A novel procedure for the estimating the response sensitivity to input parameters of a complex FE model is presented. The method is specifically directed toward problems involving high-dimensional input parameter spaces, as they are encountered during uncertainty analysis with complex, refined FEmodels. In these cases one is commonly faced with thousands of uncertain parameters and traditional ...

Context. The distribution of member stars in the surroundings an open cluster (OC) can shed light on process its formation, evolution, and dissolution. analysis structural parameters OCs as a function their age position Galaxy constrains theoretical models evolution. Gaia catalog is very appropriate for finding members at large distance from centers. Aims. We revisit membership lists solar vici...