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The vast majority of stars are born in associations or clusters rather than in isolation. To understand the general rules that govern how stars form, it is therefore crucial to decode fully the formation and evolution of young stellar clusters. This is the main goal of this project, which will focus more specifically on the early dynamical evolution of stellar systems. To pursue these objectives, we propose to bring together theoretical and observational expertise drawn from two research groups well established in their respective field: the Stellar Formation group in Grenoble, which has a vast experience in young cluster observations; and the Galaxy team in Strasbourg, which has strong expertise in N-body numerical simulations. Thanks to the recruitment of an ANR postdoc, this project will allow to develop a new expertise on numerical simulation at LAOG that is essential to interpret the observations of young stellar clusters.
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