Stellar Surface Magneto-convection as a Source of Astrophysical Noise. II. Center-to-limb Parameterization of Absorption Line Profiles and Comparison to Observations (2018)
Attributed to:
Queen's University Belfast Consolidated Grant in Solar Physics and Solar System Studies 2017 - 2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aaddfc
Publication URI: http://dx.doi.org/10.3847/1538-4357/aaddfc
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1