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Wolf-Rayet (WR) stars, as they are advanced stages of the life of massivestars, provide a good test for various physical processes involved in themodelling of massive stars, such as rotation and mass loss. In this paper, weshow the outputs of the latest grids of single massive stars computed with theGeneva stellar evolution code, and compare them with some observations. Wepresent a short discussion on the shortcomings of single stars models and wealso briefly discuss the impact of binarity on the WR populations.

Wolf-Rayet stars as an evolved stage of stellar life