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  • Eswaraiah, ChakaliChinese Academy of Sciences (author)

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

  • Article/chapterEnglish2021

Publisher, publication year, extent ...

  • 2021-05-10
  • American Astronomical Society,2021
  • electronicrdacarrier

Numbers

  • LIBRIS-ID:oai:research.chalmers.se:3d99a7fe-c320-4219-b89b-d11b5af4430c
  • https://doi.org/10.3847/2041-8213/abeb1cDOI
  • https://research.chalmers.se/publication/524182URI

Supplementary language notes

  • Language:English
  • Summary in:English

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  • Subject category:art swepub-publicationtype
  • Subject category:ref swepub-contenttype

Notes

  • We have obtained sensitive dust continuum polarization observations at 850 μm in the B213 region of Taurus using POL-2 on SCUBA-2 at the James Clerk Maxwell Telescope as part of the B-fields in STar-forming Region Observations (BISTRO) survey. These observations allow us to probe magnetic field (B-field) at high spatial resolution (∼2000 au or ∼0.01 pc at 140 pc) in two protostellar cores (K04166 and K04169) and one prestellar core (Miz-8b) that lie within the B213 filament. Using the Davis-Chandrasekhar-Fermi method, we estimate the B-field strengths in K04166, K04169, and Miz-8b to be 38 ± 14, 44 ± 16, and 12 ± 5 μG, respectively. These cores show distinct mean B-field orientations. The B-field in K04166 is well ordered and aligned parallel to the orientations of the core minor axis, outflows, core rotation axis, and large-scale uniform B-field, in accordance with magnetically regulated star formation via ambipolar diffusion taking place in K04166. The B-field in K04169 is found to be ordered but oriented nearly perpendicular to the core minor axis and large-scale B-field and not well correlated with other axes. In contrast, Miz-8b exhibits a disordered B-field that shows no preferred alignment with the core minor axis or large-scale field. We found that only one core, K04166, retains a memory of the large-scale uniform B-field. The other two cores, K04169 and Miz-8b, are decoupled from the large-scale field. Such a complex B-field configuration could be caused by gas inflow onto the filament, even in the presence of a substantial magnetic flux.

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  • Li, D.Chinese Academy of Sciences (author)
  • Furuya, Ray S.Tokushima University (author)
  • Hasegawa, TetsuoNational Astronomical Observatory of Japan (author)
  • Ward-Thompson, D.University of Central Lancashire (author)
  • Qiu, KepingNanjing University (author)
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  • Pattle, KateNational University of Ireland (author)
  • Sadavoy, S. I.Queen's University (author)
  • Hull, Charles L. H.National Astronomical Observatory of Japan (author)
  • Berry, DavidEast Asian Observatory (author)
  • Doi, YasuoUniversity of Tokyo, Japan (author)
  • Ching, Tao-ChungChinese Academy of Sciences (author)
  • Lai, Shih-PingNational Tsing Hua University (author)
  • Wang, Jia-WeiAcademia Sinica Taiwan (author)
  • Koch, Patrick M.Academia Sinica Taiwan (author)
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  • Rawlings, M.G.East Asian Observatory (author)
  • Rawlings, J. M.C.University College London (UCL) (author)
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  • Savini, GiorgioUniversity College London (UCL) (author)
  • Scaife, A. M. M.University of Manchester (author)
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  • Kim, Kyoung HeeKorea Astronomy and Space Science Institute (author)
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  • Kirchschlager, F.University College London (UCL) (author)
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  • Kobayashi, Masato I. N.Tohoku University (author)
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  • Lacaille, KevinMcMaster University (author)
  • Law, Chi Yan,1990Chalmers tekniska högskola,Chalmers University of Technology,Chinese University of Hong Kong(Swepub:cth)ychi (author)
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  • Tang, X. D.Chinese Academy of Sciences (author)
  • Tomisaka, KohjiNational Astronomical Observatory of Japan (author)
  • Tsukamoto, YusukeKagoshima University (author)
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  • Whitworth, AnthonyCardiff University (author)
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  • Zenko, Tetsuya (author)
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  • De Looze, I.University College London (UCL) (author)
  • Dowell, C. D. (author)
  • Eyres, S.University of South Wales (author)
  • Robitaille, Jean-FrançoisUniversité Grenoble Alpes,Grenoble Alpes University (author)
  • Van Loo, SvenUniversity of Leeds (author)
  • Chinese Academy of SciencesTokushima University (creator_code:org_t)

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  • In:Astrophysical Journal Letters: American Astronomical Society912:22041-82132041-8205

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