Abstract
We highlight distinct and systematic observational features of magnetic field morphologies in polarized submm dust continuum. We illustrate this with specific examples and show statistical trends from a sample of 50 star-forming regions.
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CITATION STYLE
APA
Koch, P. M., Tang, Y. W., Ho, P. T. P., Zhang, Q., Girart, J. M., Chen, H. R. V., … Ching, T. C. (2016). Local Magnetic Field Role in Star Formation. In EAS Publications Series (Vol. 75–76, pp. 159–162). EDP Sciences. https://doi.org/10.1051/eas/1575027
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