The Evolution of the Elemental Abundances in the Gas and Dust Phases of the Galaxy

Abstract

We present models for the evolution of the elemental abundances in the gas and dust phases of the interstellar medium (ISM) of our Galaxy by generalizing standard models for its dynamical and chemical evolution. In these models, the stellar birthrate history is determined by the infall rate of primordial gas, and by its functional dependence on the mass surface density of the stars and gas. We adopt a two component model for the Galaxy, consisting of a central bulge and an exponential disk with different infall rates and stellar birthrate histories. Condensation in stellar winds, Type Ia and Type II supernovae, and the accretion of refractory elements onto preexisting grains in dense molecular clouds are the dominant contributors to the abundance of elements locked up in the dust. Grain destruction by sputtering and evaporative grain-grain collisions in supernova remnants are the most important mechanisms that return these elements back to the gas phase. We calculate the dust production rate by the various dust sources, analyze the origin of the elemental depletion pattern, and study the relation between dust abundance and ISM metallicity, and the evolution of the the dust abundance and composition at each Galactocentric radius as a function of time. The derived relation of dust mass with metallicity is compared to the observed Galactic dust abundance gradient, and to the M${}_{dust}$ versus log(O/H) relation that is observed in external Dwarf galaxies. The dependence of dust composition on the mass of the progenitor star, and the delayed recycling of newly synthesized dust by low mass stars back to the ISM give rise to variations in the dust composition as a function of time. Our models provide a framework for the self-consistent inclusion of dust in

AAS TeX manuscript - submitted to ApJ (47 pages) + 15 Figures corrected figure files

References in corpus (4)

• Dust-to-gas Ratio and Metal Abundance in Dwarf Galaxies
• Can Composite Fluffy Dust Particles Solve the Interstellar Carbon Crisis?
• A New Approach to Determine the Initial Mass Function in the Solar Neighborhood
• Signatures of Intergalactic Dust From the First Supernovae

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• Simulations Find Our Accounting of Dust-Obscured Star Formation May Be Incomplete
• Modelling the evolution of PAH abundance in galaxies
• Starbursts and dusty tori in distant 3CR radio galaxies
• The mass-loss rates of red supergiants at low metallicity: Detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• The dust attenuation law in $z\sim 6$ quasars
• The Contribution of Evolved Stars to PAH Heating and Implications for Estimating Star Formation Rates
• Galactic dust evolution with rapid dust formation in the interstellar medium due to hypersonic turbulence
• The interstellar medium in Andromeda's dwarf spheroidal galaxies: I. Content and origin of the interstellar dust
• HERschel Observations of Edge-on Spirals (HEROES). II: Tilted-ring modelling of the atomic gas disks
• Dust diffusion in SPH simulations of an isolated galaxy
• Constraint on dust evolution processes in normal galaxies at $z>6$ detected by ALMA
• Evolution of dust porosity through coagulation and shattering in the interstellar medium
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• Expected dust grain size distributions in galaxies detected by ALMA at $z>7$
• The role of dust destruction and dust growth in the evolution of the interstellar medium
• Wide-field CO isotopologue emission and the CO-to-H${}_2$ factor across the nearby spiral galaxy M101
• Modification of Dust Grain Structure by Sputtering
• Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
• Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?
• Beyond the Solar Circle $-$ Trends in Massive Star Formation Between the Inner and Outer Galaxy
• Chemo-dynamical simulations of dwarf galaxy evolution
• Exploring the relation between dust mass and galaxy properties using Dusty SAGE
• Dust Survival in Galactic Winds
• Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
• Models for the IR and submm SEDs of normal, starburst and active galaxies
• Chemical modelling of dust-gas chemistry within AGB outflows -- II. Effect of the dust-grain size distribution
• The 2175 Å dust feature in star-forming galaxies at $1.3\le z\le 1.8$: the dependence on stellar mass and specific star formation rate
• Sub-millimeter brightness of early star-forming galaxies
• Far-Ultraviolet and Far-Infrared Bivariate Luminosity Function of Galaxies: Complex Relation between Stellar and Dust Emission
• On the grain-size distribution of turbulent dust growth
• An Orientation Bias in Observations of Submillimetre Galaxies
• A Variant Stellar-to-nebular Dust Attenuation Ratio on Subgalactic and Galactic Scales
• Synthesized grain size distribution in the interstellar medium
• Dust grain size evolution in local galaxies: a comparison between observations and simulations
• Properties of dust in the detached shells around U Ant, DR Ser, and V644 Sco
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• Inhibited destruction of dust by supernova in a clumpy medium
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Dense molecular cloud cores as a source of micrometer-sized grains in galaxies
• Dust Dynamics in AGN Winds: A New Mechanism For Multiwavelength AGN Variability
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• Chemical evolution models: GRB host identification and cosmic dust predictions
• Radial transport of dust in spiral galaxies
• Spectral energy distributions of dust and PAHs based on the evolution of grain size distribution in galaxies
• From Dust to Nanodust: Resolving Circumstellar Dust from the Colliding-Wind Binary Wolf-Rayet (WR) 140
• Optical Observations of the Nearby Type Ia Supernova 2021hpr
• Chemically Consistent Evolutionary Models with Dust
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• The Optical Variability of SDSS Quasars from Multi-epoch Spectroscopy. III. A Sudden UV Cutoff in Quasar SDSS J2317+0005
• Chemical evolution of galaxies: emerging dust and the different gas phases in a new multiphase code
• Evolution of dust grain size distribution and grain porosity in galaxies
• $\text{Herschel}$ Photometric Observations of $\mathrm{L}\mathrm{ITTLE}$ $\mathrm{T}\mathrm{HINGS}$ Dwarf Galaxies
• The Slow Flow Model of Dust Efflux in Local Star-Forming Galaxies
• High-Resolution X-Ray Spectroscopy of Interstellar Iron Toward Cygnus X-1 and GX 339-4
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Can star cluster environment affect dust input from massive AGB stars?
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Dust Grain Growth at High Redshift: Starburst-driven CMB-Dark Supershells
• On the Origin of Dust in Galaxy Clusters at Low to Intermediate Redshift
• Observational signatures of the dust size evolution in isolated galaxy simulations
• Extinction in the Large Magellanic Cloud Bar around NGC1854, NGC1856, and NGC1858
• Effects of dust grain size distribution on the abundances of CO and H${}_2$ in galaxy evolution
• Dwarf Galaxies: Their Low Metallicity Interstellar Medium
• Cosmic evolution of grain size distribution in galaxies using the ${\nu }^2$GC semi-analytic model
• Dust Grain Growth & Dusty Supernovae in Low-Metallicity Molecular Clouds
• Modelling galaxy spectra in presence of interstellar dust-III. From nearby galaxies to the distant Universe
• Extinction law in ultraluminous infrared galaxies at z ~ 1
• Chemical evolution of galaxies with radiation-driven dust wind
• Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud
• Origin of optically passive spiral galaxies with dusty star-forming regions: Outside-in truncation of star formation?
• Stellar, Gas, and Dust Emission of Star Forming Galaxies out to z~2
• Photoelectric heating effects on the evolution of luminous disk galaxies
• A Bayesian chemical evolution model of the DustPedia Galaxy M74
• Submillimeter Observations of CLASH 2882 and the Evolution of Dust in this Galaxy
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Exploring the Dependence of Gas Cooling and Heating Functions on the Incident Radiation Field with Machine Learning
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Dust growth in molecular cloud envelopes: a numerical approach
• Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles
• The MOSDEF Survey: Probing Resolved Stellar Populations at $z\sim 2$ Using a New Bayesian-defined Morphology Metric Called Patchiness
• Using dust to constrain dark matter models
• The Role of Dust in Producing the Cosmic Infrared Background
• The Star Formation History of Redshift z~2 Galaxies: The Role of The Infrared Prior
• Relations between ISM tracers in galaxies
• The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
• Extragalactic globular cluster near-infrared spectroscopy: I. Integrated near-infrared spectra of Centaurus A/NGC 5128
• Quantitative Morphology of Galactic Cirrus in Deep Optical Imaging
• ISM dust feedback from low to high mass stars
• DESI Mg II Absorbers: Extinction Characteristics & Quasar Redshift Accuracy
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• What is the amount of baryonic dark matter in galaxies?
• The cosmic journey of dust grains -- from nucleation to planetary system
• Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
• Metal-strong Inflows at the Outer-galactic-scale of a Quasar
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Theoretical clues about dust accumulation and galaxy obscuration at high and low redshift
• Element mixing in the Cassiopeia A supernova
• A comparison of dust content and properties in GAMA/G10-COSMOS/3D-HST and SIMBA cosmological simulations
• The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope