Thermal and non-thermal emission from supermassive black hole circumbinary disks: Disks, Coronae, Streams, and Cavities

arXiv:2609.03140 · astro-ph.HE · Submitted 2026-09-02 · Read on arXiv

astro-ph.HE

Submitted: 2026-09-02

Updated: 2026-09-21

Terminology

• Core — 16× in this paper · explained in 2 episodes
• AGN — 6× in this paper · explained in 1 episode
• Trace — 2× in this paper · explained in 2 episodes
• pulsar timing arrays — 2× in this paper · explained in 2 episodes
• Angular Error — 1× in this paper · explained in 1 episode
• Laser Interferometer Space Antenna — 1× in this paper
• Provenance — 1× in this paper · explained in 4 episodes

Sources

• High-energy Emission from Turbulent Electron-ion Coronae of Accreting Black Holes
• X-ray Reflection as Diagnostic of Supermassive Black Hole Binary Properties
• Prospects of resolving and localising individual supermassive black hole binaries with pulsar timing arrays: the host ranking challenge

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