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Delving into the depths of NGC 3783 with XRISM

Using XRISM/Resolve 439 ks time-averaged spectra of the well-known Seyfert-1.5 active galactic nucleus (AGN) in NGC 3783, we investigated the nature of the Fe Kα emission line at 6.4 keV, the strongest and most common X-ray line observed in AGNs. Even the narrow component of the line is resolved wit...

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Principais autores: Li Chen, Kaastra Jelle S., Gu Liyi, Mehdipour Missagh, Eckart Megan E., Guainazzi Matteo, Kara Erin, Brenneman Laura W., Mizumoto Misaki, Miller Jon, Fukumura Keigo, Behar Ehud, Panagiotou Christos, Signorini Matilde, Zhao Keqin, Ballhausen Ralf, Diez Camille M., Kallman Timothy R., Ogawa Shoji, Tanimoto Atsushi, Ueda Yoshihiro
פורמט: Artigo
שפה:Inglês
יצא לאור: EDP Sciences 2026-02-01
סדרה:Astronomy & Astrophysics
נושאים:
techniques: spectroscopic
galaxies: active
galaxies: seyfert
x-rays: galaxies
x-rays: individuals: ngc 3783 fe k band
גישה מקוונת:https://www.aanda.org/articles/aa/full_html/2026/02/aa57710-25/aa57710-25.html
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