Galactic Chemical Evolution: Hydrogen Through Zinc

Abstract

Using the output from a grid of 60 Type II supernova models (Woosley \& Weaver 1994) of varying mass (11 $\ltaprx$ M/M\sun $\ltaprx$ 40) and metallicity (0, 10${}^{-4}$, 0.01, 0.1, and 1 Z\sol), the chemical evolution of 76 stable isotopes, from hydrogen to zinc, is calculated. The chemical evolution calculation employs a simple dynamical model for the Galaxy (infall with a 4 billion year $e$-folding time scale onto a exponential disk and 1/r${}^2$ bulge), and standard evolution parameters, such as a Salpeter initial mass function and a quadratic Schmidt star formation rate. The theoretical results are compared in detail with observed stellar abundances in stars with metallicities in the range -3.0 $\ltaprx$ [Fe/H] $\ltaprx$ 0.0 dex. While our discussion focuses on the solar neighborhood where there are the most observations, the supernovae rates, an intrinsically Galactic quantity, are also discussed.

114 pages including 39 figures, uuencoded gzipped postscript; accepted ApJ Supp

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• Evolution of the Abundance of CO, O2, and Dust in the Early Universe
• Mn, Cu and Zn abundances in barium stars and their correlations with neutron capture elements
• Planet formation throughout the Milky Way: Planet populations in the context of Galactic chemical evolution
• Finding cool subdwarfs using a V-J reduced proper-motion diagram: Stellar parameters for 91 candidates
• The HST large programme on $\omega$ Centauri -- V. Exploring the Ultracool Dwarf Population with Stellar Atmosphere and Evolutionary Modelling
• 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 Origin of Cosmic Rays: How Their Composition Defines Their Sources and Sites, and the Processes of Their Mixing, Injection and Acceleration
• The chemical evolution of the Galaxy: the importance of stars with an initial mass larger than 40Mo
• A Bare Molecular Cloud at z~0.45
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• Impact of hypernova νp-process nucleosynthesis on the galactic chemical evolution of Mo and Ru
• Metallicity-Dependent Galactic Isotopic Decomposition for Nucleosynthesis
• Star Formation Histories versus Redshift : Consequences for Overall Metallicity and Deuterium Destruction
• Chemical abundances of two extragalactic young massive clusters
• Gravitational wave background from Population III black hole formation
• A New Chemical Evolution Model for Dwarf Spheroidal Galaxies based on Observed Long Star Formation Histories
• Abundance analysis of a CEMP-no star in the Carina dwarf spheroidal galaxy
• Oxygen isotopic ratios in first dredge-up red giant stars and nuclear reaction rate uncertainties revisited
• MINCE I. Presentation of the project and of the first year sample
• The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky Way
• A search for cool subdwarfs: Stellar parameters for 134 candidates
• A Concise Treatise on Converting Stellar Mass Fractions to Abundances to Molar Ratios
• Investigation of the Puzzling Abundance Pattern in the Stars of the Fornax Dwarf Spheroidal Galaxy
• Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid
• Can Stellar Yields Accurately Constrain the Upper Limit to the Initial Mass Function?
• Enrichment of the Galactic disc with neutron capture elements: Sr
• Limits on Pauli principle violation by nucleons
• Analysis of the TiO isotopologues in stellar optical spectra
• The Distribution of Metallicities in the Local Galactic Interstellar Medium
• The Early Chemical Enrichment Histories of Two Sculptor Group Dwarf Galaxies as Revealed by RR Lyrae Variables
• Evolution of O Abundance Relative to Fe
• Fluorine Abundances in the Galactic Disk
• Chemical Evolution of Fluorine in the Milky Way
• Detection of Al II in the Ultraviolet Spectra of Metal-Poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
• Stellar Metallicities and SNIa Rates in the Early-type Galaxy NGC5846 from ROSAT and ASCA Observations
• The Abundance of Boron in Diffuse Interstellar Clouds
• Isotopic Titanium Abundances in Local M Dwarfs
• On the oxygen isotopic composition of the Solar System
• Empirically Derived Integrated Stellar Yields of Fe-Peak Elements
• Wide-field CO isotopologue emission and the CO-to-H${}_2$ factor across the nearby spiral galaxy M101
• Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937
• Pre-explosive accretion and simmering phases of Type Ia Supernovae
• Argon and Silicon abundances in the damped Ly-alpha system I Zw 18
• No Surviving SN Ia Companion In SNR 0509-67.5: Stellar Population Characterization and Comparison To Models
• Fluorine Abundances in the Galactic Nuclear Star Cluster
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• Checking Potassium origin of new emission line at 3.5 keV with K XIX line complex at 3.7 keV
• Spectroscopic study of the elusive globular cluster ESO452-SC11 and its surroundings
• Abundance ratios in dwarf elliptical galaxies
• Nucleosynthetic yields of Z=$10^{-5}$ intermediate-mass stars
• Searching for a Hypervelocity White Dwarf Companion: A Proper Motion Survey of SN 1006
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• Chemical Abundances of Globular Clusters in NGC 5128 (Centaurus A)
• The Galactic Spatial Distribution of OB Associations and Their Surrounding Supernova-Generated Superbubble
• The Evolution Of Carbon, Sulphur, and Titanium Isotopes from High-Redshift to the Local Universe
• Evidence of a Cloud-Cloud Collision from Overshooting Gas in the Galactic Center
• Simulating a White Dwarf-dominated Galactic Halo
• A Test for the Nature of the Type Ia Supernova Explosion Mechanism
• Abundances of metal-weak thick-disc candidates
• A CO Funnel in the Galactic Centre: Molecular Counterpart of the Northern Galactic Chimney?
• Manganese evolution in Omega Centauri: a clue to the cluster formation mechanisms?
• Composite Stellar Populations and Element by Element Abundances in the Milky Way Bulge and Elliptical Galaxies
• Realistic Earth matter effects and a method to acquire information about small θ_{13} in the detection of supernova neutrinos
• Uniform Silicon Isotope Ratios Across the Milky Way Galaxy
• GalCEM I -- An Open-Source Detailed Isotopic Chemical Evolution Code
• First detection of AlF line emission towards M-type AGB stars
• Cobalt and copper abundances in 56 Galactic bulge red giants
• The Chemical Evolution of Iron-Peak Elements with Hypernovae
• The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
• Populations of evolved massive binary stars in the Small Magellanic Cloud II: Predictions from rapid binary evolution
• Parameterisations of thermal bomb explosions for core-collapse supernovae and 56Ni production
• Chandrasekhar-mass white dwarfs are the progenitors of a small fraction of Type Ia supernovae according to nucleosythesis constraints
• Millimeter Spectral Line Mapping Observations Toward Four Massive Star Forming HII Regions
• Outside-in stellar formation in the spiral galaxy M33?
• Chemical Evolution of Odd Elements in an Inhomogeneous Early Galaxy
• NLTE Analysis of Copper Abundances in the Galactic Bulge Stars
• Diverse Supernova Sources for the r-Process and Abundances in Metal-Poor Stars
• Observational constraints on the origin of the elements. IX. 3D NLTE abundances of metals in the context of Galactic Chemical Evolution Models and 4MOST
• Recent Progress in Nuclear Astrophysics
• A Monte Carlo based simulation of the galactic chemical evolution of the Milky Way galaxy
• The s-process enriched star HD 55496: origin from a globular cluster or from the tidal disruption of a dwarf galaxy?
• The Chemical Evolution of Globular Clusters - II. Metals and Fluorine
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• Can Galactic chemical evolution explain the oxygen isotopic variations in the Solar System?
• The evolution of the galaxy and the birth of the solar system: The short-lived nuclides connection
• Yields of Massive Stars and their Role in Galactic Chemical Evolution Studies
• Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
• High-resolution spectroscopic analysis of four new chemically peculiar stars
• Reaction rates for the ${}^{39}$K(p,$\gamma$)${}^{40}$Ca reaction
• Gravitational wave background from neutron star phase transition
• Chemical composition of stars with massive planets
• A non-LTE study of silicon abundances in giant stars from the Si I infrared lines in the zJ-band
• Aeos: Transport of Metals from Minihalos following Population III Stellar Feedback
• Synergies between interstellar dust and heliospheric science with an Interstellar Probe
• Modelling the chemical evolution of molecular clouds as a function of metallicity
• Distributions of Long-Lived Radioactive Nuclei Provided by Star Forming Environments
• The Role of Radioactivities in Astrophysics
• Measuring Dwarf Galaxy Intrinsic Abundance Scatter with Mid-resolution Spectroscopic Surveys: Calibrating APOGEE Abundance Errors
• Molecules, shocks, and disk in the axi-symmetric wind of the MS-type AGB star RS Cancri
• Thermal Regulation and the Star-Forming Main Sequence
• Narrowband Ca Photometry for Dwarf Spheroidal Galaxies. I. Chemostructural Study on Draco, Sextans, and Canes Venatici I
• The Radial Distribution of Mono-Metallicity Populations in the Galactic Disk as Evidence for Two-Phase Disk Formation
• Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars
• Effective Star Formation Rates for Cosmological Applications
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• Galactic Chemical Evolution Redux: Atomic Numbers 6 < Z < 15
• Theoretical Distributions of Short-Lived Radionuclides for Star Formation in Molecular Clouds
• Chemical composition of the outer halo globular cluster Palomar 15
• Kicked neutron stars and microlensing
• The Impact of Inelastic Collisions with Hydrogen on NLTE Copper Abundances in Metal-Poor Stars
• Magnesium isotope ratios in Milky Way and dwarf galaxy stars
• Peculiarities of α-element abundances in Galactic open clusters
• MINCE III. Detailed chemical analysis of the UVES sample
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• New sub-grouping of multiple stellar populations in NGC 2808 based on low-resolution spectroscopy
• Very-high-energy gamma-ray observations of the Type Ia Supernova SN 2014J with the MAGIC telescopes
• Be, V and Cu in the halo star CS 31082-001 from near-UV spectroscopy
• Background of gravitational waves from pre-galactic black hole formation
• Exploring giant barium stars: ${}^{12}\mathrm{C}{/}^{13}\mathrm{C}$ ratio and elemental abundances of carbon, nitrogen, and oxygen
• Study of the abundance features of the metal-poor star HD 94028
• Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant
• Chemical Evolution of the Juvenile Universe
• Energetic constraints to chemo-photometric evolution of spiral galaxies
• The Origin of the Metal-Poor Common Proper Motion Pair HD 134439/134440: Insights from New Elemental Abundances
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
• J01020100-7122208: an accreted evolved blue straggler that wasn't ejected from a supermassive black hole
• Dependence of the Sr-to-Ba and Sr-to-Eu Ratio on the Nuclear Equation of State in Metal Poor Halo Stars
• Contributions of supernovae type II & Ib/c to the galactic chemical evolution
• The metal-poorest tail of the Galactic halo: hypothesis on its origin from precise spectral analysis
• The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates
• The Origin of the Large Magellanic Cloud Globular Cluster NGC 2005
• A theoretical investigation of far-infrared fine structure lines at $z>6$ and of the origin of the [OIII]88/[CII]158 enhancement
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• Astrophysical Origins for the Unusual Chemical Abundance of the Globular Cluster Palomar 1
• New experimental ${}^{23}$Na($\alpha ,p$)${}^{26}$Mg Reaction Rate for Massive Star and Type-Ia Supernova models
• Big Bang Nucleosynthesis, Population III, and Stellar Genetics in the Galactic Halo
• SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604
• Primordial Black Hole Triggered Type Ia Supernovae II: Comparison with Supernova Remnants and Galactic Chemical Evolution
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Gravitational wave background from neutron star phase transition for a new class of equation of state
• On the Galactic chemical evolution of sulphur. Sulphur abundances from the [S i] 1082 nm line in giants
• EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy
• Stellar Abundances at the Center of Early Type Galaxies with Fine Structure
• Perspectives in Galactic Chemical Evolution studies
• Oxygen and Aluminum-Magnesium Isotopic Systematics of Presolar Nanospinel Grains from CI Chondrite Orgueil
• When Stars Mimic Monsters: Spectral Evidence for an $\eta$ Carinae-like Giant Eruption in SBS 0335$-$052 E
• Nitrogen Abundances and the Distance Moduli of the Pleiades and Hyades
• Neutron-capture elements record the ordered chemical evolution of the disc over time
• Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies
• Modelling the chemical evolution
• The Two-infall Model Revisited: Constraints on Milky Way Bulge Assembly from >30,000 Galactic Chemical Evolution Models and Machine Learning
• Cepheid Metallicity in the Leavitt Law (C--MetaLL) survey: VIII. High-Resolution IGRINS Spectroscopy of 23 Classical Cepheids: Validating NIR Abundances