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.
- Title
- Local Magnetic Field Role in Star Formation
- Creators - without role
- P.M. Koch - Institute of Astronomy and Astrophysics, Academia SinicaY.W. Tang - Institute of Astronomy and Astrophysics, Academia SinicaP.T.P. Ho - Institute of Astronomy and Astrophysics, Academia SinicaQ. Zhang - Center for Astrophysics Harvard & SmithsonianJ.M. Girart - Institute of Space Science - INFLPR SubsidiaryH.R.V. Chen - Institute of Astronomy and Astrophysics, Academia SinicaS.P. Lai - National Tsing Hua UniversityH.B. Li - Chinese University of Hong KongZ.Y. Li - University of VirginiaH.B. Liu - University of VirginiaM. Padovani - Arcetri Astrophysical ObservatoryK. Qiu - Nanjing UniversityR. Rao - Institute of Astronomy and Astrophysics, Academia SinicaH.W. Yen - Institute of Astronomy and Astrophysics, Academia SinicaP. Frau - Spanish National ObservatoryH.H. Chen - National Tsing Hua UniversityT.C. Ching - National Tsing Hua University
- Publication Details
- EAS Publications Series, Vol.75-76, pp.159-162
- Identifiers
- 9782759820221; 9957766446006774
- Copyright
- © 2016 EAS, EDP Sciences.
- Academic Unit
- Institute of Astronomy, College of Science, National Tsing Hua University; National Tsing Hua University
- Language
- English
- Resource Type
- Conference paper