Forming intracluster gas in a galaxy protocluster at a redshift of 2.16

Galaxy clusters are the most massive gravitationally bound structures in the Universe, comprising thousands of galaxies and pervaded by a diffuse, hot intracluster medium (ICM) that dominates the baryonic content of these systems. The formation and evolution of the ICM across cosmic time(1) is thoug...

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Detalles Bibliográficos
Autores principales: Di Mascolo, Luca, Saro, Alexandro, Mroczkowski, Tony, Borgani, Stefano, Churazov, Eugene, Rasia, Elena, Tozzi, Paolo, Dannerbauer, Helmut, Basu, Kaustuv, Carilli, Christopher L., Ginolfi, Michele, Miley, George, Nonino, Mario, Pannella, Maurilio, Pentericci, Laura, Rizzo, Francesca
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10060161/
https://www.ncbi.nlm.nih.gov/pubmed/36991192
http://dx.doi.org/10.1038/s41586-023-05761-x

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10060161/
https://www.ncbi.nlm.nih.gov/pubmed/36991192
http://dx.doi.org/10.1038/s41586-023-05761-x

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