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Stellar Surface Magneto-convection as a Source of Astrophysical Noise. II. Center-to-limb Parameterization of Absorption Line Profiles and Comparison to Observations (2018)

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