Non-Thermal Pressure due to Gas Motions in the Intracluster Medium: Confronting XRISM/Resolve with TNG-Cluster Simulations

arXiv:2608.04757 · astro-ph.CO, astro-ph.GA, astro-ph.HE · Submitted 2026-08-05 · Read on arXiv

astro-ph.CO, astro-ph.GA, astro-ph.HE

Submitted: 2026-08-05

Updated: 2026-09-08

Comments: 16 pages, 12 Figures. Submitted to PASJ. Revised after referee's report. Comments are welcome

Code: https://github.com/AtomDB/pyatomdb

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

Terminology

Core — 94× in this paper · explained in 2 episodes
Velocity Dispersion — 39× in this paper · explained in 2 episodes
AGN — 12× in this paper · explained in 1 episode
AGN Feedback — 9× in this paper · explained in 1 episode
Anisotropy — 9× in this paper · explained in 3 episodes
Accretion Shock — 3× in this paper · explained in 1 episode
Anti-correlation — 3× in this paper · explained in 3 episodes
Metallicity — 3× in this paper · explained in 3 episodes
Aperture — 2× in this paper · explained in 1 episode
Robustness — 2× in this paper · explained in 5 episodes
Trace — 2× in this paper · explained in 2 episodes
Abundance — 1× in this paper · explained in 1 episode
Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
Dynamical regimes — 1× in this paper · explained in 2 episodes
Forward modeling — 1× in this paper · explained in 2 episodes

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