Sökning: onr:"swepub:oai:research.chalmers.se:3d99a7fe-c320-4219-b89b-d11b5af4430c" > The JCMT BISTRO Sur...
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000 | 13184naa a2202065 4500 | |
001 | oai:research.chalmers.se:3d99a7fe-c320-4219-b89b-d11b5af4430c | |
003 | SwePub | |
008 | 210601s2021 | |||||||||||000 ||eng| | |
024 | 7 | a https://doi.org/10.3847/2041-8213/abeb1c2 DOI |
024 | 7 | a https://research.chalmers.se/publication/5241822 URI |
040 | a (SwePub)cth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a art2 swepub-publicationtype |
072 | 7 | a ref2 swepub-contenttype |
100 | 1 | a Eswaraiah, Chakaliu Chinese Academy of Sciences4 aut |
245 | 1 0 | a The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry |
264 | c 2021-05-10 | |
264 | 1 | b American Astronomical Society,c 2021 |
338 | a electronic2 rdacarrier | |
520 | a 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. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Annan fysik0 (SwePub)103992 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Other Physics Topics0 (SwePub)103992 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng |
700 | 1 | a Li, D.u Chinese Academy of Sciences4 aut |
700 | 1 | a Furuya, Ray S.u Tokushima University4 aut |
700 | 1 | a Hasegawa, Tetsuou National Astronomical Observatory of Japan4 aut |
700 | 1 | a Ward-Thompson, D.u University of Central Lancashire4 aut |
700 | 1 | a Qiu, Kepingu Nanjing University4 aut |
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700 | 1 | a Berry, Davidu East Asian Observatory4 aut |
700 | 1 | a Doi, Yasuou University of Tokyo, Japan4 aut |
700 | 1 | a Ching, Tao-Chungu Chinese Academy of Sciences4 aut |
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700 | 1 | a Wang, Jia-Weiu Academia Sinica Taiwan4 aut |
700 | 1 | a Koch, Patrick M.u Academia Sinica Taiwan4 aut |
700 | 1 | a Kwon, Jungmiu University of Tokyo, Japan4 aut |
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700 | 1 | a Jeong, Il-Gyou Korea Astronomy and Space Science Institute4 aut |
700 | 1 | a Kang, Ji-hyunu Korea Astronomy and Space Science Institute4 aut |
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700 | 1 | a Kim, Mi-Ryangu Korea Astronomy and Space Science Institute4 aut |
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700 | 1 | a Kirk, J.u University of Central Lancashire4 aut |
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700 | 1 | a Park, Geumsooku Korea Astronomy and Space Science Institute4 aut |
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700 | 1 | a Tomisaka, Kohjiu National Astronomical Observatory of Japan4 aut |
700 | 1 | a Tsukamoto, Yusukeu Kagoshima University4 aut |
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710 | 2 | a Chinese Academy of Sciencesb Tokushima University4 org |
773 | 0 | t Astrophysical Journal Lettersd : American Astronomical Societyg 912:2q 912:2x 2041-8213x 2041-8205 |
856 | 4 | u https://research.chalmers.se/publication/524182/file/524182_Fulltext.pdfx primaryx freey FULLTEXT |
856 | 4 | u https://doi.org/10.3847/2041-8213/abeb1c |
856 | 4 8 | u https://doi.org/10.3847/2041-8213/abeb1c |
856 | 4 8 | u https://research.chalmers.se/publication/524182 |
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