Effects of ultrafast outflows on X-ray time lags in active galactic nuclei

Context. The time lag between soft (e.g., 0.3–1 keV) and hard (e.g., 1–4 keV) X-ray photons has been observed in many active galactic nuclei (AGNs) and can reveal the accretion process and geometry around supermassive black holes. High-frequency Fe K and soft lags are considered to originate from th...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2024-12, Vol.692, p.A78
Hauptverfasser:	Xu, Yerong, Pinto, Ciro, Kara, Erin, Bianchi, Stefano, Alston, William, Tombesi, Francesco
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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