Spatially resolved magnetic field structure in the disk of a T Tauri star-Reference-Cited by-同舟云学术

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Spatially resolved magnetic field structure in the disk of a T Tauri star

Published:2014-10-22 Issue:7524 Volume:514 Page:597-599
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Stephens Ian W.,Looney Leslie W.,Kwon Woojin,Fernández-López Manuel,Hughes A. Meredith,Mundy Lee G.,Crutcher Richard M.,Li Zhi-Yun,Rao Ramprasad

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature13850.pdf

Reference32 articles.

1. Blandford, R. D. & Payne, D. G. Hydromagnetic flows from accretion discs and the production of radio jets. Mon. Not. R. Astron. Soc. 199, 883–903 (1982)

2. Balbus, S. A. & Hawley, J. F. Instability, turbulence, and enhanced transport in accretion disks. Rev. Mod. Phys. 70, 1–53 (1998)

3. Johns-Krull, C. M. The magnetic fields of classical T Tauri stars. Astrophys. J. 664, 975–985 (2007)

4. Donati, J.-F., Paletou, F., Bouvier, J. & Ferreira, J. Direct detection of a magnetic field in the innermost regions of an accretion disk. Nature 438, 466–469 (2005)

5. Lazarian, A. Tracing magnetic fields with aligned grains. J. Quant. Spectrosc. Radiat. Transf. 106, 225–256 (2007)

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