CORDIS Project
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This project aims to analyze the structure and dynamics of the Milky Way galaxy using extensive stellar data. By developing techniques to create mass density and kinematic maps, the research seeks to enhance our understanding of galaxy formation and the influence of dark matter.
Our Milky Way is a very typical galaxy, yet our position within it makes it a unique object of study: star-by-star we can obtain 3D positions, 3D velocities and chemical abundances.
This wealth of information about our Galaxy’s stellar body holds the key to understanding how disk galaxies form and how dark matter acts on the scales of galaxies.
Ongoing surveys have recently hundred-folded the number of stars with good distance estimates, radial and transverse velocities and abundance estimates;…
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
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