Observatoire de la C˘te d'Azur
The Galactic thin and thick discs can be chemically and kinetically described owing to the thousands of stellar spectra collected by the Gaia-ESO Survey (GES). I will present the first characterization of these Galactic structures based on the first data release of GES and discuss the new constraints provided to their formation scenarios.
2014 February 26, 13:30
Centro de AstrofÝsica da Universidade do Porto (Auditorium)
Rua das Estrelas, 4150-762 Porto