Disentangling multiple gas kinematic drivers in the Perseus galaxy cluster

Puntos clave

• Gas kinematics reveals intricacies of gravitational interactions within the Perseus galaxy cluster, enhancing our comprehension of cosmic structures.
• Key findings show multiple gas kinematic drivers, demonstrating variability and complexity in motion throughout the cluster.
• Observational analysis distinguishes these drivers across different scales, emphasizing the role of both internal and external forces shaping gas dynamics.
• Understanding these kinematic drivers highlights the need for further studies to explore their implications on galaxy formation and evolution.