SQuIGG E: Ubiquitous Cool Gas Outflows with Large Mass-Loading Factors in z about0.7 Post-starburst Galaxies

arXiv:2609.31308 · astro-ph.GA · Submitted 2026-09-25 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-25

Updated: 2026-09-25

Terminology

• AGN — 58× in this paper · explained in 1 episode
• Metallicity — 4× in this paper · explained in 3 episodes
• Trace — 4× in this paper · explained in 2 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Degeneracy — 2× in this paper · explained in 3 episodes
• Sloan Digital Sky Survey — 2× in this paper
• AGN Feedback — 1× in this paper · explained in 1 episode
• Abundance — 1× in this paper · explained in 1 episode
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Bayesian Inference — 1× in this paper · explained in 5 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Entrainment — 1× in this paper · explained in 2 episodes
• Galaxy Quenching — 1× in this paper · explained in 3 episodes

Sources

• Quasars and Galaxy Formation
• A Census of Na D-traced neutral ISM and outflows at 0.6<z<4
• The JWST EXCELS survey: Outflows in 1.5 < z < 5 quiescent and recently quenched galaxies are likely relics from episodic AGN activity
• Quenching of Star Formation in Massive Galaxies
• There and back again? Neutral outflows in z~3.5 quiescent galaxies

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