Non-LTE abundance corrections for late-type stars from 2000 Å to 3 µm I. Na, Mg, and Al (2022)
Attributed to:
Support for an observing programme at the University of Hertfordshire
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202142195
Publication URI: http://dx.doi.org/10.1051/0004-6361/202142195
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics