Issue |
EAS Publications Series
Volume 75-76, 2015
Conditions and Impact of Star Formation
|
|
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Page(s) | 159 - 162 | |
Section | Star Formation: Physical and Chemical Conditions, Feedback | |
DOI | https://doi.org/10.1051/eas/1575027 | |
Published online | 20 May 2016 |
R. Simon, R. Schaaf and J. Stutzki (eds)
EAS Publications Series, 75–76 (2015) 159-162
Local Magnetic Field Role in Star Formation
1 Academia Sinica Institute of Astronomy and Astrophysics, Taipei, Taiwan
2 East Asian Observatory, 660 N. Aohoku Place, University Park, Hilo, Hawaii 96720, USA
3 Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
4 Institut de Ciències de l'Espai, Facultat de Ciències, C5p 2, 08193 Bellaterra, Catalonia
5 Inst. of Astronomy and Dep. of Physics, National Tsing Hua University, Hsinchu, Taiwan
6 Department of Physics, The Chinese University of Hong Kong
7 Department of Astronomy, University of Virginia, Charlottesville, VA 22904, USA
8 Laboratoire Univers et Particules de Montpellier, Université de Montpellier, France
9 INAF-Osservatorio Astrofisico di Arcetri, Firenze, Italy
10 School of Astronomy and Space Science, Nanjing University, Nanjiing 210093, China
11 Academia Sinica Institute of Astronomy and Astrophysics, Hilo, HI 96720, USA
12 Observatorio Astronómico Nacional, 28014 Madrid, Spain
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.
© EAS, EDP Sciences, 2016