Speaker
Description
Laying at the top of structures of matter on the largest scales, galaxy clusters formation and evolution can be studied to characterize the fundamental properties of the Universe itself. Their dynamical state plays a key role in such studies but in general from observations is not trivial its determination. Since clusters morphology is strictly related to their dynamical state, one way to establish it is through morphological analysis on cluster maps from different observations. We study the connection between morphology and dynamical state of the simulated galaxy clusters from The Three Hundred Project. We quantify cluster dynamical state using a combination,