XRISM Constrains Atmospheric Motion and Turbulent Dissipation in the Archetypal Radio-mode Feedback System Hydra-A

XRISM Constrains Atmospheric Motion and Turbulent Dissipation in the Archetypal Radio-mode Feedback System Hydra-A

We present XRISM Resolve observations centered on Hydra-A, a redshift z = 0.054 brightest cluster galaxy, which hosts one of the largest and most powerful FR-I radio sources in the nearby Universe. We examine the effects of its high jet power on the velocity structure of the cluster’s hot atmosphere...

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Bibliographic Details
Main Authors: Tom Rose, B. R. McNamara, Julian Meunier, A. C. Fabian, Helen Russell, Paul Nulsen, Neo Dizdar, Timothy M. Heckman, Michael McDonald, Maxim Markevitch, Frits Paerels, Aurora Simionescu, Norbert Werner, Alison L. Coil, Edmund Hodges-Kluck, Eric D. Miller, Michael Wise
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy clusters
Intracluster medium
X-ray astronomy
Online Access:https://doi.org/10.3847/1538-4357/adf32d
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https://doi.org/10.3847/1538-4357/adf32d

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