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arXiv · 1202.4635

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

Ya-Wen Tang·Patrick M. Koch·Paul T. P. Ho
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Abstract

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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Ya-Wen Tang, Patrick M. Koch, Paul T. P. Ho. 2012-02-21. Observations and Analysis of High-Resolution Magnetic Field Structures in Molecular Clouds. https://arxiv.org/abs/1202.4635

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