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Spatially resolved magnetic field structure in the disk of a T Tauri star
Ian W. Stephens
,
Leslie W. Looney
, Woojin Kwon
, Manuel Fernández-López
, A. Meredith Hughes
, Lee G. Mundy
,
Richard M. Crutcher
, Zhi Yun Li
, Ramprasad Rao
Astronomy
National Center for Supercomputing Applications (NCSA)
Research output
:
Contribution to journal
›
Article
›
peer-review
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Keyphrases
Magnetic Field
100%
Spatially Resolved
100%
Magnetic Field Structure
100%
T Tauri Stars
100%
Accretion Discs
50%
Astronomical Unit
50%
Angular Momentum
25%
Formation Process
25%
Field Strength
25%
Theoretical Understanding
25%
Major Axis
25%
Polarized Emission
25%
Star Formation
25%
Dust Grains
25%
Continuum Emission
25%
Vertical Component
25%
Toroidal Field
25%
Unresolved Measurement
25%
Young Stars
25%
Earth and Planetary Sciences
T Tauri Stars
100%
Emissions
66%
Accretion Disk
66%
Field Strength
33%
Angular Momentum
33%
Star Formation
33%
Toroidal Field
33%
Physics
Magnetic Field
100%
T Tauri Stars
100%
Circumstellar Disks
40%
Astronomical Unit
40%
Angular Momentum
20%
Field Strength
20%
Major Axis
20%
Star Formation
20%