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What is Turbulence in Galaxy Cluster Simulations about?

This study compares turbulence in simulated galaxy clusters (Coma, Virgo, and Perseus) using SLOW simulations with XRISM observations. The findings indicate that the simulations align well with observed turbulent velocities and pressure support, with Coma being the most active cluster and Virgo being very relaxed. The results highlight the importance of understanding selection effects in observational studies of the intracluster medium (ICM).

Author

kssaisrinivas4339

Language

EN