The multipolar magnetic fields of accreting pre-main-sequence stars: B at the inner disk, B along the accretion flow, and B at the accretion shock (2016)
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/10.48550/arxiv.1609.00273
Publication URI: http://dx.doi.org/10.48550/arxiv.1609.00273
Type: Journal Article/Review
Parent Publication: arXiv e-prints