XRISM Spectroscopy of Accretion-driven Wind Feedback in NGC 4151

XRISM Spectroscopy of Accretion-driven Wind Feedback in NGC 4151

The hottest, most ionized, and fastest winds driven by accretion onto massive black holes have the potential to reshape their host galaxies. Calorimeter-resolution X-ray spectroscopy is the ideal tool to understand this feedback mode, as it enables accurate estimates of the physical characteristics...

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Bibliographic Details
Main Authors: Xin Xiang, Jon M. Miller, Ehud Behar, Rozenn Boissay-Malaquin, Laura Brenneman, Margaret Buhariwalla, Doyee Byun, Chris Done, Luigi Gallo, Dimitra Gerolymatou, Scott Hagen, Jelle Kaastra, Stephane Paltani, Frederick S. Porter, Richard Mushotzky, Hirofumi Noda, Missagh Mehdipour, Takeo Minezaki, Makoto Tashiro, Abderahmen Zoghbi
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
X-ray active galactic nuclei
Active galactic nuclei
Supermassive black holes
Online Access:https://doi.org/10.3847/2041-8213/adee9b
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https://doi.org/10.3847/2041-8213/adee9b

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