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Cited article:

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

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Frontiers in Astronomy and Space Sciences 6 (2019)
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Polarization Properties and Magnetic Field Structures in the High-mass Star-forming Region W51 Observed with ALMA

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DUST CONTINUUM AND POLARIZATION FROM ENVELOPE TO CORES IN STAR FORMATION: A CASE STUDY IN THE W51 NORTH REGION

Ya-Wen Tang, Paul T. P. Ho, Patrick M. Koch, Stephane Guilloteau and Anne Dutrey
The Astrophysical Journal 763 (2) 135 (2013)
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MAGNETIC FIELD STRENGTH MAPS FOR MOLECULAR CLOUDS: A NEW METHOD BASED ON A POLARIZATION-INTENSITY GRADIENT RELATION

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The Astrophysical Journal 747 (1) 79 (2012)
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QUANTIFYING THE SIGNIFICANCE OF THE MAGNETIC FIELD FROM LARGE-SCALE CLOUD TO COLLAPSING CORE: SELF-SIMILARITY, MASS-TO-FLUX RATIO, AND STAR FORMATION EFFICIENCY

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Magnetic fields in the nearby Universe, as observed in solar and planetary realms, stars, and interstellar starforming nurseries

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MAGNETIC FIELD PROPERTIES IN HIGH-MASS STAR FORMATION FROM LARGE TO SMALL SCALES: A STATISTICAL ANALYSIS FROM POLARIZATION DATA

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EVOLUTION OF MAGNETIC FIELDS IN HIGH-MASS STAR FORMATION: LINKING FIELD GEOMETRY AND COLLAPSE FOR THE W51 e2/e8 CORES

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THE LEGACY OF SCUPOL: 850 μm IMAGING POLARIMETRY FROM 1997 TO 2005

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The Astrophysical Journal Supplement Series 182 (1) 143 (2009)
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New Results on the Submillimeter Polarization Spectrum of the Orion Molecular Cloud

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Submillimetre polarimetric observations of magnetic fields in star-forming regions

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Evolution of Rotating Molecular Cloud Core with Oblique Magnetic Field

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Multiscale Magnetic Fields in Star‐forming Regions: Interferometric Polarimetry of the MMS 6 Core of OMC‐3

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First polarimetry results of two candidate high-mass protostellar objects

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