The dust content of galaxies from z = 0 to z = 9

Abstract

We study the dust content of galaxies from $z=0$ to $z=9$ in semi-analytic models of galaxy formation that include new recipes to track the production and destruction of dust. We include condensation of dust in stellar ejecta, the growth of dust in the interstellar medium (ISM), the destruction of dust by supernovae and in the hot halo, and dusty winds and inflows. The rate of dust growth in the ISM depends on the metallicity and density of molecular clouds. Our fiducial model reproduces the relation between dust mass and stellar mass from $z=0$ to $z=7$, the number density of galaxies with dust masses less than $10^{8.3}{\mathrm{M}}_{\odot }$, and the cosmic density of dust at $z=0$. The model accounts for the double power-law trend between dust-to-gas (DTG) ratio and gas-phase metallicity of local galaxies and the relation between DTG ratio and stellar mass. The dominant mode of dust formation is dust growth in the ISM, except for galaxies with $M_{\ast }<10^7{\mathrm{M}}_{\odot }$, where condensation of dust in supernova ejecta dominates. The dust-to-metal ratio of galaxies depends on the gas-phase metallicity, unlike what is typically assumed in cosmological simulations. Model variants including higher condensation efficiencies, a fixed timescale for dust growth in the ISM, or no growth at all reproduce some of the observed constraints, but fail to simultaneously reproduce the shape of dust scaling relations and the dust mass of high-redshift galaxies.

arXiv commentAccepted for publication in MNRAS

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• The impact of carbon and oxygen abundances on the metal-poor initial mass function
• Starduster: A multi-wavelength SED model based on radiative transfer simulations and deep learning
• Effects of dust evolution on the abundances of CO and H${}_2$
• Systematic errors in dust mass determinations: Insights from laboratory opacity measurements
• AzTEC Survey of the Central Molecular Zone: Increasing Spectral Index of Dust with Density
• Molecular gas and dust properties in $z>7$ quasar hosts
• Dust grain size evolution in local galaxies: a comparison between observations and simulations
• The efficiency of grain growth in the diffuse interstellar medium
• A Universal Relation of Dust Obscuration Across Cosmic Time
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• The slippery slope of dust attenuation curves: Correlation of dust attenuation laws with star-to-dust compactness up to z = 4
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• A${}^3$COSMOS: the dust mass function and dust mass density at $0.5<z<6$
• Radiative transfer of ionizing radiation through gas and dust: grain charging in star forming regions
• Missing dust signature in the cosmic microwave background
• Decoding the IRX-β dust attenuation relation in star-forming galaxies at intermediate redshift
• Cosmic evolution of grain size distribution in galaxies using the ${\nu }^2$GC semi-analytic model
• On the Origin of Dust in Galaxy Clusters at Low to Intermediate Redshift
• A simple numerical experiment on the dust temperature bias for Lyman break galaxies at $z\gtrsim 5$
• ALPINE: A Large Survey to Understand Teenage Galaxies
• CEERS: Forging the First Dust Grains in the Universe? A Population of Galaxies with spectroscopically-derived Extremely Low Dust Attenuation (GELDA) at 4.0<z<11.4
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• A Bayesian chemical evolution model of the DustPedia Galaxy M74
• Dust emission from the bulk of galaxies at the Epoch of Reionization
• Euclid preparation. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
• Hierarchical Bayesian inference of the Initial Mass Function in Composite Stellar Populations
• Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at $z\sim 2.1-3.6$
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Dust Evolution in Simulated Multiphase Galactic Outflows
• FLORAH: A generative model for halo assembly histories
• The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
• ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
• Dust contribution to the panchromatic galaxy emission
• HELM's deep: Highly Extincted Low-Mass galaxies seen by JWST
• Challenges and Techniques for Simulating Line Emission
• Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• The ALMA View of High-Redshift Galaxy Formation
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory