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
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
1
FisselL. M.AdeP. A. R.AngilèF. E.AshtonP.BentonS. J.DevlinM. 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. 10.3847/0004-637X/824/2/134
2
SolerJ. D.AdeP. A. R.AngilèF. E.AshtonP.BentonS. J.DevlinM. 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. 10.1051/0004-6361/201730608
Summary
Keywords
molecular clouds, far-infrared (FIR), magnetic fields, star formation, submillimeter astronomy, polarimetry
Citation
Frontiers Production Office (2019) Erratum: Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions. Front. Astron. Space Sci. 6:58. doi: 10.3389/fspas.2019.00058
Received
14 August 2019
Accepted
15 August 2019
Published
19 August 2019
Approved by
Frontiers Editorial Office, Frontiers Media SA, Switzerland
Volume
6 - 2019
Updates
Copyright
© 2019 Frontiers Production Office.
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This article was submitted to Stellar and Solar Physics, a section of the journal Frontiers in Astronomy and Space Sciences
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