Stellar Surface Magneto-Convection as a Source of Astrophysical Noise II. Center-to-Limb Parameterisation of Absorption Line Profiles and Comparison to Observations (2018)
Attributed to:
Queen's University Belfast Astronomy Observation and Theory Consolidated Grant 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1807.11423
Publication URI: https://arxiv.org/abs/1807.11423
Type: Other