Fig. A.2
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Magnetic fields, polarized intensity, and molecular line observations around the L1448 IRS2 Class 0 protostellar core (as in Figure 2). The thick light blue contours (top right and bottom panels) trace the moment 0 map of the CS (by integrating emission from 2 to 6 km s−1) molecular emission spectral line. The ALMA 1.3mm dust polarized emission is from Kwon et al. (2019) and the CS emission line is from ALMA project 2016.1.01501.S, Y. Zhang (in prep.).
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