The Chemical Evolution of the Galaxy: the two-infall model

Abstract

In this paper we present a new chemical evolution model for the Galaxy which assumes two main infall episodes for the formation of halo-thick disk and thin disk, respectively. We do not try to take into account explicitly the evolution of the halo but we implicitly assume that the timescale for the formation of the halo was of the same order as the timescale for the formation of the thick disk. The formation of the thin-disk is much longer than that of the thick disk, implying that the infalling gas forming the thin-disk comes not only from the thick disk but mainly from the intergalactic medium. The timescale for the formation of the thin-disk is assumed to be a function of the galactocentric distance, leading to an inside-out picture for the Galaxy building. The model takes into account the most up to date nucleosynthesis prescriptions and adopts a threshold in the star formation process which naturally produces a hiatus in the star formation rate at the end of the thick disk phase, as suggested by recent observations. The model results are compared with an extended set of observational constraints. Among these constraints, the tightest one is the metallicity distribution of the G-dwarf stars for which new data are now available. Our model fits very well these new data. We show that in order to reproduce most of these constraints a timescale $\le 1$ Gyr for the (halo)-thick-disk and of 8 Gyr for the thin-disk formation in the solar vicinity are required. We predict that the radial abundance gradients in the inner regions of the disk ($R<R_{\odot }$) are steeper than in the outer regions, a result confirmed by recent abundance determinations, and that the inner ones steepen in time during the Galactic lifetime.

48 pages, 20 Postscript figures, AASTex v.4.0, to be published in Astrophysical Journal

References in corpus (6)

• Galactic Chemical Evolution: Hydrogen Through Zinc
• Chemistry and Kinematics in the Solar Neighborhood: Implications for Stellar Populations and for Galaxy Evolution
• The metallicity distribution of G dwarfs in the solar neighbourhood
• The Outer Regions of the Galactic Bulge:II Analysis
• Galactic Evolution Of D And 3He Including Stellar Production Of 3He
• Chemical evolution models with a new stellar nucleosynthesis

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• An [$\alpha$/Fe]-enhanced thick disk in a Milky Way Analogue
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• Multiwavelength Absolute Magnitudes and Colours of Red Clump Stars in {\it Gaia} Era
• (Re)mind the gap: a hiatus in star formation history unveiled by APOGEE DR17
• Infrared Spectroscopy of the Diffuse Ionized Halo of NGC 891
• Modelling the chemical evolution of the Galaxy halo
• From globular clusters to the disc: the dual life of our Galaxy
• Modelling the nova rate in galaxies
• Clues to the nature of damped Lyman alpha systems from chemical evolution models
• The Chemical Evolution of the Milky Way
• A cosmological study of the star formation history in the solar neighbourhood
• Are ancient dwarf satellites the building blocks of the Galactic halo?
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• On the evolution of the Fe abundance and of the Type Ia SN rate in clusters of galaxies
• The Hydra I cluster core. I. Stellar populations in the cD galaxy NGC 3311
• The thick disk rotation-metallicity correlation as a fossil of an "inverse chemical gradient" in the early Galaxy
• Infrared Spectroscopy of Halos of Edge-on Galaxies
• Hitting the Bull's-eye: The Radial Profile of Accretion and Star Formation in the Milky Way
• Formation of Galactic Systems in Light of the Magnesium Abundance in Field Stars: The Thick Disk
• The velocity ellipsoid in the Galactic disc using Gaia DR1
• The relationship between age, metallicity, and abundances for disk stars in a simulated Milky Way galaxy
• The Black Hole Mass Function Across Cosmic Times I. Stellar Black Holes and Light Seed Distribution
• A2A: 21,000 bulge stars from the ARGOS survey with stellar parameters on the APOGEE scale
• Mapping radial abundance gradients with Gaia-ESO open clusters: Evidence of recent gas accretion in the Milky Way disk
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• The AMBRE Project: Spectrum normalisation influence on Mg abundances in the metal-rich Galactic disc
• Impact of distance determinations on Galactic structure. I. Young and intermediate-age tracers
• The contribution from rotating massive stars to the enrichment in Sr and Ba of the Milky Way
• Extragalactic archeology with the GHOSTS Survey I. - Age-resolved disk structure of nearby low-mass galaxies
• Galaxy Evolution, Deep Galaxy Counts and the Near-IR Cosmic Infrared Background
• Observational constraints on the origin of the elements. V. Non-LTE abundance ratios of [Ni/Fe] in Galactic stars and enrichment by sub-Chandrasekhar mass SNe
• The chemical evolution of the Galaxy: the importance of stars with an initial mass larger than 40Mo
• Chronology of the chemical enrichment of the old Galactic stellar populations
• The nature of the Milky Way's stellar halo revealed by the three integrals of motion
• Metallicity-Dependent Galactic Isotopic Decomposition for Nucleosynthesis
• An excessively massive thick disc of the enormous edge-on lenticular galaxy NGC7572
• The last 5 Gyr of Galactic chemical evolution based on H II region abundances derived from a temperature independent method
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• A Two-Phase Chemical Enrichment Model for the Milky Way Globular Cluster System
• Mapping electron temperature variations across a spiral arm in NGC 1672
• MINCE I. Presentation of the project and of the first year sample
• Chemical Evolution of Galaxies
• The AMBRE Project: Solar neighbourhood chemodynamical constraints on Galactic disc evolution
• An Intermediate-age Alpha-rich Galactic Population in K2
• The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky Way
• The connection between Gamma-ray bursts and Supernovae Ib/c
• A simple and general method for solving detailed chemical evolution with delayed production of iron and other chemical elements
• LAMOST Medium-Resolution Spectral Survey of Galactic Nebula (LAMOST MRS-N): An overview of Scientific goals and Survey plan
• The imprint of clump formation at high redshift. II. The chemistry of the bulge
• X-ray Observations of the Bright Old Nova V603 Aquilae
• Did the Milky Way just light up? The recent star formation history of the Galactic disc
• Metallicity Distribution of Disk Stars and the Formation History of the Milky Way
• The Distribution of Metallicities in the Local Galactic Interstellar Medium
• The Gaia-ESO Survey: Oxygen abundance in the Galactic thin and thick disks
• Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution
• Green Bank Telescope Observations of 3He+: HII Regions
• Manganese Abundances in the Globular Cluster Omega Centauri
• Chemical Evolution of Fluorine in the Milky Way
• Formation of Galactic Systems in Light of the Magnesium Abundance in Field Stars: The Thin Disk
• ISM metallicity variations across spiral arms in disk galaxies: the impact of local enrichment and gas migration in the presence of radial metallicity gradient
• Analytic solution of Chemical Evolution Models with Type Ia SNe
• Star-forming rings in lenticular galaxies: origin of the gas
• SNII enrichment and the star cluster mass function
• Star Formation in Two Luminous Spiral Galaxies
• The structure of spiral galaxies: radial profiles in stellar Mass-to-Light ratio and the Dark Matter distribution
• Local Stellar Kinematics from RAVE data - VI. Metallicity Gradients Based on the F-G Main-sequence Stars
• The chemical properties of the Milky Way's on-bar and off-bar regions: evidence for inhomogeneous star formation history in the bulge
• Cosmic Star Formation: Constraints on the Galaxy Formation Models
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• $Chempy$: A flexible chemical evolution model for abundance fitting - Do the Sun's abundances alone constrain chemical evolution models?
• Empirically Derived Integrated Stellar Yields of Fe-Peak Elements
• Disc dichotomy signature in the vertical distribution of [Mg/Fe] and the delayed gas infall scenario
• Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: VI: Radial abundance gradients of 29 chemical species in the Milky Way Disk
• Self-similarity in the chemical evolution of galaxies and the delay time distribution of SNe Ia
• The Impact of Stellar Migration on Disk Outskirts
• Chemical evolution of ${}^{26}$Al and ${}^{60}$Fe in the Milky Way
• The age of the Galactic thin disk from Th/Eu nucleocosmochronology II. Chronological analysis
• Cardinal kinematics: I. Rotation fields of the APOGEE Survey
• Cosmic star formation rate: a theoretical approach
• Nucleosynthetic yields of Z=$10^{-5}$ intermediate-mass stars
• The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy
• The Evolution Of Carbon, Sulphur, and Titanium Isotopes from High-Redshift to the Local Universe
• A Unified Exploration of the Chronology of the Galaxy
• The Gaia-ESO survey: placing constraints on the origin of r-process elements
• Tracing birth properties of stars with abundance clustering
• Co-spatial Long-slit UV/Optical Spectra of Ten Galactic Planetary Nebulae with HST/STIS II. Nebular Models, Central Star Properties and He+CNO Synthesis
• The Influence of Radial Stellar Migration on the Chemical Evolution of the Milky Way
• Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
• Fossil Imprints of Outflow from the Galactic Bulge in Elemental Abundances of Metal-Rich Disk Stars
• Nitrogen evolution in the halo, thick disc, thin disc and bulge of the Galaxy
• PN-Carbon Yields and the Chemical Evolution of the Galactic Disk
• Manganese evolution in Omega Centauri: a clue to the cluster formation mechanisms?
• SDSS-IV MaNGA: the "G-dwarf problem" revisited
• Impact of AGB stars on the chemical evolution of neutron-capture elements
• Orbital and atmospheric parameters of two wide O-type subdwarf binaries: BD$-$11${}^{\mathrm{o}}$162 and Feige 80
• The Magellanic Clouds and the Primordial Helium Abundance
• The two regimes of the cosmic sSFR evolution are due to spheroids and discs
• Modelling chemical clocks -- Theoretical evidences of the space and time evolution of [s/alpha] in the Galactic disc with Gaia-ESO survey
• Kinematics of Stellar Populations with RAVE Data
• Type Ia supernovae in a hierarchical galaxy formation model: the Milky Way
• Sun-like stars unlike the Sun: Clues for chemical anomalies of cool stars
• Helium contamination from the progenitor stars of planetary nebulae: The He/H radial gradient and the Delta Y/Delta Z enrichment ratio
• Exploring the Evolution of Massive Clumps in Simulations that Reproduce the Observed Milky Way α-element Abundance Bimodality
• The earliest phases of CNO enrichment in galaxies
• The Galactic thick and thin disks: differences in evolution
• Outside-in stellar formation in the spiral galaxy M33?
• Mock Observations: Formation and Evolution of diffuse light in Galaxy Groups and Clusters in the IllustrisTNG Simulations
• Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VIII. Carbon and oxygen
• Local Stellar Kinematics from RAVE data -- VIII. Effects of the Galactic Disc Perturbations on Stellar Orbits of Red Clump Stars
• CLUES about M33: the reversed radial stellar age gradient in the outskirts of Triangulum galaxy
• Spectroscopic Identification and Chemical Distribution of HII Regions in the Galactic Anti-center Area from LAMOST
• Using heritability of stellar chemistry to reveal the history of the Milky Way
• Role of galactic gaseous halos in recycling enriched winds from bulges to disks: A new bulge-disk chemical connection
• On the delay times of merging double neutron stars
• The Chemical Abundance Structure of the Inner Milky Way: A Signature of "Upside-Down" Disk Formation?
• 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
• Chemical Evolution of the Galaxy Based on the Oscillatory Star Formation History
• The G-dwarf distribution in star-forming galaxies: a tug-of-war between infall and outflow
• Untangling the Sources of Abundance Dispersion in Low-Metallicity Stars
• Neon, sulphur and argon abundances of planetary nebulae in the sub-solar metallicity Galactic anti-centre
• Unveiling the chemical fingerprint of phosphorus-rich stars I. In the infrared region of APOGEE-2
• Colour-magnitude diagram in simulations of galaxy formation
• A Blueprint for the Milky Way's Stellar Populations. IV. A String of Pearls $-$ the Galactic Starburst Sequence
• Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars
• The role of massive stars in galactic chemical evolution
• A Monte Carlo based simulation of the galactic chemical evolution of the Milky Way galaxy
• Chemical and photometric evolution models for disk, irregular and low mass galaxies
• The Role of a Hot Gas Environment on the Evolution of Galaxies
• The GALAH Survey: Dependence of elemental abundances on age and metallicity for stars in the Galactic disc
• Recent star formation episodes in the Galaxy: impact on its chemical properties and the evolution of its abundance gradient
• Planetary nebulae: abundances and abundance gradients
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• Stochastic processes, galactic star formation, and chemical evolution. Effects of accretion, stripping, and collisions in multiphase multi-zone models
• Chemical Evolution of the Galactic Disk and Bulge
• BreakBRD Galaxies I: Global Properties of Spiral Galaxies with Central Star Formation in Red Disks
• The evolution of the galaxy and the birth of the solar system: The short-lived nuclides connection
• A formation timescale of the Galactic halo from Mg isotopes in dwarf stars
• Metallicity gradients in the Milky Way
• Europium, we have a problem. Modelling r-process enrichment across Local Group galaxies
• The GALAH Survey: Stellar parameters and abundances for 800,000 Gaia RVS spectra using GALAH DR4 and The Cannon
• Measuring the physical imprints of gas flows in galaxies I: Accretion rate histories
• Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages
• The nature of Long-GRB host galaxies from chemical abundances
• Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy
• Estimating the age-metallicity distribution of a stellar sample from the probability distributions of the individual stars
• Chemical evolution of elliptical galaxies I: supernovae and AGN feedback
• Heterogeneous evolution of the galaxy and the origin of the short-lived nuclides in the early solar system
• The Gaia-ESO Survey DR5.1 and Gaia DR3 GSP-Spec: a comparative analysis
• 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
• Galactic Chemical Evolution Redux: Atomic Numbers 6 < Z < 15
• Geometrical tests of cosmological models. I. Probing dark energy using the kinematics of high-redshift galaxies
• New Observational Constraints to Milky Way Chemodynamical models
• Galactic disks and their evolution
• Gas Inflow and Outflow Histories in Disk Galaxies as Revealed from Observations of Distant Star-Forming Galaxies
• Nitrogen Abundance Distribution in the inner Milky Way
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
• Stellar Migration and Chemical Enrichment in the Milky Way Disc: A Hybrid Model
• Constraints on $R$-process Nucleosynthesis from ${}^{129}$I and ${}^{247}$Cm in the Early Solar System
• Geoastronomy: Rocky planets as the Lavosier-Lomonosov Bridge from the non-living to the living world
• Chemodynamical Ages of Small-Scale Kinematic Structures of the Galactic Disc in the Solar Neighborhood from ~250,000 K and M Dwarfs
• Shaping Galactic Habitability: the impact of stellar migration and gas giants
• Young Open Star Clusters: The Spatial Distribution of Metallicity in the Solar Neighborhood
• Measuring 60-pc-scale Star Formation Rate of the Nearby Seyfert Galaxy NGC 1068 with ALMA, HST, VLT/MUSE, and VLA
• Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
• Extraplanar Dust in Spiral Galaxies: Tracing Outflows in the Disk-Halo Interface
• Bimodal Distribution of Galactic Disk Stars on the [alpha/Fe]-[Fe/H] Plane as a Possible Evidence of Discontinuous Radial Migration History
• Reconstructing the Milky Way chemical map with Galactic Chemical Evolution tool OMEGA+ from SDSS-MWM
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• Energetic constraints to chemo-photometric evolution of spiral galaxies
• Spectral synthesis techniques for supernovae and kilonovae
• Extragalactic Planetary Nebulae: tracers of the chemical evolution of nearby galaxies
• A Statistical Study of H I Gas in Nearby Narrow-Line AGN-Hosting Galaxies
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• Unveiling VVV/WISE Mira variables on the far side of the Galactic disk: Distances, kinematics and a new extinction law
• The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
• Chemodynamics of the Milky Way and disc formation history: insight from the RAVE and Gaia-ESO surveys
• A study of outer disk stellar populations of face-on star-forming galaxies in SDSS-IV MaNGA: causes of H$\alpha$ deficiency
• On the Use of Field RR Lyrae as Galactic Probes -- VIII. Early Formation of the Galactic Spheroid
• Search for the metal-weak thick disk from the LAMOST DR5
• A slow spin to win -- the gradual evolution of the proto-Galaxy to the old disc
• Quantifying chemical and kinematical properties of Galactic disks
• NLTE abundances of Cr in the Sun and metal-poor stars
• Predicting interstellar radiation fields from chemical evolution models
• Outer Regions of the Milky Way
• Modelling the chemical evolution of the Milky Way
• Contributions of supernovae type II & Ib/c to the galactic chemical evolution
• On the large-scale structure of galactic disks
• Disentanglement of the chemodynamical assembly: mapping the Milky Way disks
• Hot accretion onto spiral galaxies: the origin of extended and warped HI discs
• The Multiplicity of Main Sequence Turnoffs in Globular Clusters
• The timescales of chemical enrichment in the Galaxy
• Disk galaxy evolution: from the Milky Way to high-redshift disks
• Local metallicity distribution function derived from Galactic large-scale radial iron pattern modelling
• Determining distances using asteroseismic methods
• Neutrinos from stars in the Milky Way
• Very Massive Close Binaries and the Puzzling Temporal Evolution of 14N in the Solar Neighbourhood
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• Towards Understanding the Milky Way's Typicality: Assessing the Chemodynamics of M31's Bulge & Bar, Thick & Thin Discs
• The influence of nova nucleosynthesis on the chemical evolution of the Galaxy
• Cosmic Radioactivity and Galactic Chemical Evolution
• The evolution of the Oxygen abundance radial gradient in the Milky Way Galaxy disk
• Using N-body simulations to understand the chemo-dynamical evolution of the inner Milky Way
• How does the stellar disk of the Milky Way get its gas?
• Distribution and Evolution of Metals in the Magneticum simulations
• Galaxy formation and chemical evolution
• Close Pairs as Probes of the Galaxy's Chemical Evolution
• Short-lived Radionuclides in the Milky Way Galaxy
• Turning Points in the Age-Metallicity Relations -- Created by Late Satellite Infall and Enhanced by Radial Migration
• The effects of a Variable IMF on the Chemical Evolution of the Galaxy
• On the Galactic chemical evolution of sulphur. Sulphur abundances from the [S i] 1082 nm line in giants
• Modelling the chemical evolution
• Old open clusters as key tracers of Galactic chemical evolution. I. Fe abundances in NGC 2660, NGC 3960, and Berkeley 32
• Galactic evolution of D, 3He and 4He
• A Census of Sun's Ancestors and their Contributions to the Solar System Chemical Composition
• Formation of Disk Galaxies: On the Angular Momentum Problem, the Tully-Fisher Relation and Magnetohydrodynamics
• Rapid early gas accretion for the inner Galactic disc
• Measuring Cosmic Elements with Gamma-Ray Telescopes
• Fundamental mechanism of the creation of chemical bimodality in the Milky Way disc in the cold accretion theory
• Neutron-capture elements record the ordered chemical evolution of the disc over time
• A comparative study of O, Ne, Cl, and Ar in Hii regions and PNe of the Galactic disk: Temporal evolution of radial gradients?
• The multiple corrugations in the Galactic disk derived from the LAMOST and Gaia survey data
• KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at $z\sim 1.5$
• Dynamical properties of high-[Mg/Fe] stars in the Milky Way bar region
• QED V: Variations in metal loading of galactic winds with element nucleosynthetic origin
• A hybrid SLAM-Payne framework for atmospheric parameter and abundance determination of early-type Stars from LAMOST DR9 low-resolution Spectra
• Two sequences in the age-metallicity relation as seen from [C/N] abundances in APOGEE
• Closing remarks and Outlook
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• Origin of the Galactic Halo: accretion vs. in situ formation
• The role of HI in regulating size growth of local galaxies