Local Heavily Obscured Active Galaxies Observed With Chandra (I): Spectral Properties of the Nuclear and Extended X-ray Emission

arXiv:2609.00182 · astro-ph.GA · Submitted 2026-08-31 · Read on arXiv

astro-ph.GA

Submitted: 2026-08-31

Updated: 2026-08-31

Terminology

• AGN — 78× in this paper · explained in 1 episode
• Core — 54× in this paper · explained in 2 episodes
• Trace — 6× in this paper · explained in 2 episodes
• Alignment — 4× in this paper · explained in 1 episode
• Aperture — 4× in this paper · explained in 1 episode
• AGN Feedback — 3× in this paper · explained in 1 episode
• Consistency — 3× in this paper · explained in 3 episodes
• Active Galactic Nuclei — 2× in this paper
• Active Galactic Nuclei (AGN) — 2× in this paper · explained in 1 episode
• Calibration — 2× in this paper · explained in 7 episodes
• Clustering — 2× in this paper · explained in 2 episodes
• Abundance — 1× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes

Sources

• High Resolution (<100pc) Ionization Structures in the ISM of AGN ESO~137-G34

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