@article{4ce8254760d64dceaecf4d5f629634cf,
title = "The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy",
abstract = "Context. The solar vicinity is currently populated by a mix of stars with various chemo-dynamic properties, including stars with a high metallicity compared to the Sun. Dynamical processes such as churning and blurring are expected to relocate such metal-rich stars from the inner Galaxy to the solar region.Aims. We report the identification of a set of old super-metal-rich (+0.15",
keywords = "Galaxy: abundances, Galaxy: evolution, Galaxy: kinematics and dynamics, Galaxy: stellar content, stars: abundances, CHEMICAL EVOLUTION, MILKY-WAY, STELLAR ABUNDANCE, RADIAL MIGRATION, GALACTIC DISK, SOLAR NEIGHBORHOOD, F-DWARF, STARS, THICK, KINEMATICS",
author = "Dantas, {M. L. L.} and R. Smiljanic and R. Boesso and Rocha-Pinto, {H. J.} and L. Magrini and G. Guiglion and G. Tautvaisiene and G. Gilmore and S. Randich and T. Bensby and A. Bragaglia and M. Bergemann and G. Carraro and P. Jofre and S. Zaggia",
year = "2023",
month = jan,
day = "17",
doi = "10.1051/0004-6361/202243667",
language = "English",
volume = "669",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",
}