Chemodynamical evolution of the Milky Way disk I: The solar vicinity

Abstract

[Abridged] In this first paper of this series, we present a new approach for studying the chemo-dynamical evolution in disk galaxies, which consists of fusing disk chemical evolution models with compatible numerical simulations of galactic disks. This method avoids known star formation and chemical enrichment problems encountered in simulations. Here we focus on the Milky Way, by using a detailed thin-disk chemical evolution model and a simulation in the cosmological context, with dynamical properties close to those of our Galaxy. We show that, due to radial migration from mergers at high redshift and the central bar at later times, a sizable fraction of old metal-poor high-[alpha/Fe] stars reaches the solar vicinity. This naturally accounts for a number of recent observations related to both the thin and thick disks, despite the fact that we use thin-disk chemistry only. Although significant radial mixing is present, the slope in the age-metallicity relation is only weakly affected, with a scatter compatible with recent observational work. While we find a smooth density distribution in the [O/Fe]-[Fe/H] plane, we can recover the observed discontinuity by selecting particles according to kinematic criteria used in high-resolution samples to define the thin and thick disks. We outline a new method for estimating the birth place of the Sun and predict that the most likely radius lies in the range 4.4 < r < 7.7 kpc (for a location at r = 8 kpc). A new, unifying model for the Milky Way thick disk is offered, where both mergers and radial migration play a role at different stages of the disk evolution. We show that in the absence of early-on massive mergers the vertical velocity dispersion of the oldest stars is underestimated by a factor of ~2 compared with observations. We can, therefore, argue that the Milky Way thick disk is unlikely to have been formed through a quiescent disk evolution.

27 pages, 18 figures, exact match to published version

References in corpus (29)

• The Radial Velocity Experiment (RAVE): first data release
• New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program.Galactic stellar populations and planets
• The age structure of stellar populations in the solar vicinity. Clues of a two-phase formation history of the Milky Way disk
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks
• On the mass-to-light ratio of the local Galactic disc and the optical luminosity of the Galaxy
• Inside Out and Upside Down: Tracing the Assembly of a Simulated Disk Galaxy Using Mono-Age Stellar Populations
• Oxygen Abundances in Nearby FGK Stars and the Galactic Chemical Evolution of the Local Disk and Halo
• The Milky Way's Stellar Disk
• Radial mixing and the transition between the thick and thin Galactic discs
• Vertical density waves in the Milky Way disc induced by the Sagittarius Dwarf Galaxy
• The Galaxy and its stellar halo: insights on their formation from a hybrid cosmological approach
• Thin disc, Thick Disc and Halo in a Simulated Galaxy
• Simulations of Cosmic Chemical Enrichment
• Radial Migration Does Little for Galactic Disc Thickening
• APOGEE: The Apache Point Observatory Galactic Evolution Experiment
• Is the Milky Way ringing? The hunt for high velocity streams
• Abundance gradients in the Milky Way for alpha elements, Iron peak elements, Barium, Lanthanum and Europium
• The properties of the local spiral arms from RAVE data: two-dimensional density wave approach
• New Constraints on the Galactic Bar
• Chemical evolution of galaxies. I. A composition-dependent SPH model for chemical evolution and cooling
• The Destruction of Thin Stellar Disks Via Cosmologically Common Satellite Accretion Events
• The relation between chemical abundances and kinematics of the Galactic disc with RAVE
• A Schmidt-Kennicutt law for star formation in the Milky Way disk
• Circular velocity profiles of dark matter haloes
• Abundances in the Galactic bulge: results from planetary nebulae and giant stars
• The Galactic thin and thick disk

Cited by in corpus (331)

• The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
• The GALAH Survey: Scientific Motivation
• Chemical Cartography with APOGEE: Metallicity Distribution Functions and the Chemical Structure of the Milky Way Disk
• The age structure of stellar populations in the solar vicinity. Clues of a two-phase formation history of the Milky Way disk
• The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies
• Chemodynamical evolution of the Milky Way disk II: Variations with Galactic radius and height above the disk plane
• The stellar population structure of the Galactic disk
• On the metallicity of open clusters. III. Homogenised sample
• Chemodynamics of the Milky Way. I. The first year of APOGEE data
• Chemodynamical history of the Galactic Bulge
• Tracing chemical evolution over the extent of the Milky Way's Disk with APOGEE Red Clump Stars
• Characterizing the FRB host galaxy population and its connection to transients in the local and extragalactic Universe
• The Gaia-ESO Survey: radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk
• On the fine structure of the Cepheid metallicity gradient in the Galactic thin disk
• Estimating stellar birth radii and the time evolution of the Milky Way's ISM metallicity gradient
• Young [$\alpha$/Fe]-enhanced stars discovered by CoRoT and APOGEE: What is their origin?
• On the Formation of Galactic Thick Disks
• The age-metallicity structure of the Milky Way disk
• Age dissection of the Milky Way discs: red giants in the Kepler field
• Evolution of the Milky Way with radial motions of stars and gas I. The solar neighborhood and the thin and thick disk
• Chemical Cartography with APOGEE: Large-scale Mean Metallicity Maps of the Milky Way
• On the origin of the chemical bimodality of disk stars: A tale of merger and migration
• Vertical disc heating in Milky Way-sized galaxies in a cosmological context
• From the bulge to the outer disc: StarHorse stellar parameters, distances, and extinctions for stars in APOGEE DR16 and other spectroscopic surveys
• Inflow, Outflow, Yields, and Stellar Population Mixing in Chemical Evolution Models
• VINTERGATAN I: The origins of chemically, kinematically and structurally distinct discs in a simulated Milky Way-mass galaxy
• r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos
• The Open Cluster Chemical Abundances and Mapping Survey: IV. Abundances for 128 Open Clusters using SDSS/APOGEE DR16
• The Structure and Dynamical Evolution of the Stellar Disk of a Simulated Milky Way-Mass Galaxy
• The History of R-Process Enrichment in the Milky Way
• Measuring Radial Orbit Migration in the Milky Way Disk
• Red giants observed by CoRoT and APOGEE: The evolution of the Milky Way's radial metallicity gradient
• Chemical Cartography with APOGEE: Multi-element abundance ratios
• Abundance to age ratios in the HARPS-GTO sample with Gaia DR2: Chemical clocks for a range of [Fe/H]
• Origin of chemically distinct discs in the Auriga cosmological simulations
• Bending and Breathing Modes of the Galactic Disk
• Kinematic modelling of the Milky Way using the RAVE and GCS stellar surveys
• The Gaia-ESO Survey: the chemical structure of the Galactic discs from the first internal data release
• High-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations
• The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS
• Stroemgren survey for Asteroseismology and Galactic Archaeology: let the SAGA begin
• The Milky Way bar and bulge revealed by APOGEE DR16 and Gaia EDR3
• $Gaia$ white dwarfs within 40 pc II: the volume-limited northern hemisphere sample
• The GALAH survey: tracing the Galactic disk with Open Clusters
• Carbon and oxygen abundances from recombination lines in low-metallicity star-forming galaxies. Implications for chemical evolution
• Chemical Enrichment and Radial Migration in the Galactic Disk -- the origin of the [$\alpha /\mathrm{Fe}]$ Double Sequence
• Spiral-induced velocity and metallicity patterns in a cosmological zoom simulation of a Milky Way-sized galaxy
• The imprint of clump formation at high redshift. I. A disc alpha-abundance dichotomy
• Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution
• StarHorse results for spectroscopic surveys + Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young-alpha rich stars
• Galactic Archaeology with asteroseismology and spectroscopy: Red giants observed by CoRoT and APOGEE
• Dissecting simulated disc galaxies II: the age-velocity relation
• Spectro-photometric distances to stars: a general-purpose Bayesian approach
• PLATO as it is: a legacy mission for Galactic archaeology
• The effects of bar-spiral coupling on stellar kinematics in the Galaxy
• The origin of diverse $\alpha$-element abundances in galaxy discs
• Keeping it Cool: Much Orbit Migration, yet Little Heating, in the Galactic Disk
• Correcting the spectroscopic surface gravity using transits and asteroseismology. No significant effect on temperatures or metallicities with ARES+MOOG in LTE
• Oxygen abundances in G- and F-type stars from HARPS
• Fluctuations in galactic bar parameters due to bar-spiral interaction
• On the origin of stars with and without planets. Tc trends and clues to Galactic evolution
• Cannibals in the thick disk: the young $\alpha -$rich stars as evolved blue stragglers
• Extended distribution functions for our Galaxy
• Advanced LIGO Constraints on Neutron Star Mergers and R-Process Sites
• A new stellar chemo-kinematic relation reveals the merger history of the Milky Way disc
• The Pristine survey X: a large population of low-metallicity stars permeates the Galactic disk
• The Rich Are Different: Evidence from the RAVE Survey for Stellar Radial Migration
• Dissecting stellar chemical abundance space with t-SNE
• Galactic abundance gradients from Cepheids: alpha and heavy elements in the outer disk
• Heavy metal rules. I. Exoplanet incidence and metallicity
• Age-resolved chemistry of red giants in the solar neighbourhood
• Spatial variations in the Milky Way disc metallicity-age relation
• Metallicity Fluctuation Statistics in the Interstellar Medium and Young Stars. I. Variance and Correlation
• The formation of the solar system
• Chemical gradients in the Milky Way from the RAVE data. I. Dwarf stars
• ExoMol molecular line lists - XXIII: spectra of PO and PS
• Impact of radial migration on stellar and gas radial metallicity distribution
• The Gaia-ESO survey: mapping the shape and evolution of the radial abundance gradients with open clusters
• The Gaia-ESO Survey: Sodium and aluminium abundances in giants and dwarfs - Implications for stellar and Galactic chemical evolution
• The physics of gas phase metallicity gradients in galaxies
• High-precision abundances of elements in Kepler LEGACY stars. Verification of trends with stellar age
• VINTERGATAN II: the history of the Milky Way told by its mergers
• The Gaia-ESO Survey: Probes of the inner disk abundance gradient
• The Gaia-ESO Survey: Characterisation of the [alpha/Fe] sequences in the Milky Way discs
• Inside Out and Upside-Down: The Roles of Gas Cooling and Dynamical Heating in Shaping the Stellar Age-Velocity Relation
• On the alpha-element gradients of the Galactic thin disk using Cepheids
• APOGEE DR14/DR15 Abundances in the Inner Milky Way
• A Tale of Two Disks: Mapping the Milky Way with the Final Data Release of APOGEE
• The Gaia-ESO Survey: a new approach to chemically characterising young open clusters
• The Open Cluster Chemical Abundances and Mapping Survey: VI. Galactic Chemical Gradient Analysis from APOGEE DR17
• Phylogeny of the Milky Way's inner disk and bulge populations: Implications for gas accretion, (the lack of) inside-out thick disk formation, and quenching
• Evolution of the Milky Way with radial motions of stars and gas II. The evolution of abundance profiles from H to Ni
• Dissecting simulated disc galaxies I: the structure of mono-age populations
• Metallicity Structure in the Milky Way Disk Revealed by Galactic HII Regions
• The relationship between mono-abundance and mono-age stellar populations in the Milky Way disk
• The evolution of the Milky Way: New insights from open clusters
• The AMBRE Project: Constraining the lithium evolution in the Milky Way
• Chemical gradients in the Milky Way from the RAVE data. II. Giant stars
• Bimodality of [α/Fe]-[Fe/H] distributions is a natural outcome of dissipative collapse and disc growth in Milky Way-type galaxies
• The GALAH Survey: Chemodynamics of the Solar Neighbourhood
• Revisiting long-standing puzzles of the Milky Way: the Sun and its vicinity as typical outer disk chemical evolution
• How magnetic activity alters what we learn from stellar spectra
• Spectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc
• Prospects for chemically tagging stars in the Galaxy
• Mapping the Galactic Metallicity Gradient with Open Clusters: The State-of-the-Art and Future Challenges
• Determining Ages of APOGEE Giants with Known Distances
• Unveiling the Distinct Formation Pathways of the Inner and Outer Discs of the Milky Way with Bayesian Machine Learning
• The chemical evolution of local star forming galaxies: Radial profiles of ISM metallicity, gas mass, and stellar mass and constraints on galactic accretion and winds
• Direct evidence of multiple reservoirs of volatile nitrogen in a protosolar nebula analogue
• The Galactic metallicity gradient shown by open clusters in the light of radial migration
• The age-chemical abundance structure of the Galactic disc II: $\alpha$-dichotomy and thick disc formation
• The effect of stellar migration on Galactic chemical evolution: a heuristic approach
• 2D chemical evolution model: the impact of galactic disc asymmetries on azimuthal chemical abundance variations
• Exploring open cluster properties with Gaia and LAMOST
• Stellar ages, masses, extinctions and orbital parameters based on spectroscopic parameters of Gaia DR3
• Uncertainties in Galactic Chemical Evolution Models
• Mixing and transport of metals by gravitational instability-driven turbulence in galactic discs
• Abundance-age relations with red clump stars in open clusters
• The Gaia-ESO Survey: Insights on the inner-disc evolution from open clusters
• Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE
• The First Neptune Analog or Super-Earth with Neptune-like Orbit: MOA-2013-BLG-605Lb
• How Many Elements Matter?
• Kinematics with Gaia DR2: The Force of a Dwarf
• Quantitative chemical tagging, stellar ages and the chemo-dynamical evolution of the Galactic disc
• Abundance patterns in early-type galaxies: is there a 'knee' in the [Fe/H] vs. [alpha/Fe] relation?
• OCCASO III. Iron peak and $\alpha$ elements of 18 open clusters. Comparison with chemical evolution models and field stars
• The Gaia-ESO Survey: New constraints on the Galactic disc velocity dispersion and its chemical dependencies
• On the origin of the Galactic thin and thick discs, their abundance gradients and the diagnostic potential of their abundance ratios
• Formation of S0 galaxies through mergers. Evolution in the Tully-Fisher relation since $z\sim 1$
• Chemodynamics of a Simulated Disc Galaxy: Initial Mass Functions and SNIa Progenitors
• Oxygen, α-element and iron abundance distributions in the inner part of the Galactic thin disc
• Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the $TESS$ Continuous Viewing Zones and beyond
• Chemical Cartography with APOGEE: Mapping Disk Populations with a Two-Process Model and Residual Abundances
• Cosmic phylogeny: reconstructing the chemical history of the solar neighbourhood with an evolutionary tree
• Impacts of a Flaring Star-forming Disc and Stellar Radial Mixing on the Vertical Metallicity Gradient
• Age-chemical abundance structure of the Galaxy I: Evidence for a late accretion event in the outer disc at z ~ 0.6
• OCCASO II. Physical parameters and Fe abundances of Red Clump stars in 18 Open Clusters
• Chemical separation of disc components using RAVE
• Unmixing the Galactic Halo with RR Lyrae tagging
• Constraining churning and blurring in the Milky Way using large spectroscopic surveys -- an exploratory study
• Quantifying radial migration in the Milky Way: Inefficient over short timescales but essential to the very outer disc beyond ~15 kpc
• The galactic habitable zone of the Milky Way and M31 from chemical evolution models with gas radial flows
• Radial Migration of the Sun in the Milky Way: a Statistical Study
• The Gaia-ESO Survey: A new approach to chemically characterising young open clusters II. Abundances of the neutron-capture elements Cu, Sr, Y, Zr, Ba, La, and Ce
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• A new method for estimating the pattern speed of spiral structure in the Milky Way
• H${}_2$O${}_2$ within chaos terrain on Europa's leading hemisphere
• Exploring the origin of thick disks using the NewHorizon and Galactica simulations
• Radial abundance gradients in the outer Galactic disk as traced by main-sequence OB stars
• A method to estimate stellar ages from kinematical data
• Constraining the solar neighbourhood age-metallicity relation from white dwarf-main sequence binaries
• Tracing the Milky Way warp and spiral arms with classical Cepheids
• Radial Migration from Metallicity Gradient of Open Clusters and Outliers
• Chronology of our Galaxy from Gaia Colour-Magnitude Diagram-fitting (ChronoGal). I. The formation and evolution of the thin disk from the Gaia Catalogue of Nearby Stars
• On the variation of carbon abundance in galaxies and its implications
• The stellar velocity distribution function in the Milky Way galaxy
• Mapping the Galactic Disk with the LAMOST and Gaia Red Clump Sample VII: the Stellar Disk Structure Revealed by the Mono-abundance Populations
• Stellar population astrophysics (SPA) with the TNG. Revisiting the metallicity of Praesepe (M44)
• The GAPS Programme at TNG XXVIII -- A pair of hot-Neptunes orbiting the young star TOI-942
• The Three-Phase Evolution of the Milky Way
• The Red and Featureless Outer Disks of Nearby Spiral Galaxies
• The AMBRE project: a study of Li evolution in the Galactic thin and thick discs
• The asymmetric drift, the local standard of rest, and implications from RAVE data
• Chemo-kinematics of the Milky Way from the SDSS-III MARVELS Survey
• The hunt for the Milky Way's accreted disc
• Chemical abundances and kinematics of 257 G-, K-type field giants. Setting a base for further analysis of giant-planet properties orbiting evolved stars
• The distribution of [$\alpha$/Fe] in the Milky Way disc
• The Vertical Metallicity Gradient of the Milky Way Disk: Transitions in [a/Fe] Populations
• The Gaia-ESO Survey: Churning through the Milky Way
• Yule-Simpson's paradox in Galactic Archaeology
• The Pristine survey XIII: Uncovering the very metal-poor tail of the thin disc
• The impact of early massive mergers on the chemical evolution of Milky Way-like galaxies: insights from NIHAO-UHD simulations
• From giant clumps to clouds -- II. The emergence of thick disc kinematics from the conditions of star formation in high redshift gas rich galaxies
• The AMBRE Project: r-process elements in the Milky Way thin and thick discs
• Cosmic variance in [O/Fe] in the Galactic disk
• APOGEE [C/N] Abundances Across the Galaxy: Migration and Infall from Red Giant Ages
• A self-consistent dynamical model of the Milky Way disc adjusted to Gaia data
• Abundance trend with condensation temperature for stars with different Galactic birth places
• Explaining the decrease in ISM lithium at super-solar metallicities in the solar vicinity
• The BaLROG project - II. Quantifying the influence of bars on the stellar populations of nearby galaxies
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• The rate of stellar encounters along a migrating orbit of the Sun
• The K2 Galactic Caps Project -- Going Beyond the \textit{Kepler} Field and Ageing the Galactic Disc
• Migration and Mixing in the Galactic Disc from Encounters between Sagittarius and the Milky Way
• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• [Mg/Fe] ratios in the solar neighbourhood: stellar yields and chemical evolution scenarios
• Abundances and kinematics for ten anticentre open clusters
• The innate origin of radial and vertical gradients in a simulated galaxy disc
• An HST Survey of Protostellar Outflow Cavities: Does Feedback Clear Envelopes?
• Milky Way Analogues in MaNGA: Multi-Parameter Homogeneity and Comparison to the Milky Way
• Deciphering the evolution of the Milky Way discs: Gaia APOGEE Kepler giant stars and the Besançon Galaxy Model
• The evolution of the Milky Way's thin disc radial metallicity gradient with K2 asteroseismic ages
• Open Clusters as Tracers on Radial Migration of the Galactic Disk
• Cosmic nucleosynthesis: a multi-messenger challenge
• Milky Way's Thick and Thin disk: Is there distinct thick disk?
• The Gaia-ESO Survey: the N/O abundance ratio in the Milky Way
• Understanding the evolution and dust formation of carbon stars in the LMC with a look at the JWST
• Stellar Population Astrophysics (SPA) with TNG Atmospheric parameters of members of 16 unstudied open clusters
• Modelling the chemical evolution of Zr, La, Ce and Eu in the Galactic discs and bulge
• Reliability and limitations of inferring birth radii in the Milky Way disk
• APOGEE chemical tagging constraint on the maximum star cluster mass in the $\alpha$-enhanced Galactic disk
• Migration in the shearing sheet and estimates for young open cluster migration
• The radial metallicity gradient and the history of elemental enrichment in M81 through emission-line probes
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• First metallicity determination from Near-Infrared spectra for five obscured Cepheids discovered in the inner Disk
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• On the mass and metallicity distribution of parent AGB stars of presolar SiC
• (Re)mind the gap: a hiatus in star formation history unveiled by APOGEE DR17
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• Resonant thickening of self-gravitating discs: imposed or self-induced orbital diffusion in the tightly wound limit
• The imprint of satellite accretion on the chemical and dynamical properties of disc galaxies
• Characterizing the radial oxygen abundance distribution in disk galaxies
• The GALAH Survey: Temporal Chemical Enrichment of the Galactic Disk
• Revisiting the Stellar Velocity Ellipsoid - Hubble type relation: observations versus simulations
• Detection of metallicity correlations in 100 nearby galaxies
• Open clusters and associations in the Gaia era
• 2D-Galactic chemical evolution: the role of the spiral density wave
• The last 5 Gyr of Galactic chemical evolution based on H II region abundances derived from a temperature independent method
• Neutron Star Mergers as the Main Source of R-process: Natal Kicks And Inside-Out Evolution to The Rescue
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• Spatial metallicity distribution statistics at $\lesssim 100$ pc scales in the AMUSING++ nearby galaxy sample
• The AMBRE Project: Solar neighbourhood chemodynamical constraints on Galactic disc evolution
• Observational Constraints of Radial Migration in the Galactic Disc Driven by the Slowing Bar
• A simple and general method for solving detailed chemical evolution with delayed production of iron and other chemical elements
• Universal properties of the high- and low-α disk: small intrinsic abundance scatter and migrating stars
• The Gaia-ESO Survey: Oxygen abundance in the Galactic thin and thick disks
• Numerical Simulation of a possible origin of the positive radial metallicity gradient of the thick disk
• Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution
• Secular resonant dressed orbital diffusion I : method and WKB limit for tepid discs
• Linking the formation and fate of exo-Kuiper belts within solar system analogues
• Fluorine Abundances in the Galactic Disk
• Metallicity Distribution of Disk Stars and the Formation History of the Milky Way
• Age-metallicity dependent stellar kinematics of the Milky Way disc from LAMOST and Gaia
• Revealing the spiral arms through radial migration and the shape of the Metallicity Distribution Function
• ISM metallicity variations across spiral arms in disk galaxies: the impact of local enrichment and gas migration in the presence of radial metallicity gradient
• Depletion and fractionation of nitrogen in collapsing cores
• 2D chemical evolution models II. Effects of multiple spiral arm patterns on O, Eu, Fe and Ba abundance gradients
• Secular resonant dressed orbital diffusion II : application to an isolated self similar tepid galactic disc
• Murchison Widefield Array rapid-response observations of the short GRB 180805A
• CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars
• Can ultralight dark matter explain the age-velocity dispersion relation of the Milky Way disc: A revised and improved treatment
• Radial migration in numerical simulations of Milky Way-sized galaxies
• On the Chemical and Structural Evolution of the Galactic Disk
• Self-similarity in the chemical evolution of galaxies and the delay time distribution of SNe Ia
• Fluorine Abundances in the Galactic Nuclear Star Cluster
• Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
• The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy
• Spectroscopy of Dwarf Stars Around the North Celestial Pole
• Metallicity Gradient of the Thick Disc Progenitor at High Redshift
• The Parent Populations of 6 groups identified from Chemical Tagging in the Solar neighborhood
• The CoRoT-GES Collaboration. Improving Red Giants spectroscopic surface gravity and abundances with asteroseismology
• The vertical metallicity gradients of mono-age stellar populations in the Milky Way with the RAVE and Gaia data
• Gas accretion in Milky Way-like galaxies: temporal and radial dependencies
• Stellar migration in the Auriga simulations
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• Galactic Archaeology with CoRoT and APOGEE: Creating mock observations from a chemodynamical model
• Asymmetric metallicity patterns in the stellar velocity space with RAVE
• Nucleosynthesis signatures of neutrino-driven winds from proto-neutron stars: a perspective from chemical evolution models
• Insights into the Formation and Evolution History of the Galactic Disk System
• GalCEM I -- An Open-Source Detailed Isotopic Chemical Evolution Code
• Stellar escapers from M67 can reach solar-like Galactic orbits
• Sun-like stars unlike the Sun: Clues for chemical anomalies of cool stars
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Efficient radial migration by giant molecular clouds in the first several hundred Myr after the stellar birth
• Using heritability of stellar chemistry to reveal the history of the Milky Way
• Local Stellar Kinematics from RAVE data -- VIII. Effects of the Galactic Disc Perturbations on Stellar Orbits of Red Clump Stars
• The chemical enrichment of the Milky Way disk evaluated using conditional abundances
• Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal) II. Unveiling the formation and evolution of the kinematically selected Thick and Thin Discs
• Neon, sulphur and argon abundances of planetary nebulae in the sub-solar metallicity Galactic anti-centre
• Milky Way chemo-dynamics in the era of Gaia
• SpectroTranslator: a deep-neural network algorithm to homogenize spectroscopic parameters
• Recent star formation episodes in the Galaxy: impact on its chemical properties and the evolution of its abundance gradient
• A Monte Carlo based simulation of the galactic chemical evolution of the Milky Way galaxy
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• The GALAH Survey: Dependence of elemental abundances on age and metallicity for stars in the Galactic disc
• The vertical structure of the spiral galaxy NGC 3501: first stages of the formation of a thin metal-rich disc
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (I) Temporal dependency
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Two-dimensional non-LTE \ion{O}{I} 777\,nm line formation in radiation hydrodynamics simulations of Cepheid atmospheres
• The formation history of the Milky Way disc with high-resolution cosmological simulations
• The GALAH Survey: Stellar parameters and abundances for 800,000 Gaia RVS spectra using GALAH DR4 and The Cannon
• Bar-spiral interaction produces radial migration and star formation bursts
• The Gaia-ESO Survey DR5.1 and Gaia DR3 GSP-Spec: a comparative analysis
• Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy
• Are Milky-Way-like galaxies like the Milky Way? A view from SDSS-IV/MaNGA
• A Galactic Self-Portrait: Density Structure and Integrated Properties of the Milky Way Disk
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• SSSpaNG! Stellar Spectra as Sparse, data-driven, Non-Gaussian processes
• Ensemble age inversions for large spectroscopic surveys
• The role of radial migration on tracing lithium evolution in the Galactic disk
• Stellar Population Astrophysics (SPA) with the TNG. alpha-elements, lithium, sodium and aluminum in 16 open clusters
• Gas Inflow and Outflow Histories in Disk Galaxies as Revealed from Observations of Distant Star-Forming Galaxies
• New Observational Constraints to Milky Way Chemodynamical models
• Bimodal Distribution of Galactic Disk Stars on the [alpha/Fe]-[Fe/H] Plane as a Possible Evidence of Discontinuous Radial Migration History
• Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
• The nature of the KFR08 stellar stream
• Shaping Galactic Habitability: the impact of stellar migration and gas giants
• Stellar Migration and Chemical Enrichment in the Milky Way Disc: A Hybrid Model
• Precision Pollution - The effects of enrichment yields and timing on galactic chemical evolution
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• Tracking Cluster Debris (TraCD)- I. Dissolution of clusters and searching the solar cradle
• Rubidium abundances in solar metallicity stars
• A slow spin to win -- the gradual evolution of the proto-Galaxy to the old disc
• Open cluster members in APOGEE DR17 I. Dynamics and star members
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Photometry of the Four Anti-Galactocentric Old Open Clusters: Czernik 30, Berkeley 34, Berkeley 75, and Berkeley 76
• The dawn is quiet here: Rise in [$\alpha$/Fe] is a signature of massive gas accretion that fueled proto-Milky Way
• Outer Regions of the Milky Way
• The SAMI Survey: Evidence for dynamical coupling of ionised gas and young stellar populations
• Transit Timing Variations of Five Transiting Planets
• Structural diversity of disc galaxies originating in the cold gas inflow from cosmic webs
• Solar twins in Gaia DR3 GSP-Spec I. Building a large catalog of Solar twins with ages
• Multi-epoch Low Radio Frequency Surveys of the Kepler K2 Mission Campaign Fields 3, 4, and 5 with the Murchison Widefield Array
• Gas-phase Elemental abundances in Molecular cloudS (GEMS) XI. The evolution of HCN, HNC, and N2H+ isotopic ratios in starless cores
• Rediscovering the Milky Way with orbit superposition approach and APOGEE data III. Panoramic view of the bulge
• Photometric stellar parameters for asteroseismology and Galactic studies
• Modelling the chemical evolution of the Milky Way
• Lessons learnt from the Solar neighbourhood and the Kepler field
• How does the stellar disk of the Milky Way get its gas?
• The age-metallicity structure of the Milky Way disc with APOGEE
• Revisiting the Radial Metallicity Gradient-Age Relation in the Milky Way's Thin and Thick Disks
• Revisiting the Galactic age-metallicity relation from wide white dwarf-main-sequence binaries
• Asteroseismology of red giants & galactic archaeology
• The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
• A hybrid SLAM-Payne framework for atmospheric parameter and abundance determination of early-type Stars from LAMOST DR9 low-resolution Spectra
• Neutron-capture elements record the ordered chemical evolution of the disc over time
• QED V: Variations in metal loading of galactic winds with element nucleosynthetic origin
• The cosmic journey of dust grains -- from nucleation to planetary system
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• Chemical evolution history of MaNGA galaxies