An Investigation of the Formation and Line Properties of MgH in 3D Hydrodynamical Model Stellar Atmospheres (2017)

First Author: Thygesen A

Attributed to: WEAVE Detectors Completion funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aa79a0

Publication URI: http://dx.doi.org/10.3847/1538-4357/aa79a0

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2