Context. The [Mg/Fe] abundance ratios are a fundamental fossil signature used to trace the chemical evolution of the disc and to divide it into low-α and high-α populations. Despite the huge observational and theoretical efforts, discrepancies between models and data are still present and several explanations have been put forward to explain the [α/Fe] bimodality. Aims. In this work we take advantage of a new AMBRE:HARPS dataset, which provides new more precise [Mg/Fe] estimations and reliable stellar ages for a subsample of stars, to study the [α/Fe] bimodality and the evolution of the solar neighbourhood. Methods. The data are compared with detailed chemical evolution models for the Milky Way, exploring the most used prescriptions for ste...
Uncertainties in stellar nucleosynthesis and their impact on models of chemical evolution are discus...
8We study the chemical evolution of the thick and thin discs of the Galaxy by comparing detailed che...
We present Mg abundances derived from high-resolution spectra using several MgI and two high-excitat...
Context. The [Mg/Fe] abundance ratios are a fundamental fossil signature used to trace the chemical ...
Context. The [Mg/Fe] abundance ratios are a fundamental fossil signature to trace the chemical evolu...
International audienceContext. The abundance of α-elements relative to iron ([α/Fe]) is an important...
Context. The pattern of chemical abundance ratios in stellar populations of the Milky Way is a finge...
It is well established that the chemical structure of the Milky Way exhibits a bimodality with respe...
Models of the chemical evolution of our Galaxy are extended to include radial migration of stars and...
Aims. Previous high-precision studies of abundances of elements in solar twin stars are extended to ...
The accurate O, Mg and Fe abundances derived in previous papers of this series from a homogeneous re...
International audienceWe present new maps of the Milky Way disk showing the distribution of metallic...
Context. The spatial distribution of elemental abundances in the disc of our Galaxy gives insights b...
Context. The Galactic bulge has a bimodal metallicity distribution function: different kinematic, sp...
Aims. The main goal of this work is to study element ratios that are important for the formation of ...
Uncertainties in stellar nucleosynthesis and their impact on models of chemical evolution are discus...
8We study the chemical evolution of the thick and thin discs of the Galaxy by comparing detailed che...
We present Mg abundances derived from high-resolution spectra using several MgI and two high-excitat...
Context. The [Mg/Fe] abundance ratios are a fundamental fossil signature used to trace the chemical ...
Context. The [Mg/Fe] abundance ratios are a fundamental fossil signature to trace the chemical evolu...
International audienceContext. The abundance of α-elements relative to iron ([α/Fe]) is an important...
Context. The pattern of chemical abundance ratios in stellar populations of the Milky Way is a finge...
It is well established that the chemical structure of the Milky Way exhibits a bimodality with respe...
Models of the chemical evolution of our Galaxy are extended to include radial migration of stars and...
Aims. Previous high-precision studies of abundances of elements in solar twin stars are extended to ...
The accurate O, Mg and Fe abundances derived in previous papers of this series from a homogeneous re...
International audienceWe present new maps of the Milky Way disk showing the distribution of metallic...
Context. The spatial distribution of elemental abundances in the disc of our Galaxy gives insights b...
Context. The Galactic bulge has a bimodal metallicity distribution function: different kinematic, sp...
Aims. The main goal of this work is to study element ratios that are important for the formation of ...
Uncertainties in stellar nucleosynthesis and their impact on models of chemical evolution are discus...
8We study the chemical evolution of the thick and thin discs of the Galaxy by comparing detailed che...
We present Mg abundances derived from high-resolution spectra using several MgI and two high-excitat...