Galactic chemical evolution: Carbon through Zinc

Abstract

We calculate the evolution of heavy element abundances from C to Zn in the solar neighborhood adopting our new nucleosynthesis yields. Our yields are calculated for wide ranges of metallicity (Z=0-Z_\odot) and the explosion energy (normal supernovae and hypernovae), based on the light curve and spectra fitting of individual supernovae. The elemental abundance ratios are in good agreement with observations. Among the alpha-elements, O, Mg, Si, S, and Ca show a plateau at [Fe/H] < -1, while Ti is underabundant overall. The observed abundance of Zn ([Zn/Fe] ~ 0) can be explained only by the high energy explosion models, which requires a large contribution of hypernovae. The observed decrease in the odd-Z elements (Na, Al, and Cu) toward low [Fe/H] is reproduced by the metallicity effect on nucleosynthesis. The iron-peak elements (Cr, Mn, Co, and Ni) are consistent with the observed mean values at -2.5 < [Fe/H] < -1$, and the observed trend at the lower metallicity can be explained by the energy effect. We also show the abundance ratios and the metallicity distribution functions of the Galactic bulge, halo, and thick disk. Our results suggest that the formation timescale of the thick disk is ~ 1-3 Gyr.

50pages, 33figures, Accepted for publication in ApJ

References in corpus (65)

• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• The Geneva-Copenhagen survey of the Solar neighbourhood: Ages, metallicities, and kinematic properties of 14,000 F and G dwarfs
• Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation
• First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
• The Chemical Evolution of the Galaxy: the two-infall model
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• Galactic Evolution of Sr, Y, Zr: A Multiplicity of Nucleosynthetic Processes
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• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• APOGEE chemical tagging constraint on the maximum star cluster mass in the $\alpha$-enhanced Galactic disk
• Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• Oxygen and zinc abundances in 417 Galactic bulge red giants
• Correlations of r-Process Elements in Very Metal-Poor Stars as Clues to their Nucleosynthesis Sites
• Constraining The Single-Degenerate Channel of Type Ia Supernovae With Stable Iron-Group Elements in SNR 3C 397
• The R-Process Alliance: Chemo-Dynamically Tagged Groups II. An Extended Sample of Halo $r$-Process-Enhanced Stars
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• The IGIMF and other IMFs in dSphs: the case of Sagittarius
• Chemical Compositions of Evolved Stars From Near-Infrared IGRINS High-Resolution Spectra. I. Abundances in Three Red Horizontal Branch Stars
• Perspectives on Intracluster Enrichment and the Stellar Initial Mass Function in Elliptical Galaxies
• Galactic Chemical Evolution and the Oxygen Isotopic Composition of the Solar System
• Phosphorus Abundances in FGK Stars
• Sulfur and zinc abundances of red giant stars
• Nothing to see here: Failed supernovae are faint or rare
• The Galactic Chemical Evolution of phosphorus observed with IGRINS
• Chemical evolution of the Galactic Center
• ZFIRE: Using H$\alpha$ equivalent widths to investigate the in situ initial mass function at z~2
• Neutron-capture elements in dwarf galaxies II: Challenges for the s- and i-processes at low metallicity
• Nucleosynthesis Constraints on the Energy Growth Timescale of a Core-collapse Supernova Explosion
• Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. V. The Zn-Enhanced Metal-Poor Star BS 16920-017
• Modelling the chemical evolution of the Galaxy halo
• Machine learning detects multiplicity of the first stars in stellar archaeology data
• Metal enrichment and evolution in four z > 6.5 quasar sightlines observed with JWST/NIRSpec
• Unusual neutron-capture nucleosynthesis in a carbon-rich Galactic bulge star
• Are ancient dwarf satellites the building blocks of the Galactic halo?
• Mono-enriched stars and Galactic chemical evolution -- Possible biases in observations and theory
• The CARMENES search for exoplanets around M dwarfs: Not-so-fine hyperfine-split vanadium lines in cool star spectra
• Evidence of Early Enrichment of the Galactic Disk by Large-Scale Winds
• nu-Process Nucleosynthesis in Population III Core-Collapse Supernovae
• Cosmological evolution of the Nitrogen abundance
• Chemical Signature Indicating A Lack of Massive Stars in Dwarf Galaxies
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Mapping radial abundance gradients with Gaia-ESO open clusters: Evidence of recent gas accretion in the Milky Way disk
• NLTE analysis of copper lines in different stellar populations
• Chlorine-bearing molecules in molecular absorbers at intermediate redshifts
• The energy distribution of the first supernovae
• Massive Stars and their Supernovae
• Tests of model predictions for the response of stellar spectra and absorption line indices to element abundance variations
• The nature of NV absorbers at high redshift
• The contribution from rotating massive stars to the enrichment in Sr and Ba of the Milky Way
• Detailed Iron-Peak Element Abundances in Three Very Metal-Poor Stars
• Enrichment of Strontium in Dwarf Galaxies
• 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
• A Model for Clumpy Self-Enrichment in Globular Clusters
• The Hamburg/ESO R-process Enhanced Star survey (HERES) VI. The Galactic Chemical Evolution of Silicon
• Extreme r-process enhanced stars at high metallicity in Fornax
• Galactic chemical evolution of exoplanet host stars: Are high-mass planetary systems young?
• Neutron Star Mergers as the Main Source of R-process: Natal Kicks And Inside-Out Evolution to The Rescue
• Chemical abundances in a high velocity RR Lyrae star near the bulge
• On the origin of the helium-rich population in Omega Centauri
• The Abundance Pattern in the Hot ISM of NGC 4472: Insights and Anomalies
• Ancient Very Metal-Poor Stars Associated With the Galactic Disk in the H3 Survey
• Manganese spread in Ursa Minor as a proof of sub-classes of type Ia supernovae
• In pursuit of giants: II. Evolution of dusty quiescent galaxies over the last six billion years from the hCOSMOS survey
• Metallicity-Dependent Galactic Isotopic Decomposition for Nucleosynthesis
• The Cosmic Evolution of Magnesium Isotopes
• The Chemical Nature of the Young 120-Myr-old Nearby Pisces-Eridanus Stellar Stream Flowing through the Galactic Disk
• BAL Outflow Contribution to AGN Feedback: Frequency of S iv Outflows in the SDSS
• X-Shooting ULLYSES: Massive Stars at low metallicity II. DR1: Advanced optical data products for the Magellanic Clouds
• The Most Metal-poor Stars in the Inner Bulge
• Nitrogen abundance in the X-ray halos of clusters and groups of galaxies
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• MINCE I. Presentation of the project and of the first year sample
• The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
• The chemical connection between damped Lyman-α systems and Local Group dwarf galaxies
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
• Are Faint Supernovae Responsible for Carbon-Enhanced Metal-Poor Stars?
• A Local Leaky-box Model for the Local Stellar Surface Density - Gas Surface Density - Gas Phase Metallicity Relation
• Large proper motion of the Thorne-Żytkow object candidate HV 2112 reveals its likely nature as foreground Galactic S-star
• Abundance analysis of a CEMP-no star in the Carina dwarf spheroidal galaxy
• Keck and VLT Observations of Super-damped Lyman-alpha Absorbers at z=2=2.5: Constraints on Chemical Compositions and Physical Conditions
• The most metal-rich stars in the universe: chemical contributions of low and intermediate mass asymptotic giant branch stars with metallicities between $0.04\le Z\le \mathrm{0.10.}$
• Chemical abundances in the metal-intermediate GC NGC 6723
• Mining S-PLUS for Metal-Poor Stars in the Milky Way
• Suzaku Observation of the Diffuse X-Ray Emission from the Open Cluster Westerlund 2: a Hypernova Remnant?
• Investigation of the Puzzling Abundance Pattern in the Stars of the Fornax Dwarf Spheroidal Galaxy
• Sulphur abundances in halo giants from the [S I] line at 1082 nm and the S I triplet around 1045 nm
• Galaxy Ecosystems: gas contents, inflows and outflows
• Phosphorus Abundances in the Hyades and Galactic Disk
• Population III stars around the Milky Way
• Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties
• Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties
• Origin of metals in old Milky Way halo stars based on GALAH and Gaia
• Discovery of Shocked Molecular Clouds Associated with the Shell-Type Supernova Remnant RX J0046.5$-$7308 in the Small Magellanic Cloud
• Inhomogeneous enrichment of radioactive nuclei in the Galaxy: Deposition of live Mn-53, Fe-60, Hf-182, and Pu-244 into deep-sea archives. Surfing the wave?
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• Gas-phase Fe/O and Fe/N abundances in Star-Forming Regions. Relations between nucleosynthesis, metallicity and dust
• Heavy element evolution in the inner regions of the Milky Way
• Early chemical evolution of Zn driven by magnetorotational supernovae and the pathway to the solar Zn composition
• Dust evolution processes constrained by extinction curves in nearby galaxies
• Is the metallicity of their hosts a good measure of the metallicity of Type Ia supernovae?
• Chemical Evolution of Fluorine in the Milky Way
• Fates of the oldest intermediate-mass stars - Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors
• Spatially Resolved Chandra Spectroscopy of the Large Magellanic Cloud Supernova Remnant N132D
• Abundance analysis of SDSS J134338.67+484426.6; an extremely metal-poor star from the MARVELS pre-survey
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• Exploring the Carbon Simmering Phase: Reaction Rates, Mixing, and the Convective Urca Process
• Detection of Al II in the Ultraviolet Spectra of Metal-Poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
• What is the Milky Way outer halo made of? High resolution spectroscopy of distant red giants
• Evidence of Pop~III stars' chemical signature in neutral gas at z~6. A study based on the E-XQR-30 spectroscopic sample
• The extreme CNO-enhanced composition of the primitive iron-poor dwarf star J0815+4729
• NGC 1261: an $r$-process enhanced globular cluster from the Gaia-Enceladus event
• Isotopic Titanium Abundances in Local M Dwarfs
• Abundance ratios in the hot ISM of elliptical galaxies
• Analytic solution of Chemical Evolution Models with Type Ia SNe
• Abundances of the light elements from UV (HST) and red (ESO) spectra in the very old star HD 84937
• A data-driven model of nucleosynthesis with chemical tagging in a lower-dimensional latent space
• Nucleosynthesis in Primordial Hypernovae
• Empirically Derived Integrated Stellar Yields of Fe-Peak Elements
• Peeking beneath the precision floor I: metallicity spreads and multiple elemental dispersions in the globular clusters NGC 288 and NGC 362
• Are oxygen and neon enriched in PNe and is the current solar Ne/O abundance ratio underestimated?
• $Chempy$: A flexible chemical evolution model for abundance fitting - Do the Sun's abundances alone constrain chemical evolution models?
• The impact of black hole seeding in cosmological simulations
• Metallicities in the Outer Regions of Spiral Galaxies
• Keck HIRES Spectroscopy of SkyMapper Commissioning Survey Candidate Extremely Metal-Poor Stars
• The metal-poor end of the Spite plateau. II. Detailed chemical investigation
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• The [Y/Mg] chemical clock in the Galactic Disk: The influence of metallicity and Galactic population in the solar neighbourhood
• Chlorine Abundances in Cool Stars
• Chlorine Isotope Ratios in M Giants
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• Expanding space, quasars and St. Augustine's fireworks
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• Testing Feedback from Star Clusters in Simulations of the Milky Way Formation
• Inhomogeneous Galactic Chemical Evolution: Modelling Ultra-Faint Dwarf Galaxies of the Large Magellanic Cloud
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• Nucleosynthetic yields of Z=$10^{-5}$ intermediate-mass stars
• Chemo-dynamical simulations of dwarf galaxy evolution
• The Evolution Of Carbon, Sulphur, and Titanium Isotopes from High-Redshift to the Local Universe
• Star Formation and Gas Phase History of the Cosmic Web
• ColdSIM predictions of [C II] emission in primordial galaxies
• Galactic Constraints on Supernova Progenitor Models
• A new algorithm for optimizing the wavelength coverage for spectroscopic studies: Spectral Wavelength Optimization Code (SWOC)
• IR characteristic emission and dust properties of star-forming galaxies at 4.5 $<$ z $<$ 6.2
• On the [$\alpha$/Fe]-[Fe/H] relations in early-type galaxies
• Composite Stellar Populations and Element by Element Abundances in the Milky Way Bulge and Elliptical Galaxies
• Neutron Star Planets: Atmospheric processes and habitability
• Time evolution of Ce as traced by APOGEE using giant stars observed with the Kepler, TESS and K2 missions
• Ages of 70 dwarfs of three populations in the solar neighborhood: considering O and C abundances in stellar models
• Neutrino-dominated accretion flows: second nucleosynthesis factory in core-collapse supernovae and regulation of iron markets in galaxies
• Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• Modeling and Analysis of a Spectrum of the Globular Cluster NGC 2419
• Uniform Silicon Isotope Ratios Across the Milky Way Galaxy
• Supernova-driven turbulent metal mixing in high redshift galactic disks: metallicity fluctuations in the interstellar medium and its imprints on metal poor stars in the Milky Way
• Chemical analysis of eight giant stars of the globular cluster NGC 6366
• An In-Depth Study of the Abundance Pattern in the Hot Interstellar Medium in NGC 4649
• Testing the Universality of the Stellar IMF with Chandra and HST
• Chemical Abundances in the Globular Clusters NGC 6229 and NGC 6779
• The Pristine Inner Galaxy Survey (PIGS) X. Probing the early chemical evolution of the Sagittarius dwarf galaxy with carbon abundances
• Cobalt and copper abundances in 56 Galactic bulge red giants
• On the Hunt for the Origins of the Orphan--Chenab Stream: Detailed Element Abundances with APOGEE and Gaia
• Chemical evolution of ultra-faint dwarf galaxies: testing the IGIMF
• The Chemical Evolution of Iron-Peak Elements with Hypernovae
• An outer shade of Pal: Abundance analysis of the outer halo globular cluster Palomar 13
• Using heritability of stellar chemistry to reveal the history of the Milky Way
• Neutron-capture elements in dwarf galaxies III: A homogenized analysis of 13 dwarf spheroidal and ultra-faint galaxies
• The formation of the Milky Way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum II, and Coma Berenices UFDs
• Modeling Increased Metal Production in Galaxy Clusters with Pair-Instability Supernovae
• The earliest phases of CNO enrichment in galaxies
• Clustering in the Stellar Abundances Space
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• The Pristine Inner Galaxy Survey (PIGS) IX. The largest detailed chemical analysis of very metal-poor stars in the Sagittarius dwarf galaxy
• Outside-in stellar formation in the spiral galaxy M33?
• From Galactic Chemical Evolution to Cosmic Supernova Rates Synchronized with Core-Collapse Supernovae Limited to the Narrow Progenitor Mass Range
• r-Process enrichment in the Galactic halo characterized by nucleosynthesis variation in the ejecta of coalescing neutron star binaries
• Study of the element abundances in HD 140283: the abundance robustness of the weak r- and main r-process 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
• Unveiling the chemical fingerprint of phosphorus-rich stars I. In the infrared region of APOGEE-2
• NLTE Analysis of Copper Abundances in the Galactic Bulge Stars
• G112-43/44: A metal-poor binary star with a unique chemical composition and kinematics like the Helmi streams
• Is Germanium (Ge, Z=32) A Neutron-Capture Element?
• A Monte Carlo based simulation of the galactic chemical evolution of the Milky Way galaxy
• Elemental Abundances of the Hot Atmosphere of Luminous Infrared Galaxy Arp 299
• The Chemical Evolution of Globular Clusters - II. Metals and Fluorine
• Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
• Metal Enrichment in the Fermi Bubbles as a Probe of Their Origin
• Stellar ($n,\gamma$) cross section of ${}^{23}$Na
• Sulphur in the metal poor globular cluster NGC 6397
• Extremely Metal-Poor Stars and a Hierarchical Chemical Evolution Model
• A new formation model for omega Centauri: the crossroad of astrophysical processes
• Traits for chemical evolution in solar twins: Trends of neutron-capture elements with stellar age
• A formation timescale of the Galactic halo from Mg isotopes in dwarf stars
• HII Region Metallicity Constraints Near the Site of the Strongly Lensed Supernova "SN Refsdal" at Redshift 1.49
• Empirical Constraints on Core Collapse Supernova Yields using Very Metal Poor Damped Lyman Alpha Absorbers
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• North Polar Spur: gaseous plume(s) from star-forming regions at $\sim$3-5 kpc from Galactic Center?
• X-ray Properties of Young Early Type Galaxies: II. Abundance Ratio in the Hot ISM
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Evolution of radioactive elements in the LMC: predictions for future gamma-ray surveys
• CD -24_17504 revisited: a new comprehensive element abundance analysis
• Detailed Chemical Abundances of Star Clusters in the Large Magellanic Cloud
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages
• A Systematic Study of Evolved Supernova Remnants in the Large and Small Magellanic Clouds with Suzaku
• The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories
• Heterogeneous evolution of the galaxy and the origin of the short-lived nuclides in the early solar system
• LOTUS: A (non-)LTE Optimization Tool for Uniform derivation of Stellar atmospheric parameters
• Galaxy Formation and Symbiotic Evolution with the Inter-Galactic Medium in the Age of ELT-ANDES
• Measuring Dwarf Galaxy Intrinsic Abundance Scatter with Mid-resolution Spectroscopic Surveys: Calibrating APOGEE Abundance Errors
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Aeos: Transport of Metals from Minihalos following Population III Stellar Feedback
• Modelling the composition of a young star cluster ejecta
• A new model for the origin of very metal poor stars and their chemical composition
• Optical and NIR spectroscopy of cool CEMP stars to probe the nucleosynthesis in low mass AGB binary system
• First Evidence of Globular Cluster Formation from the Ejecta of Prompt Type Ia Supernovae
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• A two-phase model of galaxy formation: III. The formation of globular clusters
• Initial Mass Function Variation in two Elliptical Galaxies using Near-Infrared Tracers
• Chemical abundances of the metal-poor horizontal-branch stars CS 22186-005 and CS 30344-033
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• Using chemical evolution models of the Milky Way disk to constrain Type Ia supernova progenitors
• Nitrogen Abundance Distribution in the inner Milky Way
• Analysis of integrated-light spectra of Galactic globular clusters
• A Galactic Self-Portrait: Density Structure and Integrated Properties of the Milky Way Disk
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
• Chemical composition of the outer halo globular cluster Palomar 15
• Study of the abundance features of the metal-poor star HD 94028
• Transition Elements in Supernova Presolar Grains: Condensation vs. Implantation
• Constraints on $R$-process Nucleosynthesis from ${}^{129}$I and ${}^{247}$Cm in the Early Solar System
• Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant
• Be, V and Cu in the halo star CS 31082-001 from near-UV spectroscopy
• Explosive Nucleosynthesis: What we learned and what we still do not understand
• The Impact of Inelastic Collisions with Hydrogen on NLTE Copper Abundances in Metal-Poor Stars
• High-resolution spectroscopic study of dwarf stars in the northern sky: Na to Zn abundances in two fields with radii of 20 degrees
• The origin of elements: the need for UV spectra
• Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
• Survey for Distant Solar Twins (SDST) -- III. Identification of new solar twin and solar analogue stars
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Abundance of zinc in the red giants of Galactic globular cluster 47 Tucanae
• The Origin of the Metal-Poor Common Proper Motion Pair HD 134439/134440: Insights from New Elemental Abundances
• Assessing stellar yields in Galaxy chemical evolution: observational stellar abundance patterns
• Binary stellar evolution yields in galactic chemical evolution calculations
• Kinematical & Chemical Characteristics of the Thin and Thick Disks
• Impacts of Black-Hole-Forming Supernova Explosions on the Diffuse Neutrino Background
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• CANGAROO-III observation of TeV gamma rays from the unidentified gamma-ray source HESS J1614-518
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• Puzzling radial gradients of K-band absorption features in the giant elliptical galaxy M87
• A chemical close-up of the main body of the Sagittarius dwarf galaxy
• Chemical tagging with APOGEE, MUSE, and HST: constraints on the formation of $\omega$ Centauri
• The Missing Link: Testing Galactic Chemical Evolution Models with the First Multi-Isotopic Abundances in Solar Twin Stars
• The impact of cosmic ray feedback during the epoch of reionisation
• The dawn is quiet here: Rise in [$\alpha$/Fe] is a signature of massive gas accretion that fueled proto-Milky Way
• J01020100-7122208: an accreted evolved blue straggler that wasn't ejected from a supermassive black hole
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Silicon and iron dust in gamma-ray burst host galaxy absorbers
• Chemical abundances of field halo stars -- Implications for the building blocks of the Milky Way
• The Near-Infrared Spectrum of the Nuclear Star Cluster: Looking Below the Tip of the Iceberg and Comparisons with Extragalactic Nuclei
• The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates
• Main-sequence Turnoff Stars as Probes of the Ancient Galactic Relic: Chemo-dynamical Analysis of a Pilot Sample
• Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
• Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations
• Estimating Ejecta Mass Ratios in Kepler's SNR: Global X-Ray Spectral Analysis Including Suzaku Systematics and Emitting Volume Uncertainties
• The LEGARE Project. I. Chemical evolution model of the Nuclear Stellar Disc in a Bayesian framework
• Complexity in small-scale dwarf spheroidal galaxies
• The metal-poorest tail of the Galactic halo: hypothesis on its origin from precise spectral analysis
• Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
• Modelling the chemical evolution of the Milky Way
• Fe-peak element abundances in disk and halo stars
• On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster
• Metallicity and kinematical clues to the formation of the Local Group
• A theoretical investigation of far-infrared fine structure lines at $z>6$ and of the origin of the [OIII]88/[CII]158 enhancement
• Observing Double White Dwarfs with the Lunar GW Antenna
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• Distribution of Europium in The Milky Way Disk; Its Connection to Planetary Habitability and The Source of The R-Process
• Heavy Elements -- They came out of the blue
• Proton-rich production of lanthanides: the $\nu i$ process
• Study of Integrated Spectra of Four Globular Clusters in M31
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• The assembly history of NGC 1365 through chemical archaeology
• Neutron-capture elements record the ordered chemical evolution of the disc over time
• Purveyors of fine halos III. Chemical abundance analysis of a potential omega Cen associate
• Evaluating star formation rates at z = 5
• A Census of Sun's Ancestors and their Contributions to the Solar System Chemical Composition
• Globular Cluster Abundances and What They Can Tell Us About Galaxy Formation
• A relic from a past merger event in the Large Magellanic Cloud
• Chemical abundances in Seyfert galaxies -- VII. Direct abundance determination of neon based on optical and infrared emission lines
• The COMBS Survey -- III. The Chemodynamical Origins of Metal-Poor Bulge Stars
• Downsizing revised: Star formation timescales for elliptical galaxies with an environment-dependent IMF and number of SNIa
• Viability of novae as sources of Galactic lithium
• Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates
• Origin and evolution of the Galactic inventories of interstellar dust and its composition
• On the Galactic chemical evolution of sulphur. Sulphur abundances from the [S i] 1082 nm line in giants
• APOGEE chemical abundances of stars in the MW satellites Fornax, Sextans, Draco and Carina
• Stellar Abundances at the Center of Early Type Galaxies with Fine Structure
• On the Chemical Composition of the Evolved Very Bright Metal-Poor Star HD 1936
• Type Iax supernovae from deflagrations in Chandrasekhar mass white dwarfs
• Chemical composition and ages of four globular clusters in M31 from the analysis of their integrated-light spectra