The metal-poor edge of the Milky Way's "thin disc"
Context. The emergence of the disc in our Galaxy and the relation between thick and thin disc formation and evolution is still a matter of debate. The chemo-dynamical characterization of disc stars is key to resolving this question, particularly at parameter regimes, where both disc components overlap, such as the region around [Fe/H] ∼ −0.7
Fernández-Alvar, Emma et al.
Fecha de publicación:
5
2024