XRISM Data Reveals Gas Dynamics in Hydra-A Galaxy Cluster

New observations from the XRISM telescope, detailed in a preprint, offer insights into the gas motions within the X-ray atmosphere of the Hydra-A galaxy cluster. By integrating data from both XRISM and Chandra, scientists are analyzing atmospheric kinematics, noting similar velocity dispersion in different regions. These findings are preliminary and await peer review.