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Observational Evidence for Hot Wind Impact on Parsec Scales in Low-luminosity Active Galactic Nuclei

  • Authors: Fangzheng Shi, Feng Yuan, Zhiyuan Li, Zhao Su, Suoqing Ji

Fangzheng Shi et al 2024 The Astrophysical Journal 970 .

  • Provider: AAS Journals

Caption: Figure 4.

Predicted 0.5–8 keV X-ray surface brightness (left columns) and temperature distribution (right columns) of circumnuclear medium shocked by the expanding hot winds within central 10 pc for M81* at t = 4000 yr (upper panels) and t = 10,000 yr (lower panels). Strong X-ray emitting regions coincide with ∼107 K gas. Hot winds continuously push the circumnuclear medium outward.

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