Magnetospheric accretion on the fully convective classical T Tauri star DN Tau (2013)
Attributed to:
Magnetic fields: the key to understanding the physics of stellar evolution and exoplanetary systems
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stt1622
Publication URI: http://dx.doi.org/10.1093/mnras/stt1622
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1