × 6.″5.

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