Energy deposited by black holes in the hot X-ray gas of elliptical galaxies, groups and clusters

arXiv:2609.01407 · astro-ph.CO, astro-ph.GA · Submitted 2026-09-01 · Read on arXiv

astro-ph.CO, astro-ph.GA

Submitted: 2026-09-01

Updated: 2026-09-04

Terminology

• AGN — 29× in this paper · explained in 1 episode
• Core — 10× in this paper · explained in 2 episodes
• AGN Feedback — 7× in this paper · explained in 1 episode
• Metallicity — 7× in this paper · explained in 3 episodes
• Calibration — 2× in this paper · explained in 7 episodes
• Accretion Efficiency — 1× in this paper · explained in 2 episodes
• Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• N-body simulations — 1× in this paper · explained in 2 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Beyond Self-Similarity: Reconciling X-Ray Scaling Relations in Galaxy Clusters and Groups

Related papers

• Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
• Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
• Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
• Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation