Dissecting the Nuclear Structure of NGC 5548 with XRISM. I. Physical Properties of the Highly Ionized Outflows
Missagh Mehdipour, Jon M. Miller, Jelle S. Kaastra, Gerard A. Kriss, Keigo Fukumura, Liyi Gu, Doyee Byun, Xin Xiang, Ehud Behar, Laura W. Brenneman, Elisa Costantini, Maryam Dehghanian, Jacobo Ebrero, Massimo Gaspari, Anna Juráňová, Erin Kara, Chen Li, Junjie Mao, Hirofumi Noda, Anna Ogorzalek, Ioanna Psaradaki, Daniele Rogantini, Sascha T. Zeegers, Keqin Zhao
astro-ph.HE, astro-ph.GA
Submitted: 2026-08-05
Comments: Accepted for publication in ApJ, 14 pages
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Anatomy of the AGN in NGC 5548: II. The Spatial, Temporal and Physical Nature of the Outflow from HST/COS Observations
- Active galactic nuclei with high-resolution X-ray spectroscopy
- The dynamic central environment of NGC 3516 revealed by XRISM
- XRISM Discovery of Multiple Ionized Fe-K Emission and Absorption Components in Centaurus A
- Winds of Change: XRISM Resolve X-ray spectroscopy of NGC 4051
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