The coronal evolution of pre-main-sequence stars (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.1608.05434
Publication URI: http://dx.doi.org/10.48550/arxiv.1608.05434
Type: Journal Article/Review
Parent Publication: arXiv e-prints