Source Themes

Gas motion in the ICM of the Virgo cluster replica
Within the deep gravitational potential of galaxy clusters lies the intracluster medium (ICM). At the first order, it is considered to …
Théo Lebeau, Stefano Ettori, Jenny G. Sorce, Nabila Aghanim, Jade Paste
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Gas motion in the ICM of the Virgo cluster replica
Velocity fields and turbulence from cosmic filaments to galaxy clusters
Galaxy clusters are currently the endpoint of the hierarchical structure formation; they form via the accretion of dark matter and …
Théo Lebeau, Saleem Zaroubi, Nabila Aghanim, Jenny G. Sorce, Mathieu Langer
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Velocity fields and turbulence from cosmic filaments to galaxy clusters
Can the splashback radius be an observable boundary of galaxy clusters?
The splashback radius was proposed as a physically motivated boundary of clusters as it sets the limit between the infalling and the …
Théo Lebeau, Stefano Ettori, Nabila Aghanim, Jenny G. Sorce
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Can the splashback radius be an observable boundary of galaxy clusters?
Mass bias in clusters of galaxies: Projection effects on the case study of Virgo replica
When measuring the observed pressure, density, or temperature profiles of the intracluster gas, and hence the mass of clusters of …
Théo Lebeau, Jenny G. Sorce, Nabila Aghanim, Elena Hernández-Martínez, Klaus Dolag
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Mass bias in clusters of galaxies: Projection effects on the case study of Virgo replica