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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 C1.

Comparison between synthetic hot wind spectral models from numerical simulations in S21 and S22 and observed spectra in the 0.5–2 keV band. The normalization of the models has been accordingly adjusted. The legends are the same as in Figures 1(b) and (d).

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