3D NLTE sodium abundance corrections relative to 1D LTE are typically negative and larger for saturated lines in giants, reaching -0.7 dex, with a public grid released for use.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
citation-role summary
background 1
method 1
citation-polarity summary
years
2026 4representative citing papers
A mechanical supernova feedback model conserves energy via rest-frame momentum injection and conditional thermal switching, yielding converged star formation histories in dwarf galaxy simulations at two resolutions.
Dust mass in early-type galaxies correlates with summed SiO and CO absorption equivalent widths, supporting internal production from evolved stars, while PAHs correlate with hot/warm dust but not with the absorption features.
A revised parallel chemical evolution model with pre-enriched delayed second infall explains the Milky Way's alpha-element abundance patterns, co-evolution phase, and old low-alpha stars from APOGEE data.
citing papers explorer
-
Co-evolution of the Milky Way high- and low-{\alpha} sequences with chemical evolution models
A revised parallel chemical evolution model with pre-enriched delayed second infall explains the Milky Way's alpha-element abundance patterns, co-evolution phase, and old low-alpha stars from APOGEE data.