The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies

Abstract

The recent decade has seen an exponential growth in spatially-resolved metallicity measurements in the interstellar medium (ISM) of galaxies. To first order, these measurements are characterised by the slope of the radial metallicity profile, known as the metallicity gradient. In this work, we model the relative role of star formation feedback, gas transport, cosmic gas accretion, and galactic winds in driving radial metallicity profiles and setting the mass-metallicity gradient relation (MZGR). We include a comprehensive treatment of these processes by including them as sources that supply mass, metals, and energy to marginally unstable galactic discs in pressure and energy balance. We show that both feedback and accretion that can drive turbulence and enhance metal-mixing via diffusion are crucial to reproduce the observed MZGR in local galaxies. Metal transport also contributes to setting metallicity profiles, but it is sensitive to the strength of radial gas flows in galaxies. While the mass loading of galactic winds is important to reproduce the mass metallicity relation (MZR), we find that metal mass loading is more important to reproducing the MZGR. Specifically, our model predicts preferential metal enrichment of galactic winds in low-mass galaxies. This conclusion is robust against our adopted scaling of the wind mass-loading factor, uncertainties in measured wind metallicities, and systematics due to metallicity calibrations. Overall, we find that at $z\sim 0$, galactic winds and metal transport are more important in setting metallicity gradients in low-mass galaxies whereas star formation feedback and gas accretion dominate setting metallicity gradients in massive galaxies.

arXiv comment21 pages (+ appendix), 11 figures, 4 tables. Accepted by MNRAS

References in corpus (303)

• SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
• Array Programming with NumPy
• Astropy: A Community Python Package for Astronomy
• Planck 2015 results. XIII. Cosmological parameters
• A Universal Density Profile from Hierarchical Clustering
• The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
• Star Formation in Galaxies Along the Hubble Sequence
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
• How Do Galaxies Get Their Gas?
• Simulating Galaxy Formation with the IllustrisTNG Model
• The Star Formation Efficiency in Nearby Galaxies: Measuring Where Gas Forms Stars Effectively
• The Star Formation Law in Nearby Galaxies on Sub-Kpc Scales
• [O III]/[N II] as an Abundance Indicator at High Redshift
• Galaxy Bimodality due to Cold Flows and Shock Heating
• Cold streams in early massive hot haloes as the main mode of galaxy formation
• First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
• Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
• Galactic Winds
• Metallicity Calibrations and the Mass-Metallicity Relation for Star-Forming Galaxies
• Galactic star formation and accretion histories from matching galaxies to dark matter haloes
• Physical Models of Galaxy Formation in a Cosmological Framework
• 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$
• CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation
• Concentrations of Dark Halos from their Assembly Histories
• FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation
• The Neutral Atomic Phases of the ISM in the Galaxy
• The Circumgalactic Medium
• Formation of Massive Galaxies at High Redshift: Cold Streams, Clumpy Disks and Compact Spheroids
• On the Maximum Luminosity of Galaxies and Their Central Black Holes: Feedback From Momentum-Driven Winds
• Starburst-driven Mass Loss from Dwarf Galaxies: Efficiency and Metal Ejection
• AMAZE. I. The evolution of the mass-metallicity relation at z>3
• Gas-regulation of galaxies: the evolution of the cosmic sSFR, the metallicity-mass-SFR relation and the stellar content of haloes
• Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing
• The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations
• The chemical make-up of the Sun: A 2020 vision
• Metallicities of 0.3<z<1.0 Galaxies in the GOODS-North Field
• De Re Metallica: The cosmic chemical evolution of galaxies
• Abundance Gradients and the Formation of the Milky Way
• Gusty, gaseous flows of FIRE: galactic winds in cosmological simulations with explicit stellar feedback
• PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions
• From rings to bulges: evidence for rapid secular galaxy evolution at z~2 from integral field spectroscopy in the SINS survey
• Combined CO & Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star Formation Rate and Stellar Mass
• The Impact of cold gas accretion above a mass floor on galaxy scaling relations
• The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7
• The Large, Oxygen-Rich Halos of Star-Forming Galaxies Are A Major Reservoir of Galactic Metals
• Dissipation in Compressible MHD Turbulence
• A Universal, Local Star Formation Law in Galactic Clouds, Nearby Galaxies, High-Redshift Disks, and Starbursts
• Understanding Galaxy Evolution through Emission Lines
• An Analytic Model for the Evolution of the Stellar, Gas, and Metal Content of Galaxies
• A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA
• The SAMI Galaxy Survey: instrument specification and target selection
• Kinetic Energy Decay Rates of Supersonic and Super-Alfvenic Turbulence in Star-Forming Clouds
• The Origin of the Galaxy Mass-Metallicity Relation and Implications for Galactic Outflows
• Accurate universal models for the mass accretion histories and concentrations of dark matter halos
• Cool Outflows in Galaxies and their Implications
• The Atomic to Molecular Transition in Galaxies. II: HI and H_2 Column Densities
• Rapid formation of exponential disks and bulges at high redshift from the dynamical evolution of clump cluster and chain galaxies
• The Evolution of the Star-forming Interstellar Medium across Cosmic Time
• The Science Performance of JWST as Characterized in Commissioning
• Energy Input and Mass Redistribution by Supernovae in the Interstellar Medium
• The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations
• A Constant Molecular Gas Depletion Time in Nearby Disk Galaxies
• Regulation of Star Formation Rates in Multiphase Galactic Disks: a Thermal/Dynamical Equilibrium Model
• Momentum Injection by Supernovae in the Interstellar Medium
• COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: II. The non-universality of the Molecular Gas Depletion Timescale
• Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift
• GASP I: Gas stripping phenomena in galaxies with MUSE
• Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven Turbulence
• Turbulent Heating in Galaxy Clusters Brightest in X-rays
• What is Driving the HI Velocity Dispersion?
• CMasher: Scientific colormaps for making accessible, informative and 'cmashing' plots
• A Unified Model for Galactic Discs: Star Formation, Turbulence Driving, and Mass Transport
• The Universal Relation of Galactic Chemical Evolution: The Origin of the Mass-Metallicity Relation
• New calibrations for abundance determinations in HII regions
• Four phases of angular-momentum buildup in high-z galaxies: from cosmic-web streams through an extended ring to disc and bulge
• SDSS IV MaNGA - Metallicity and nitrogen abundance gradients in local galaxies
• Toy Models for Galaxy Formation versus Simulations
• Accretion-Driven Turbulence as Universal Process: Galaxies, Molecular Clouds, and Protostellar Disks
• New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies
• New Strong Line Abundance Diagnostics for \HII Regions: Effects of $\kappa$-Distributed Electron Energies and New Atomic Data
• The Baryonic Assembly of Dark Matter Halos
• High-redshift clumpy discs and bulges in cosmological simulations
• The COS-Halos Survey: Metallicities in the Low-Redshift Circumgalactic Medium
• The density profile of equilibrium and non-equilibrium dark matter halos
• Cooling Radiation and the Lyman-alpha Luminosity of Forming Galaxies
• The MOSDEF Survey: The Evolution of the Mass-Metallicity Relation from $z=0$ to $z\sim 3.3$
• The Mass-Metallicity relation explored with CALIFA: I. Is there a dependence on the star formation rate?
• Physical properties of galactic winds using background quasars
• An Analytic Model of Angular Momentum Transport by Gravitational Torques: From Galaxies to Massive Black Holes
• An accurate physical model for halo concentrations
• The PHANGS-MUSE survey -- Probing the chemo-dynamical evolution of disc galaxies
• The Metallicity of Galaxy Disks: Infall versus Outflow
• Relativistic jet feedback III: feedback on gas disks
• Dissipation and Extra Light in Galactic Nuclei: IV. Evolution in the Scaling Relations of Spheroids
• Gas accretion as the origin of chemical abundance gradients in distant galaxies
• Accretion of gas onto nearby spiral galaxies
• The SINS/zC-SINF survey of z~2 galaxy kinematics: Outflow properties
• SDSS-IV MaNGA: The Impact of Diffuse Ionized Gas on Emission-line Ratios, Interpretation of Diagnostic Diagrams, and Gas Metallicity Measurements
• Galaxy Mergers and the Mass-Metallicity Relation: Evidence for Nuclear Metal Dilution and Flattened Gradients from Numerical Simulations
• How stellar feedback simultaneously regulates star formation and drives outflows
• The SINS/zC-SINF survey of z~2 galaxy kinematics: SINFONI adaptive optics-assisted data and kiloparsec-scale emission line properties
• Einstein Observatory evidence for the widespread baryon overdensity in clusters of galaxies,
• Spatially-Resolved Spectroscopic Properties of Low-Redshift Star-Forming Galaxies
• Metallicity gradients in local field star-forming galaxies: Insights on inflows, outflows, and the coevolution of gas, stars and metals
• The evolution of the mass-metallicity relation in IllustrisTNG
• Constraints on star-formation driven galaxy winds from the mass-metallicity relation at z=0
• Differential Rotation and Turbulence in Extended HI Disks
• The energy and momentum input of supernova explosions in structured and ionised molecular clouds
• The KMOS^3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6 - 2.7
• The life-time of galactic bars: central mass concentrations and gravity torques
• A Superbubble Feedback Model for Galaxy Simulations
• The cold interstellar medium of galaxies in the Local Universe
• Feedback-regulated star formation in molecular clouds and galactic discs
• High-redshift star formation in the ALMA era
• In-N-Out: the gas cycle from dwarfs to spiral galaxies
• Shape of the oxygen abundance profiles in CALIFA face-on spiral galaxies
• The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim 2.6$ to $z\sim 0.6$ with KMOS${}^{3D}$
• Metal flows of the circumgalactic medium, and the metal budget in galactic halos
• The Mass and Momentum Outflow Rates of Photoionized Galactic Outflows
• Modelling chemical abundance distributions for dwarf galaxies in the Local Group: the impact of turbulent metal diffusion
• Mapping metallicity variations across nearby galaxy disks
• Superbubbles in the Multiphase ISM and the Loading of Galactic Winds
• The Star Formation Law in Molecule-Poor Galaxies
• Unstable disks at high redshift: Evidence for smooth accretion in galaxy formation
• XMM-Newton Observations of the Perseus Cluster II: Evidence for Gas Motions in the Core
• The Physical Nature of Starburst-Driven Galactic Outflows
• When the Milky Way turned off the lights: APOGEE provides evidence of star formation quenching in our Galaxy
• Characterizing mass, momentum, energy and metal outflow rates of multi-phase galactic winds in the FIRE-2 cosmological simulations
• High-Redshift Star-Forming Galaxies: Angular Momentum and Baryon Fraction, Turbulent Pressure Effects and the Origin of Turbulence
• The KMOS^3D Survey: data release and final survey paper
• Mergers, AGN, and 'Normal' Galaxies: Contributions to the Distribution of Star Formation Rates and Infrared Luminosity Functions
• IZI: Inferring the Gas Phase Metallicity (Z) and Ionization Parameter (q) of Ionized Nebulae using Bayesian Statistics
• Balance among gravitational instability, star formation, and accretion determines the structure and evolution of disk galaxies
• How supernova explosions power galactic winds
• The shape of oxygen abundance profiles explored with MUSE: evidence for widespread deviations from single gradients
• Ultra Fast Outflows: Galaxy-Scale Active Galactic Nucleus Feedback
• MASSIV: Mass Assembly Survey with SINFONI in VVDS. III. Evidence for positive metallicity gradients in z~1.2 star-forming galaxies
• A simple and accurate approximation for the Q stability parameter in multi-component and realistically thick discs
• Metal-enriched galactic outflows shape the mass-metallicity relationship
• z~2: An Epoch of Disk Assembly
• A new scaling relation for HII regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation
• Galactic outflow rates in the EAGLE simulations
• Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): II. Cold Molecular Gas Evolution out to Redshift 6
• Enhanced Momentum Feedback from Clustered Supernovae
• Simulations of supermassive black hole growth in high-redshift disk galaxies
• On the Dynamics and Evolution of Gravitational Instability-Dominated Disks
• First results from SMAUG: Characterization of Multiphase Galactic Outflows from a Suite of Local Star-Forming Galactic Disk Simulations
• Stochastic modelling of star-formation histories II: star-formation variability from molecular clouds and gas inflow
• Evolving Gravitationally Unstable Disks Over Cosmic Time: Implications For Thick Disk Formation
• The Star Formation Rate in the Gravoturbulent Interstellar Medium
• Accretion-Driven Turbulence and the Transition to Global Instability in Young Galaxy Disks
• Simulating an Isolated Dwarf Galaxy with Multi-Channel Feedback and Chemical Yields from Individual Stars
• MusE GAs FLOw and Wind (MEGAFLOW) III: galactic wind properties using background quasars
• The equilibrium view on dust and metals in galaxies: Galactic outflows drive low dust-to-metal ratios in dwarf galaxies
• Vertical Equilibrium, Energetics, and Star Formation Rates in Magnetized Galactic Disks Regulated by Momentum Feedback from Supernovae
• Constructing Merger Trees that Mimic N-Body Simulations
• Do galaxy global relationships emerge from local ones? The SDSS IV MaNGA surface mass density-metallicity relation
• The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disk turbulence in z~0.9 star-forming galaxies
• Bar quenching in gas-rich galaxies
• Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal re-distribution
• Steady Outflows in Giant Clumps of High-z Disk Galaxies During Migration and Growth by Accretion
• Galactic Winds in Low-Mass Galaxies
• Kiloparsec Scale Properties of Star-Formation Driven Outflows at z~2.3 in the SINS/zC-SINF AO Survey
• Forming Super Star Clusters in the Central Starburst of NGC 253
• Star Formation and Metallicity Gradients in Semi-analytic Models of Disk Galaxy Formation
• GHASP : An Halpha kinematic survey of 203 spiral and irregular galaxies - VII. Revisiting the analysis of Halpha data cubes for 97 galaxies
• Saturated-State Turbulence and Structure from Thermal and Magnetorotational Instability in the ISM: Three-Dimensional Numerical Simulations
• On the origin of the fundamental metallicity relation and the scatter in galaxy scaling relations
• The KLEVER Survey: Spatially resolved metallicity maps and gradients in a sample of 1.2 < z < 2.5 lensed galaxies
• Gas-phase metallicity gradients of TNG50 star-forming galaxies
• Hot-mode accretion and the physics of thin-disk galaxy formation
• The SAMI Galaxy Survey: Spatially Resolved Metallicity and Ionization Mapping
• A deep X-ray observation of M82 with XMM-Newton
• HI and CO Velocity Dispersions in Nearby Galaxies
• Dissipation and Heating in Supersonic Hydrodynamic and MHD Turbulence
• Thermal-Instability-Driven Turbulent Mixing in Galactic Disks: I. Effective Mixing of Metals
• Why do high-redshift galaxies show diverse gas-phase metallicity gradients?
• Biases in metallicity measurements from global galaxy spectra: the effects of flux-weighting and diffuse ionized gas contamination
• The Chemical Evolution Carousel of Spiral Galaxies: Azimuthal Variations of Oxygen Abundance in NGC1365
• SDSS IV MaNGA -- Metallicity and ionisation parameter in local star-forming galaxies from Bayesian fitting to photoionisation models
• Metallicity Fluctuation Statistics in the Interstellar Medium and Young Stars. I. Variance and Correlation
• Gravitational torques in spiral galaxies: gas accretion as a driving mechanism of galactic evolution
• Sub-Eddington Star-Forming Regions are Super-Eddington: Momentum Driven Outflows from Supersonic Turbulence
• The momentum budget of clustered supernova feedback in a 3D, magnetised medium
• The effects of spatial resolution on Integral Field Spectrograph surveys at different redshifts. The CALIFA perspective
• Direct Detection of Black Hole-Driven Turbulence in the Centers of Galaxy Clusters
• Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies II: The Effects of Star Formation Feedback
• Temperature and Metallicity Gradients in the Hot Gas Outflows of M82
• Origin and Evolution of the Abundance Gradient along the Milky Way Disk
• Gravitational Runaway and Turbulence Driving in Star-Gas Galactic Disks
• New Perspective on Galaxy Outflows From the First Detection of Both Intrinsic and Traverse Metal-Line Absorption
• Radial motions and radial gas flows in local spiral galaxies
• The physics of gas phase metallicity gradients in galaxies
• CLASSY III: The Properties of Starburst-Driven Warm Ionized Outflows
• The EDGE-CALIFA survey: Variations in the Molecular Gas Depletion Time in Local Galaxies
• The Shapes of the HI Velocity Profiles of the THINGS Galaxies
• Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at $z$$\sim$2
• Cold Filamentary Accretion and the Formation of Metal Poor Globular Clusters and Halo Stars
• What controls the ionized gas turbulent motions in dwarf galaxies?
• From 'bathtub' galaxy evolution models to metallicity gradients
• Shaken, not blown: the gentle baryonic feedback of nearby starburst dwarf galaxies
• The Effects of Diffuse Ionized Gas and Spatial Resolution on Metallicity Gradients: TYPHOON Two-Dimensional Spectrophotometry of M83
• Accretion, radial flows and abundance gradients in spiral galaxies
• Measuring the mixing scale of the ISM within nearby spiral galaxies
• Evolution of the Milky Way with radial motions of stars and gas II. The evolution of abundance profiles from H to Ni
• Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
• Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
• Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies. I: The Case of Pure Self-Gravity
• The VLT SINFONI Mg ii Program for Line Emitters (SIMPLE) II: background quasars probing z $\sim$ 1 galactic winds
• Stellar and gaseous abundances in M82
• Radial gas motions in The HI Nearby Galaxy Survey (THINGS)
• The oxygen abundance gradients in the gas discs of galaxies in the EAGLE simulation
• The effect of differential galactic winds on the chemical evolution of galaxies
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• Gas infall and radial transport in cosmological simulations of Milky Way-mass disks
• On the effect of cosmological inflow on turbulence and instability in galactic discs
• 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
• How to get cool in the heat: comparing analytic models of hot, cold, and cooling gas in haloes and galaxies with EAGLE
• The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
• Diffuse ionized gas and its effects on nebular metallicity estimates of star-forming galaxies
• SDSS-IV MaNGA: Modelling the metallicity gradients of gas and stars - radially dependent metal outflow vs IMF
• Systematic difference between ionized and molecular gas velocity dispersion in $z\sim 1-2$ disks and local analogues
• L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
• Early results from GLASS-JWST. IV: Spatially resolved metallicity in a low-mass $z\sim 3$ galaxy with NIRISS
• Mixing and transport of metals by gravitational instability-driven turbulence in galactic discs
• The metallicity's fundamental dependence on both local and global galactic quantities
• Effects of Galactic fountains and delayed mixing in the chemical evolution of the Milky Way
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Azimuthal variations of gas-phase oxygen abundance in NGC 2997
• Swirls of FIRE: Spatially Resolved Gas Velocity Dispersions and Star Formation Rates in FIRE-2 Disk Environments
• The role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• The gas metallicity gradient and the star formation activity of disc galaxies
• The JCMT Nearby Galaxies Legacy Survey IV. Velocity Dispersions in the Molecular Interstellar Medium in Spiral Galaxies
• How Do Supernovae Impact the Circumgalactic Medium? I. Large-Scale Fountains Around a Milky Way-Like Galaxy
• Metal Mixing and Ejection in Dwarf Galaxies is Dependent on Nucleosynthetic Source
• Alfvenic Turbulence Beyond the Ambipolar Diffusion Scale
• Jets blowing bubbles in the young radio galaxy 4C 31.04
• On the origin of the mass-metallicity gradient relation in the local Universe
• ALMA hints at the presence of turbulent disk galaxies at z > 5
• Accretion Does Not Drive the Turbulence in Galactic Disks
• Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
• The evolution of turbulent galactic discs: gravitational instability, feedback and accretion
• The SAMI Galaxy Survey: Gas velocity dispersions in low-$z$ star-forming galaxies and the drivers of turbulence
• The Relationship Between Galaxy ISM and Circumgalactic Gas Metallicities
• Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
• Kinematics and Dynamics of Multiphase Outflows in Simulations of the Star-Forming Galactic ISM
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• The DUVET Survey: Direct $T_e$-based metallicity mapping of metal-enriched outflows and metal-poor inflows in Mrk 1486
• Bursting Bubbles: Feedback from Clustered SNe and the Trade-off Between Turbulence and Outflows
• Ly$\alpha$ Blobs from Cold Streams Undergoing Kelvin-Helmholtz Instabilities
• GASP and MaNGA surveys shed light on the enigma of the gas metallicity gradients in disk galaxies
• The role of gas infall in the evolution of disc galaxies
• What drives the velocity dispersion of ionized gas in star-forming galaxies?
• Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods
• The Effects of radial inflow of gas and galactic fountains on the chemical evolution of M31
• Dust depletion of metals from local to distant galaxies I: Peculiar nucleosynthesis effects and grain growth in the ISM
• The metallicity of galactic winds
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• The Origin of Interstellar Turbulence in M33
• The global structure of magnetic fields and gas in simulated Milky Way-analogue galaxies
• X-ray Properties of NGC 253's Starburst-Driven Outflow
• The Origin of Exponential Star-forming Disks
• Delayed star formation in high-redshift stream-fed galaxies
• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• Testing Star Formation Laws on Spatially Resolved Regions in a $z\approx 4.3$ Starburst Galaxy
• Filaments and striations: anisotropies in observed, supersonic, highly-magnetised turbulent clouds
• Bar effect on gas-phase abundance gradients. II. Luminosity-dependent flattening
• The Gas-phase Metallicity Profiles of Star-forming Galaxies in the Modified Accretion Disk Framework
• Quantifying the effects of spatial resolution and noise on galaxy metallicity gradients
• The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
• Metallicity Gradient of Barred Galaxies with TYPHOON
• Gas Accretion Can Drive Turbulence in Galaxies
• Turbulent mixing of r-process elements in the Milky Way
• The physical drivers of gas turbulence in simulated disc galaxies
• A geostatistical analysis of multiscale metallicity variations in galaxies [I]: Introduction and comparison of high-resolution metallicity maps to an analytic metal transport model
• Resolved gas kinematics in a sample of low-redshift high star-formation rate galaxies
• The Evolution of Gas-Phase Metallicity and Resolved Abundances in Star-forming Galaxies at $z\approx 0.6-1.8$
• Spatially Resolved Metal Loss from M31
• Spiral Arms are Metal Freeways: Azimuthal Gas-Phase Metallicity Variations in Simulated Cosmological Zoom-in Flocculent Disks
• Accretion driven turbulence in filaments II: Effects of self-gravity
• Detection of metallicity correlations in 100 nearby galaxies
• Scaling relations and baryonic cycling in local star-forming galaxies. III. Outflows, effective yields and metal loading factors
• Spatial metallicity distribution statistics at $\lesssim 100$ pc scales in the AMUSING++ nearby galaxy sample
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• Extreme Variation in Star Formation Efficiency Across a Compact, Starbursting Disk Galaxy
• How well do local relations predict gas-phase metallicity gradients? Results from SDSS-IV MaNGA
• The role of gas kinematics in setting metallicity gradients at high redshift
• The major mechanism to drive turbulence in star-forming galaxies
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• Multifluid magnetohydrodynamic turbulent decay
• SDSS-IV MaNGA: the chemical co-evolution of gas and stars in spiral galaxies
• Non-ideal MHD turbulent decay in molecular clouds
• Reconstructing three-dimensional densities from two-dimensional observations of molecular gas
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
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• Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
• The circum-galactic gas around cosmologically simulated disks
• Gas accretion onto galaxies and Kelvin-Helmholtz turbulence

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