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Magnetospheric accretion on the fully convective classical T Tauri star DN Tau (2013)

First Author: Donati J

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