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X-ray cavities in TNG-Cluster: a direct comparison to observations

The TNG-Cluster magnetohydrodynamic cosmological simulations produce a diverse population of X-ray cavities in the intracluster medium (ICM) of simulated galaxy clusters. These arise from episodic, high velocity, kinetic energy injections from the central active supermassive black hole (AGN, SMBH)....

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Bibliographic Details
Main Authors: Prunier, Marine (Author) , Pillepich, Annalisa (Author) , Hlavacek-Larrondo, Julie (Author) , Nelson, Dylan (Author)
Format: Article (Journal)
Language:English
Published: May 2025
In: Monthly notices of the Royal Astronomical Society
Year: 2025, Volume: 539, Issue: 2, Pages: 1040-1064
ISSN:1365-2966
DOI:10.1093/mnras/staf525
Online Access:Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/staf525
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Author Notes:Marine Prunier, Annalisa Pillepich, Julie Hlavacek-Larrondo and Dylan Nelson
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Summary:The TNG-Cluster magnetohydrodynamic cosmological simulations produce a diverse population of X-ray cavities in the intracluster medium (ICM) of simulated galaxy clusters. These arise from episodic, high velocity, kinetic energy injections from the central active supermassive black hole (AGN, SMBH). Here, we present the first comprehensive comparative analysis of X-ray cavities in TNG-Cluster with observational data. First, we select a volume-limited sample of 35 real clusters
Item Description:Veröffentlicht: 01. April 2025
Gesehen am 30.09.2025
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/staf525

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