Erratum: Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions

An Erratum on
Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions

by Pattle, K., and Fissel, L. (2019). Front. Astron. Space Sci. 6:15. doi: 10.3389/fspas.2019.00015

Due to a production error, a copyrighted figure was used as part of Figure 4 in the original article. This figure and the corresponding part label have been removed from the article and the updated Figure 4 can be seen below.

FIGURE 4

Figure 4. Polarization observations of the Vela C cloud from the BLASTPol telescope. (A) Magnetic field orientation (texture) inferred from the BLASTPol 500 μm data overlaid on a Herschel-derived column density (N_H) map—Soler et al. (2017), reproduced with permission © ESO. Four sub-region are labeled, while the shaded pink region indicates where the dust is heated by a compact H_II region. (B) Map of polarized intensity with contours of total intensity (green) overlaid (from Figure 3 of Fissel et al., 2016© AAS. Reproduced with permission).

The publisher apologizes for this error and states that this does not change the scientific conclusions of the article in any way. The original version of this article was updated on July 4th, 2019.

References

Fissel, L. M., Ade, P. A. R., Angilè, F. E., Ashton, P., Benton, S. J., Devlin, M. J., et al. (2016). Balloon-borne submillimeter polarimetry of the Vela C molecular cloud: systematic dependence of polarization fraction on column density and local polarization-angle dispersion. Astrophys. J. 824:134. doi: 10.3847/0004-637X/824/2/134

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Soler, J. D., Ade, P. A. R., Angilè, F. E., Ashton, P., Benton, S. J., Devlin, M. J., et al. (2017). The relation between the column density structures and the magnetic field orientation in the Vela C molecular complex. Astron. Astrophys. 603:A64. doi: 10.1051/0004-6361/201730608

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