The impact of hot mode accretion and angular momentum conservation on metallicity gradients of galactic discs

arXiv:2608.31144 · astro-ph.GA · Submitted 2026-08-31 · Read on arXiv

astro-ph.GA

Submitted: 2026-08-31

Updated: 2026-08-31

Comments: 27 pages, 20 figures. Submitted to A&A

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Metallicity — 104× in this paper · explained in 3 episodes
Abundance — 29× in this paper · explained in 1 episode
Milky Way — 20× in this paper
Degeneracy — 5× in this paper · explained in 3 episodes
Trace — 4× in this paper · explained in 2 episodes
Age Gradients — 2× in this paper · explained in 1 episode
AGN — 1× in this paper · explained in 1 episode
Accretion Flows — 1× in this paper · explained in 1 episode
Bayesian Framework — 1× in this paper · explained in 3 episodes
Bayesian Inference — 1× in this paper · explained in 5 episodes
Core — 1× in this paper · explained in 2 episodes
Initial Mass Function (IMF) — 1× in this paper · explained in 2 episodes
Markov Chain Monte Carlo — 1× in this paper
Momentum transfer — 1× in this paper · explained in 2 episodes
Stellar Feedback — 1× in this paper · explained in 2 episodes

Sources

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