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Observations of magnetic fields in star-forming clouds

Published online by Cambridge University Press:  03 March 2020

Juan D. Soler*
Affiliation:
Max-Planck-Institute for Astronomy, Königstuhl 17, 69117, Heidelberg, Germany. email: soler@mpia.de
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Abstract

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This review examines observations of magnetic fields in molecular clouds, that is, at spatial scales ranging from tens to tenths of parsecs and densities up to hundreds of particles per cubic centimetre. I will briefly summarize the techniques for observing and mapping magnetic fields in molecular clouds. I will review important examples of observational results obtained using each technique and their implications for our understanding of the role of the magnetic field in molecular cloud formation and evolution. Finally, I will briefly discuss the prospects for advances in our observational capabilities with telescopes and instruments now beginning operation or under construction.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Pattle, K., et al. ApJ, 846 (2017) 112P Google Scholar
Planck 2015 results I, 2016. A&A, 594 (2016) A1 Google Scholar
Planck Collaboration XXXV, 2016. A&A, 586 (2016) A138 Google Scholar
Soler, J. D., Bracco, A. & Pon, A. A&A, 609L (2018) 3S Google Scholar
Ward-Thompson, D., et al. ApJ, 842 (2017) 66W CrossRefGoogle Scholar