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We use SEGUE and Hipparcos data to restrict the behaviour of the rotation curve of the Milky Way in the solar neighbourhood. Then we construct a density model of the Milky Way which best reproduces the available observations of the rotation curve and is consistent with the density constraints in the solar neighbourhood.doi:10.1051/epjconf/20121901006 fatcat:oeexejdgozbvtfkbadjcndhxxa