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The aim of this thesis is to find where Hyper Velocity Stars (HVS) originate from. This is done by first finding the HVS, a phenomenon observed in space in which the star has a terminal velocity of more than 1000 km/s. A cross-match of stars will provide the data from two catalogues Gaia and RAVE. Then this data is used to simulate the past trajectory of the HVS and evaluate its origins. One prob
