Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation

Abstract

We implement a detailed dust model into the L-Galaxies semi-analytical model which includes: injection of dust by type II and type Ia supernovae (SNe) and AGB stars; grain growth in molecular clouds; and destruction due to supernova-induced shocks, star formation, and reheating. Our grain growth model follows the dust content in molecular clouds and the inter-cloud medium separately, and allows growth only on pre-existing dust grains. At early times, this can make a significant difference to the dust growth rate. Above $z\sim 8$, type II SNe are the primary source of dust, whereas below $z\sim 8$, grain growth in molecular clouds dominates, with the total dust content being dominated by the latter below $z\sim 6$. However, the detailed history of galaxy formation is important for determining the dust content of any individual galaxy. We introduce a fit to the dust-to-metal (DTM) ratio as a function of metallicity and age, which can be used to deduce the DTM ratio of galaxies at any redshift. At $z\lesssim 3$, we find a fairly flat mean relation between metallicity and the DTM, and a positive correlation between metallicity and the dust-to-gas (DTG) ratio, in good agreement with the shape and normalisation of the observed relations. We also match the normalisation of the observed stellar mass -- dust mass relation over the redshift range of $0-4$, and to the dust mass function at $z=0$. Our results are important in interpreting observations on the dust content of galaxies across cosmic time, particularly so at high redshift.

arXiv comment19 pages, 16 figures. Edits: Corrected equation 15 and its parameters. Accepted in MNRAS

References in corpus (86)

• The chemical composition of the Sun
• Galactic Stellar and Substellar Initial Mass Function
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
• Simulating Galaxy Formation with the IllustrisTNG Model
• Planck 2013 results. I. Overview of products and scientific results
• A luminous quasar at a redshift of z = 7.085
• A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
• Simba: Cosmological Simulations with Black Hole Growth and Feedback
• Semi-Analytic Modelling of Galaxy Formation: The Local Universe
• A model for cosmological simulations of galaxy formation physics
• A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium
• Resolving Cosmic Structure Formation with the Millennium-II Simulation
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
• New Interstellar Dust Models Consistent with Extinction, Emission, and Abundance Constraints
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• The Evolution of the Elemental Abundances in the Gas and Dust Phases of the Galaxy
• The Role of Pressure in GMC Formation II: The H_2 - Pressure Relation
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• An interferometric CO survey of luminous submm galaxies
• An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling
• Andromeda's Dust
• KINGFISH -- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel: Survey Description and Image Atlas
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• A dusty, normal galaxy in the epoch of reionization
• A deep ALMA image of the Hubble Ultra Deep Field
• Modelling the nebular emission from primeval to present-day star-forming galaxies
• Evolution of interstellar dust and stardust in the solar neighbourhood
• An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South: Source catalog and multiplicity
• The Herschel Reference Survey
• The evolution of the dust and gas content in galaxies
• Herschel Far-Infrared and Sub-millimeter Photometry for the KINGFISH Sample of Nearby Galaxies
• An Overview of the Dwarf Galaxy Survey
• Dust Formation In Early Galaxies
• The dust content of galaxies from z = 0 to z = 9
• Dusty, Radiation Pressure Dominated Photoionization. II. Multi-Wavelength Emission Line Diagnostics for Narrow Line Regions
• Non-Standard Grain Properties, Dark Gas Reservoir, and Extended Submillimeter Excess, Probed by Herschel in the Large Magellanic Cloud
• A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios
• Dust Spectral Energy Distributions of Nearby Galaxies: an Insight from the Herschel Reference Survey
• The Atomic-to-Molecular Transition in Galaxies. III. A New Method for Determining the Molecular Content of Primordial and Dusty Clouds
• Linking dust emission to fundamental properties in galaxies: The low-metallicity picture
• Detection of atomic carbon [CII] 158 micron and dust emission from a z=7.1 quasar host galaxy
• Are Dusty Galaxies Blue? Insights on UV Attenuation from Dust-Selected Galaxies
• Dust Formation in Milky Way-like Galaxies
• The dust mass in z > 6 normal star forming galaxies
• Simulating the dust content of galaxies: successes and failures
• The First Detections of the Extragalactic Background Light at 3000, 5500, and 8000A (I): Results
• DustPedia - A Definitive Study of Cosmic Dust in the Local Universe
• Galaxy Simulation with Dust Formation and Destruction
• Dust production 680-850 million years after the Big Bang
• Simulating galactic dust grain evolution on a moving mesh
• Modelling Element Abundances in Semi-analytic Models of Galaxy Formation
• Dust origin in late-type dwarf galaxies: ISM growth vs. type II supernovae
• Star Formation and Metallicity Gradients in Semi-analytic Models of Disk Galaxy Formation
• The SCUBA Local Universe Galaxy Survey - III. Dust along the Hubble sequence
• Cosmological simulation with dust formation and destruction
• Coevolution of dust, gas, and stars in galaxies - I. Spatial distributions and scaling-relations of dust and molecular hydrogen
• Interstellar Grains in Elliptical Galaxies: Grain Evolution
• Galactic chemical evolution in hierarchical formation models - I. Early-type galaxies in the local Universe
• Dust and star-formation properties of a complete sample of local galaxies drawn from the Planck Early Release Compact Source Catalogue
• Evolution of Dust-to-Metal Ratio in Galaxies
• Elemental Abundances in Milky Way-like Galaxies from a Hierarchical Galaxy Formation Model
• Evolution of the dust-to-metals ratio in high-redshift galaxies probed by GRB-DLAs
• Formation of Dust in the Ejecta of Type Ia Supernovae
• Depletion patterns and dust evolution in the ISM
• New constraints on dust emission and UV attenuation of z=6.5-7.5 galaxies from millimeter observations
• Dust in the Circumgalactic Medium of Low-Redshift Galaxies
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• Dust scaling relations in a cosmological simulation
• The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20--600 $\mu$m wavelengths
• Thermal and nonthermal dust sputtering in hydrodynamical simulations of the multiphase interstellar medium
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• The sudden appearance of dust in the early Universe
• A consistent model for both the HI and stellar mass functions of galaxies

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