Fig. 4
A comparison of polarized SiO emission with polarized dust continuum emission in HH 211. The asterisk marks the position of the central driving source. Black and gray contours show the blueshifted and redshifted jet components, respectively, with their contour levels the same as in Fig. 2. Magenta line segments show the polarization orientations of the polarized SiO emission. Blue contours and orange line segments show the intensity and the orientations of the polarized emission in continuum at 350 GHz, obtained alongside in our ALMA observations (Lee et al., in preparation)
