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SZ–X-Ray Surface Brightness Fluctuations in the SPT-XMM Clusters

The hot plasma in galaxy clusters, the intracluster medium, is expected to be shaped by subsonic turbulent motions, which are key for heating, cooling, and transport mechanisms. The turbulent motions contribute to the nonthermal pressure, which, if not accounted for, consequently imparts a hydrostat...

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Principais autores: Charles E. Romero, Massimo Gaspari, Gerrit Schellenberger, Bradford A. Benson, Lindsey E. Bleem, Esra Bulbul, William Forman, Ralph Kraft, Paul Nulsen, Christian L. Reichardt, Arnab Sarkar, Taweewat Somboonpanyakul, Yuanyuan Su
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Assuntos:
Intracluster medium
Galaxy clusters
Acceso en liña:https://doi.org/10.3847/1538-4357/adcd74
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