In FOGGIE simulations, Mg II is concentrated near the galaxy while O VI forms a diffuse halo; Mg II-O VI absorber pairs with similar velocities are usually not spatially close.
Title resolution pending
1 Pith paper cite this work, alongside 3 external citations. Polarity classification is still indexing.
1
Pith paper citing it
3
external citations · OpenAlex
fields
astro-ph.GA 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Figuring Out Gas & Galaxies in Enzo (FOGGIE). XV. Examining the Spatial and Kinematic Relationship between Circumgalactic Mg II and O VI
In FOGGIE simulations, Mg II is concentrated near the galaxy while O VI forms a diffuse halo; Mg II-O VI absorber pairs with similar velocities are usually not spatially close.