Magnetic field properties in star formation: A review of their analysis methods and interpretation

Magnetic field properties in star formation: A review of their analysis methods and interpretation

Linearly polarized emission from dust grains and molecular spectroscopy is an effective probe of the magnetic field topology in the interstellar medium and molecular clouds. The longstanding Davis-Chandrasekhar-Fermi (DCF) method and the recently developed Histogram of Relative Orientations (HRO) an...

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Bibliographic Details
Main Authors: Junhao Liu, Qizhou Zhang, Keping Qiu
Format: Article
Language:English
Published: Frontiers Media S.A. 2022-09-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
star formation
magnetic fields
polarization
molecular clouds
interstellar medium
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2022.943556/full

Internet

https://www.frontiersin.org/articles/10.3389/fspas.2022.943556/full

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