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Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation

  • Authors: Charles L. H. Hull, Philip Mocz, Blakesley Burkhart, Alyssa A. Goodman, Josep M. Girart, Paulo C. Cortés, Lars Hernquist, Volker Springel, Zhi-Yun Li, and Shih-Ping Lai

2017 The Astrophysical Journal Letters 842 L9.

  • Provider: AAS Journals

Caption: Figure 4.

Polarized intensity vs. total intensity in Ser-emb 8. Values in the P vs. I plot on the left are plotted for pixels in the Ser-emb 8 ALMA map (shown on the right, and also in Figure 1(c)) where there are significant detections of both P and I (see Table 2). The gray, magenta, and orange points on the left-hand plot are associated with the points of the same color in the right-hand plot of Ser-emb 8.

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