A systematic study of AGN feedback in a disk galaxy using MACER. III. High Gas Fractions in AGN Hosts

arXiv:2608.25341 · astro-ph.GA · Submitted 2026-08-26 · Read on arXiv

astro-ph.GA

Submitted: 2026-08-26

Updated: 2026-08-26

Comments: 14 pages, 9 figures. To be submitted to ApJ

Project page: https://macer-project.github.io

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

Terminology

• AGN — 132× in this paper · explained in 1 episode
• AGN Feedback — 30× in this paper · explained in 1 episode
• Aperture — 15× in this paper · explained in 1 episode
• Stellar Feedback — 3× in this paper · explained in 2 episodes
• Trace — 3× in this paper · explained in 2 episodes
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Core — 1× in this paper · explained in 2 episodes
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes

Sources

• Black Hole Binaries
• Quasars and Galaxy Formation
• PhotoIFU: NIRCam as a Photometric Integral Field Unit for Mapping Feedback in Galaxies

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