Modelling the magnetic activity & filtering radial velocity curves of young Suns: the weak-line T Tauri star LkCa 4 (2014)
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.1408.3273
Publication URI: https://arxiv.org/abs/1408.3273
Type: Other