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

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.

preprint2012arXivOpen access
Ya-Wen TangPatrick M. KochPaul T. P. Ho
astro-ph.GA
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Open access3 authors1 topic
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Ya-Wen TangPatrick M. KochPaul T. P. Ho

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