Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31

arXiv:2605.16501 · astro-ph.GA · Submitted 2026-05-15 · Read on arXiv

astro-ph.GA

Submitted: 2026-05-15

Updated: 2026-08-27

Code: https://github.com/jchelly/read_eagle

Terminology

• AGN — 53× in this paper · explained in 1 episode
• AGN Feedback — 32× in this paper · explained in 1 episode
• Abundance — 7× in this paper · explained in 1 episode
• Metallicity — 5× in this paper · explained in 3 episodes
• Milky Way — 3× in this paper
• Trace — 3× in this paper · explained in 2 episodes
• Calibration — 2× in this paper · explained in 7 episodes
• Core — 2× in this paper · explained in 2 episodes
• Stellar Feedback — 1× in this paper · explained in 2 episodes
• Velocity Dispersion — 1× in this paper · explained in 2 episodes

Sources

• The COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution
• The EAGLE simulations of galaxy formation: Public release of particle data
• The Merging History of the Milky Way Disk

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