Local Magnetic Field Role in Star Formation
arXiv:1511.07116 · doi:10.1051/eas/1575027
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.
4 pages, 3 figures; to appear in the EAS Proceedings of the 6th Zermatt ISM Symposium "Conditions and Impact of Star Formation from Lab to Space", September 2015
References in corpus (6)
- TADPOL: A 1.3 mm Survey of Dust Polarization in Star-forming Cores and Regions
- Magnetic Fields and Massive Star Formation
- Submillimeter Array Observations of Magnetic Fields in G240.31+0.07: an Hourglass in a Massive Cluster-forming Core
- The Importance of the Magnetic Field from an SMA-CSO-Combined Sample of Star-Forming Regions
- From Poloidal to Toroidal: Detection of Well-ordered Magnetic Field in High-mass Proto-cluster G35.2-0.74N
- Interpreting the Role of the Magnetic Field from Dust Polarization Maps