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. 2018 Nov 6;9:4636. doi: 10.1038/s41467-018-07143-8

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© The Author(s) 2018

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

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Fig. 5 — Possible toroidal fields in the HH 211 jet. Yellow line segments indicate the possible toroidal fields obtained by rotating the polarization orientations by 90°. The asterisk marks the position of the central driving source. Blue image with the blue contours shows the blueshifted jet component. Red image with the red contours shows the redshifted jet component. The contour levels are the same as in Fig. 2