The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C

Junhao Liu; Keping Qiu; David Berry; James Di Francesco; Pierre Bastien; Patrick M. Koch; Ray S. Furuya; Kee Tae Kim; Simon Coudé; Chang Won Lee; Archana Soam; Chakali Eswaraiah; Di Li; Jihye Hwang; A. Ran Lyo; Kate Pattle; Tetsuo Hasegawa; Woojin Kwon; Shih Ping Lai; Derek Ward-Thompson; Tao Chung Ching; Zhiwei Chen; Qilao Gu; Dalei Li; Hua Bai Li; Hong Li Liu; Lei Qian; Hongchi Wang; Jinghua Yuan; Chuan Peng Zhang; Guoyin Zhang; Ya Peng Zhang; Jianjun Zhou; Lei Zhu; Philippe André; Doris Arzoumanian; Yusuke Aso; Do Young Byun; Michael Chun Yuan Chen; Huei Ru Vivien Chen; Wen Ping Chen; Jungyeon Cho; Minho Choi; Antonio Chrysostomou; Eun Jung Chung; Yasuo Doi; Emily Drabek-Maunder; C. Darren Dowell; Stewart P.S. Eyres; Sam Falle; Lapo Fanciullo; Jason Fiege; Erica Franzmann; Per Friberg; Rachel K. Friesen; Gary Fuller; Tim Gledhill; Sarah F. Graves; Jane S. Greaves; Matt J. Griffin; Ilseung Han; Jennifer Hatchell; Saeko S. Hayashi; Thiem Hoang; Wayne Holland; Martin Houde; Tsuyoshi Inoue; Shu Ichiro Inutsuka; Kazunari Iwasaki; Il Gyo Jeong; Doug Johnstone; Yoshihiro Kanamori; Ji Hyun Kang; Miju Kang; Sung Ju Kang; Akimasa Kataoka; Koji S. Kawabata; Francisca Kemper; Gwanjeong Kim; Jongsoo Kim; Kyoung Hee Kim; Mi Ryang Kim; Shinyoung Kim; Jason M. Kirk; Masato I.N. Kobayashi; Takayoshi Kusune; Jungmi Kwon; Kevin M. Lacaille; Chin Fei Lee; Jeong Eun Lee; Hyeseung Lee; Sang Sung Lee; Sheng Yuan Liu; Tie Liu; Sven Van Loo; Steve Mairs; Masafumi Matsumura; Brenda C. Matthews; Gerald H. Moriarty-Schieven; Tetsuya Nagata; Fumitaka Nakamura; Hiroyuki Nakanishi; Nagayoshi Ohashi; Takashi Onaka; Josh Parker; Harriet Parsons; Enzo Pascale; Nicolas Peretto; Andy Pon; Tae Soo Pyo; Ramprasad Rao; Mark G. Rawlings; Brendan Retter; John Richer; Andrew Rigby; Jean François Robitaille; Sarah Sadavoy; Hiro Saito; Giorgio Savini; Anna M.M. Scaife; Masumichi Seta; Hiroko Shinnaga; Motohide Tamura; Ya Wen Tang; Kohji Tomisaka; Yusuke Tsukamoto; Jia Wei Wang; Anthony P. Whitworth; Hsi Wei Yen; Hyunju Yoo; Tetsuya Zenko

doi:10.3847/1538-4357/ab0958

The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C

Junhao Liu, Keping Qiu, David Berry, James Di Francesco, Pierre Bastien, Patrick M. Koch, Ray S. Furuya, Kee Tae Kim, Simon Coudé, Chang Won Lee, Archana Soam, Chakali Eswaraiah, Di Li, Jihye Hwang, A. Ran Lyo, Kate Pattle, Tetsuo Hasegawa, Woojin Kwon, Shih Ping Lai, Derek Ward-ThompsonTao Chung Ching, Zhiwei Chen, Qilao Gu, Dalei Li, Hua Bai Li, Hong Li Liu, Lei Qian, Hongchi Wang, Jinghua Yuan, Chuan Peng Zhang, Guoyin Zhang, Ya Peng Zhang, Jianjun Zhou, Lei Zhu, Philippe André, Doris Arzoumanian, Yusuke Aso, Do Young Byun, Michael Chun Yuan Chen, Huei Ru Vivien Chen, Wen Ping Chen, Jungyeon Cho, Minho Choi, Antonio Chrysostomou, Eun Jung Chung, Yasuo Doi, Emily Drabek-Maunder, C. Darren Dowell, Stewart P.S. Eyres, Sam Falle, Lapo Fanciullo, Jason Fiege, Erica Franzmann, Per Friberg, Rachel K. Friesen, Gary Fuller, Tim Gledhill, Sarah F. Graves, Jane S. Greaves, Matt J. Griffin, Ilseung Han, Jennifer Hatchell, Saeko S. Hayashi, Thiem Hoang, Wayne Holland, Martin Houde, Tsuyoshi Inoue, Shu Ichiro Inutsuka, Kazunari Iwasaki, Il Gyo Jeong, Doug Johnstone, Yoshihiro Kanamori, Ji Hyun Kang, Miju Kang, Sung Ju Kang, Akimasa Kataoka, Koji S. Kawabata, Francisca Kemper, Gwanjeong Kim, Jongsoo Kim, Kyoung Hee Kim, Mi Ryang Kim, Shinyoung Kim, Jason M. Kirk, Masato I.N. Kobayashi, Takayoshi Kusune, Jungmi Kwon, Kevin M. Lacaille, Chin Fei Lee, Jeong Eun Lee, Hyeseung Lee, Sang Sung Lee, Sheng Yuan Liu, Tie Liu, Sven Van Loo, Steve Mairs, Masafumi Matsumura, Brenda C. Matthews, Gerald H. Moriarty-Schieven, Tetsuya Nagata, Fumitaka Nakamura, Hiroyuki Nakanishi, Nagayoshi Ohashi, Takashi Onaka, Josh Parker, Harriet Parsons, Enzo Pascale, Nicolas Peretto, Andy Pon, Tae Soo Pyo, Ramprasad Rao, Mark G. Rawlings, Brendan Retter, John Richer, Andrew Rigby, Jean François Robitaille, Sarah Sadavoy, Hiro Saito, Giorgio Savini, Anna M.M. Scaife, Masumichi Seta, Hiroko Shinnaga, Motohide Tamura, Ya Wen Tang, Kohji Tomisaka, Yusuke Tsukamoto, Jia Wei Wang, Anthony P. Whitworth, Hsi Wei Yen, Hyunju Yoo, Tetsuya Zenko

Research output: Contribution to journal › Article › peer-review

40 Citations (Scopus)

Abstract

We report 850 μm dust polarization observations of a low-mass (∼12 M _o) starless core in the ρ Ophiuchus cloud, Ophiuchus C, made with the POL-2 instrument on the James Clerk Maxwell Telescope (JCMT) as part of the JCMT B-fields In STar-forming Region Observations survey. We detect an ordered magnetic field projected on the plane of the sky in the starless core. The magnetic field across the ∼0.1 pc core shows a predominant northeast-southwest orientation centering between ∼40° and ∼100°, indicating that the field in the core is well aligned with the magnetic field in lower-density regions of the cloud probed by near-infrared observations and also the cloud-scale magnetic field traced by Planck observations. The polarization percentage (P) decreases with increasing total intensity (I), with a power-law index of -1.03 ± 0.05. We estimate the plane-of-sky field strength (B _pos) using modified Davis-Chandrasekhar-Fermi methods based on structure function (SF), autocorrelation function (ACF), and unsharp masking (UM) analyses. We find that the estimates from the SF, ACF, and UM methods yield strengths of 103 ± 46 μG, 136 ± 69 μG, and 213 ± 115 μG, respectively. Our calculations suggest that the Ophiuchus C core is near magnetically critical or slightly magnetically supercritical (i.e., unstable to collapse). The total magnetic energy calculated from the SF method is comparable to the turbulent energy in Ophiuchus C, while the ACF method and the UM method only set upper limits for the total magnetic energy because of large uncertainties.

Original language	English
Article number	43
Journal	Astrophysical Journal
Volume	877
Issue number	1
DOIs	https://doi.org/10.3847/1538-4357/ab0958
Publication status	Published - 20 May 2019

Bibliographical note

Publisher Copyright:
© 2019. The American Astronomical Society. All rights reserved..

Keywords

ISM: individual objects (Ophiuchus)
magnetic fields
polarization
stars: formation

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10.3847/1538-4357/ab0958

Cite this

Liu, J., Qiu, K., Berry, D., Di Francesco, J., Bastien, P., Koch, P. M., Furuya, R. S., Kim, K. T., Coudé, S., Lee, C. W., Soam, A., Eswaraiah, C., Li, D., Hwang, J., Lyo, A. R., Pattle, K., Hasegawa, T., Kwon, W., Lai, S. P., ... Zenko, T. (2019). The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C. Astrophysical Journal, 877(1), Article 43. https://doi.org/10.3847/1538-4357/ab0958

@article{77584fe69f134a80b1453999f234f1b8,

title = "The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C",

abstract = "We report 850 μm dust polarization observations of a low-mass (∼12 M o) starless core in the ρ Ophiuchus cloud, Ophiuchus C, made with the POL-2 instrument on the James Clerk Maxwell Telescope (JCMT) as part of the JCMT B-fields In STar-forming Region Observations survey. We detect an ordered magnetic field projected on the plane of the sky in the starless core. The magnetic field across the ∼0.1 pc core shows a predominant northeast-southwest orientation centering between ∼40° and ∼100°, indicating that the field in the core is well aligned with the magnetic field in lower-density regions of the cloud probed by near-infrared observations and also the cloud-scale magnetic field traced by Planck observations. The polarization percentage (P) decreases with increasing total intensity (I), with a power-law index of -1.03 ± 0.05. We estimate the plane-of-sky field strength (B pos) using modified Davis-Chandrasekhar-Fermi methods based on structure function (SF), autocorrelation function (ACF), and unsharp masking (UM) analyses. We find that the estimates from the SF, ACF, and UM methods yield strengths of 103 ± 46 μG, 136 ± 69 μG, and 213 ± 115 μG, respectively. Our calculations suggest that the Ophiuchus C core is near magnetically critical or slightly magnetically supercritical (i.e., unstable to collapse). The total magnetic energy calculated from the SF method is comparable to the turbulent energy in Ophiuchus C, while the ACF method and the UM method only set upper limits for the total magnetic energy because of large uncertainties.",

keywords = "ISM: individual objects (Ophiuchus), magnetic fields, polarization, stars: formation",

author = "Junhao Liu and Keping Qiu and David Berry and {Di Francesco}, James and Pierre Bastien and Koch, {Patrick M.} and Furuya, {Ray S.} and Kim, {Kee Tae} and Simon Coud{\'e} and Lee, {Chang Won} and Archana Soam and Chakali Eswaraiah and Di Li and Jihye Hwang and Lyo, {A. Ran} and Kate Pattle and Tetsuo Hasegawa and Woojin Kwon and Lai, {Shih Ping} and Derek Ward-Thompson and Ching, {Tao Chung} and Zhiwei Chen and Qilao Gu and Dalei Li and Li, {Hua Bai} and Liu, {Hong Li} and Lei Qian and Hongchi Wang and Jinghua Yuan and Zhang, {Chuan Peng} and Guoyin Zhang and Zhang, {Ya Peng} and Jianjun Zhou and Lei Zhu and Philippe Andr{\'e} and Doris Arzoumanian and Yusuke Aso and Byun, {Do Young} and Chen, {Michael Chun Yuan} and Chen, {Huei Ru Vivien} and Chen, {Wen Ping} and Jungyeon Cho and Minho Choi and Antonio Chrysostomou and Chung, {Eun Jung} and Yasuo Doi and Emily Drabek-Maunder and Dowell, {C. Darren} and Eyres, {Stewart P.S.} and Sam Falle and Lapo Fanciullo and Jason Fiege and Erica Franzmann and Per Friberg and Friesen, {Rachel K.} and Gary Fuller and Tim Gledhill and Graves, {Sarah F.} and Greaves, {Jane S.} and Griffin, {Matt J.} and Ilseung Han and Jennifer Hatchell and Hayashi, {Saeko S.} and Thiem Hoang and Wayne Holland and Martin Houde and Tsuyoshi Inoue and Inutsuka, {Shu Ichiro} and Kazunari Iwasaki and Jeong, {Il Gyo} and Doug Johnstone and Yoshihiro Kanamori and Kang, {Ji Hyun} and Miju Kang and Kang, {Sung Ju} and Akimasa Kataoka and Kawabata, {Koji S.} and Francisca Kemper and Gwanjeong Kim and Jongsoo Kim and Kim, {Kyoung Hee} and Kim, {Mi Ryang} and Shinyoung Kim and Kirk, {Jason M.} and Kobayashi, {Masato I.N.} and Takayoshi Kusune and Jungmi Kwon and Lacaille, {Kevin M.} and Lee, {Chin Fei} and Lee, {Jeong Eun} and Hyeseung Lee and Lee, {Sang Sung} and Liu, {Sheng Yuan} and Tie Liu and {Van Loo}, Sven and Steve Mairs and Masafumi Matsumura and Matthews, {Brenda C.} and Moriarty-Schieven, {Gerald H.} and Tetsuya Nagata and Fumitaka Nakamura and Hiroyuki Nakanishi and Nagayoshi Ohashi and Takashi Onaka and Josh Parker and Harriet Parsons and Enzo Pascale and Nicolas Peretto and Andy Pon and Pyo, {Tae Soo} and Ramprasad Rao and Rawlings, {Mark G.} and Brendan Retter and John Richer and Andrew Rigby and Robitaille, {Jean Fran{\c c}ois} and Sarah Sadavoy and Hiro Saito and Giorgio Savini and Scaife, {Anna M.M.} and Masumichi Seta and Hiroko Shinnaga and Motohide Tamura and Tang, {Ya Wen} and Kohji Tomisaka and Yusuke Tsukamoto and Wang, {Jia Wei} and Whitworth, {Anthony P.} and Yen, {Hsi Wei} and Hyunju Yoo and Tetsuya Zenko",

year = "2019",

month = may,

day = "20",

doi = "10.3847/1538-4357/ab0958",

language = "English",

volume = "877",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1",

}

Liu, J, Qiu, K, Berry, D, Di Francesco, J, Bastien, P, Koch, PM, Furuya, RS, Kim, KT, Coudé, S, Lee, CW, Soam, A, Eswaraiah, C, Li, D, Hwang, J, Lyo, AR, Pattle, K, Hasegawa, T, Kwon, W, Lai, SP, Ward-Thompson, D, Ching, TC, Chen, Z, Gu, Q, Li, D, Li, HB, Liu, HL, Qian, L, Wang, H, Yuan, J, Zhang, CP, Zhang, G, Zhang, YP, Zhou, J, Zhu, L, André, P, Arzoumanian, D, Aso, Y, Byun, DY, Chen, MCY, Chen, HRV, Chen, WP, Cho, J, Choi, M, Chrysostomou, A, Chung, EJ, Doi, Y, Drabek-Maunder, E, Dowell, CD, Eyres, SPS, Falle, S, Fanciullo, L, Fiege, J, Franzmann, E, Friberg, P, Friesen, RK, Fuller, G, Gledhill, T, Graves, SF, Greaves, JS, Griffin, MJ, Han, I, Hatchell, J, Hayashi, SS, Hoang, T, Holland, W, Houde, M, Inoue, T, Inutsuka, SI, Iwasaki, K, Jeong, IG, Johnstone, D, Kanamori, Y, Kang, JH, Kang, M, Kang, SJ, Kataoka, A, Kawabata, KS, Kemper, F, Kim, G, Kim, J, Kim, KH, Kim, MR, Kim, S, Kirk, JM, Kobayashi, MIN, Kusune, T, Kwon, J, Lacaille, KM, Lee, CF, Lee, JE, Lee, H, Lee, SS, Liu, SY, Liu, T, Van Loo, S, Mairs, S, Matsumura, M, Matthews, BC, Moriarty-Schieven, GH, Nagata, T, Nakamura, F, Nakanishi, H, Ohashi, N, Onaka, T, Parker, J, Parsons, H, Pascale, E, Peretto, N, Pon, A, Pyo, TS, Rao, R, Rawlings, MG, Retter, B, Richer, J, Rigby, A, Robitaille, JF, Sadavoy, S, Saito, H, Savini, G, Scaife, AMM, Seta, M, Shinnaga, H, Tamura, M, Tang, YW, Tomisaka, K, Tsukamoto, Y, Wang, JW, Whitworth, AP, Yen, HW, Yoo, H & Zenko, T 2019, 'The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C', Astrophysical Journal, vol. 877, no. 1, 43. https://doi.org/10.3847/1538-4357/ab0958

TY - JOUR

T1 - The JCMT BISTRO Survey

T2 - The Magnetic Field in the Starless Core ρ Ophiuchus C

AU - Liu, Junhao

AU - Qiu, Keping

AU - Berry, David

AU - Di Francesco, James

AU - Bastien, Pierre

AU - Koch, Patrick M.

AU - Furuya, Ray S.

AU - Kim, Kee Tae

AU - Coudé, Simon

AU - Lee, Chang Won

AU - Soam, Archana

AU - Eswaraiah, Chakali

AU - Li, Di

AU - Hwang, Jihye

AU - Lyo, A. Ran

AU - Pattle, Kate

AU - Hasegawa, Tetsuo

AU - Kwon, Woojin

AU - Lai, Shih Ping

AU - Ward-Thompson, Derek

AU - Ching, Tao Chung

AU - Chen, Zhiwei

AU - Gu, Qilao

AU - Li, Dalei

AU - Li, Hua Bai

AU - Liu, Hong Li

AU - Qian, Lei

AU - Wang, Hongchi

AU - Yuan, Jinghua

AU - Zhang, Chuan Peng

AU - Zhang, Guoyin

AU - Zhang, Ya Peng

AU - Zhou, Jianjun

AU - Zhu, Lei

AU - André, Philippe

AU - Arzoumanian, Doris

AU - Aso, Yusuke

AU - Byun, Do Young

AU - Chen, Michael Chun Yuan

AU - Chen, Huei Ru Vivien

AU - Chen, Wen Ping

AU - Cho, Jungyeon

AU - Choi, Minho

AU - Chrysostomou, Antonio

AU - Chung, Eun Jung

AU - Doi, Yasuo

AU - Drabek-Maunder, Emily

AU - Dowell, C. Darren

AU - Eyres, Stewart P.S.

AU - Falle, Sam

AU - Fanciullo, Lapo

AU - Fiege, Jason

AU - Franzmann, Erica

AU - Friberg, Per

AU - Friesen, Rachel K.

AU - Fuller, Gary

AU - Gledhill, Tim

AU - Graves, Sarah F.

AU - Greaves, Jane S.

AU - Griffin, Matt J.

AU - Han, Ilseung

AU - Hatchell, Jennifer

AU - Hayashi, Saeko S.

AU - Hoang, Thiem

AU - Holland, Wayne

AU - Houde, Martin

AU - Inoue, Tsuyoshi

AU - Inutsuka, Shu Ichiro

AU - Iwasaki, Kazunari

AU - Jeong, Il Gyo

AU - Johnstone, Doug

AU - Kanamori, Yoshihiro

AU - Kang, Ji Hyun

AU - Kang, Miju

AU - Kang, Sung Ju

AU - Kataoka, Akimasa

AU - Kawabata, Koji S.

AU - Kemper, Francisca

AU - Kim, Gwanjeong

AU - Kim, Jongsoo

AU - Kim, Kyoung Hee

AU - Kim, Mi Ryang

AU - Kim, Shinyoung

AU - Kirk, Jason M.

AU - Kobayashi, Masato I.N.

AU - Kusune, Takayoshi

AU - Kwon, Jungmi

AU - Lacaille, Kevin M.

AU - Lee, Chin Fei

AU - Lee, Jeong Eun

AU - Lee, Hyeseung

AU - Lee, Sang Sung

AU - Liu, Sheng Yuan

AU - Liu, Tie

AU - Van Loo, Sven

AU - Mairs, Steve

AU - Matsumura, Masafumi

AU - Matthews, Brenda C.

AU - Moriarty-Schieven, Gerald H.

AU - Nagata, Tetsuya

AU - Nakamura, Fumitaka

AU - Nakanishi, Hiroyuki

AU - Ohashi, Nagayoshi

AU - Onaka, Takashi

AU - Parker, Josh

AU - Parsons, Harriet

AU - Pascale, Enzo

AU - Peretto, Nicolas

AU - Pon, Andy

AU - Pyo, Tae Soo

AU - Rao, Ramprasad

AU - Rawlings, Mark G.

AU - Retter, Brendan

AU - Richer, John

AU - Rigby, Andrew

AU - Robitaille, Jean François

AU - Sadavoy, Sarah

AU - Saito, Hiro

AU - Savini, Giorgio

AU - Scaife, Anna M.M.

AU - Seta, Masumichi

AU - Shinnaga, Hiroko

AU - Tamura, Motohide

AU - Tang, Ya Wen

AU - Tomisaka, Kohji

AU - Tsukamoto, Yusuke

AU - Wang, Jia Wei

AU - Whitworth, Anthony P.

AU - Yen, Hsi Wei

AU - Yoo, Hyunju

AU - Zenko, Tetsuya

PY - 2019/5/20

Y1 - 2019/5/20

N2 - We report 850 μm dust polarization observations of a low-mass (∼12 M o) starless core in the ρ Ophiuchus cloud, Ophiuchus C, made with the POL-2 instrument on the James Clerk Maxwell Telescope (JCMT) as part of the JCMT B-fields In STar-forming Region Observations survey. We detect an ordered magnetic field projected on the plane of the sky in the starless core. The magnetic field across the ∼0.1 pc core shows a predominant northeast-southwest orientation centering between ∼40° and ∼100°, indicating that the field in the core is well aligned with the magnetic field in lower-density regions of the cloud probed by near-infrared observations and also the cloud-scale magnetic field traced by Planck observations. The polarization percentage (P) decreases with increasing total intensity (I), with a power-law index of -1.03 ± 0.05. We estimate the plane-of-sky field strength (B pos) using modified Davis-Chandrasekhar-Fermi methods based on structure function (SF), autocorrelation function (ACF), and unsharp masking (UM) analyses. We find that the estimates from the SF, ACF, and UM methods yield strengths of 103 ± 46 μG, 136 ± 69 μG, and 213 ± 115 μG, respectively. Our calculations suggest that the Ophiuchus C core is near magnetically critical or slightly magnetically supercritical (i.e., unstable to collapse). The total magnetic energy calculated from the SF method is comparable to the turbulent energy in Ophiuchus C, while the ACF method and the UM method only set upper limits for the total magnetic energy because of large uncertainties.

AB - We report 850 μm dust polarization observations of a low-mass (∼12 M o) starless core in the ρ Ophiuchus cloud, Ophiuchus C, made with the POL-2 instrument on the James Clerk Maxwell Telescope (JCMT) as part of the JCMT B-fields In STar-forming Region Observations survey. We detect an ordered magnetic field projected on the plane of the sky in the starless core. The magnetic field across the ∼0.1 pc core shows a predominant northeast-southwest orientation centering between ∼40° and ∼100°, indicating that the field in the core is well aligned with the magnetic field in lower-density regions of the cloud probed by near-infrared observations and also the cloud-scale magnetic field traced by Planck observations. The polarization percentage (P) decreases with increasing total intensity (I), with a power-law index of -1.03 ± 0.05. We estimate the plane-of-sky field strength (B pos) using modified Davis-Chandrasekhar-Fermi methods based on structure function (SF), autocorrelation function (ACF), and unsharp masking (UM) analyses. We find that the estimates from the SF, ACF, and UM methods yield strengths of 103 ± 46 μG, 136 ± 69 μG, and 213 ± 115 μG, respectively. Our calculations suggest that the Ophiuchus C core is near magnetically critical or slightly magnetically supercritical (i.e., unstable to collapse). The total magnetic energy calculated from the SF method is comparable to the turbulent energy in Ophiuchus C, while the ACF method and the UM method only set upper limits for the total magnetic energy because of large uncertainties.

KW - ISM: individual objects (Ophiuchus)

KW - magnetic fields

KW - polarization

KW - stars: formation

UR - http://www.scopus.com/inward/record.url?scp=85068692356&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/ab0958

DO - 10.3847/1538-4357/ab0958

M3 - Article

AN - SCOPUS:85068692356

SN - 0004-637X

VL - 877

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 43

ER -

The JCMT BISTRO Survey: The Magnetic Field in the Starless Core ρ Ophiuchus C

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Keywords

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