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Observations and Analysis of High-Resolution Magnetic Field Structures in Molecular Clouds

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arxiv 1202.4635 v1 pith:VFSVAGN2 submitted 2012-02-21 astro-ph.GA

Observations and Analysis of High-Resolution Magnetic Field Structures in Molecular Clouds

Ya-Wen Tang , Patrick M. Koch , Paul T.P. Ho This is my paper
classification astro-ph.GA
keywords fieldmagneticstructuresanalysisobservationsstararrayclouds
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Recent high-angular-resolution (up to 0.7") dust polarization observations toward star forming regions are summarized. With the Sub-Millimeter Array, the emission from the dense structures is traced and resolved. The detected magnetic field morphologies vary from hourglass-like structures to isolated patches depending on the evolutionary stage of the source. These observed features have also served as a testbed to develop new analysis methods, with a particular focus on quantifying the role of the magnetic field in the star formation process.

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