Résumé
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.
- Titre
- Local Magnetic Field Role in Star Formation
- Créateurs - sans rôle
- 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 SciencesH.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 - Université de Montpellier, Laboratoire Univers et Particules de Montpellier - LUPMK Qiu - Nanjing UniversityR RaoH.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
- Détails de publication
- EAS Publ.Ser, Vol.75-76, pp.159-162
- Colloque
- Conditions and Impact of Star Formation (Zermatt, Switzerland, 07/09/2015–11/09/2015)
- Identifiants
- 99151304009311
- Unité académique
- Laboratoire Univers et Particules de Montpellier - LUPM
- Langue
- English
- Type de ressource
- Conference proceeding
- Champs locaux
- hal-04696043