Origin of the Sloshing Spiral in the Abell 2107 Galaxy Cluster

arXiv:2607.16496 · astro-ph.CO, astro-ph.GA · Submitted 2026-07-17 · Read on arXiv

Muhammed Kıyami Erdim

astro-ph.CO, astro-ph.GA

Submitted: 2026-07-17

Comments: 11 pages, 9 figures. Accepted for publication in MNRAS

DOI: 10.1093/mnras/stag1268

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

Terminology

• Cold front — 29× in this paper · explained in 2 episodes
• Core — 25× in this paper · explained in 2 episodes
• Metallicity — 10× in this paper · explained in 3 episodes
• Abundance — 8× in this paper · explained in 1 episode
• Trace — 4× in this paper · explained in 2 episodes
• AGN — 3× in this paper · explained in 1 episode
• AGN Feedback — 3× in this paper · explained in 1 episode
• Alignment — 2× in this paper · explained in 1 episode
• Calibration — 2× in this paper · explained in 7 episodes
• Robustness — 2× in this paper · explained in 5 episodes

Sources

• Sherpa: a Mission-Independent Data Analysis Application

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