Despite multiple cold fronts and a history of dynamical disturbance, the Ophiuchus cluster core has remarkably low gas velocity dispersions (115 to 186 km/s) and a nearly stationary inner core.
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XRISM Observation of the Ophiuchus Galaxy Cluster: Quiescent Velocity Structure in the Dynamically Disturbed Core
Despite multiple cold fronts and a history of dynamical disturbance, the Ophiuchus cluster core has remarkably low gas velocity dispersions (115 to 186 km/s) and a nearly stationary inner core.