Updated stellar yields from Asymptotic Giant Branch models

Abstract

An updated grid of stellar yields for low to intermediate-mass thermally-pulsing Asymptotic Giant Branch (AGB) stars are presented. The models cover a range in metallicity Z = 0.02, 0.008, 0.004, and 0.0001, and masses between 1Msun to 6Msun. New intermediate-mass Z = 0.0001 AGB models are also presented, along with a finer mass grid than used in previous studies. The yields are computed using an updated reaction rate network that includes the latest NeNa and MgAl proton capture rates, with the main result that between ~6 to 30 times less Na is produced by intermediate-mass models with hot bottom burning. In low-mass AGB models we investigate the effect on the production of light elements of including some partial mixing of protons into the intershell region during the deepest extent of each third dredge-up episode. The protons are captured by the abundant 12C to form a 13C pocket. The 13C pocket increases the yields of 19F, 23Na, the neutron-rich Mg and Si isotopes, 60Fe, and 31P. The increase in 31P is by factors of ~4 to 20, depending on the metallicity. Any structural changes caused by the addition of the 13C pocket into the He-intershell are ignored. However, the models considered are of low mass and any such feedback is likely to be small. Further study is required to test the accuracy of the yields from the partial-mixing models. For each mass and metallicity, the yields are presented in a tabular form suitable for use in galactic chemical evolution studies or for comparison to the composition of planetary nebulae.

Accepted for publication in MNRAS; 15 pages

References in corpus (9)

• Stellar Models and Yields of Asymptotic Giant Branch Stars
• Origin of multiple stellar populations in globular clusters and their helium enrichment
• Nucleosynthesis Predictions for Intermediate-Mass AGB Stars: Comparison to Observations of Type I Planetary Nebulae
• Thermohaline mixing and gravitational settling in carbon-enhanced metal-poor stars
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• Low temperature Rosseland opacities with varied abundances of carbon and nitrogen
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• The impact of the 18F(a,p)21Ne reaction on asymptotic giant branch nucleosynthesis
• The thermonuclear rate for the 19F(a,p)22Ne reaction at stellar temperatures

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• Evidence of extra-mixing in field giants as traced by lithium and carbon isotope ratio
• Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• Molecular line study of the S-type AGB star W Aquilae. ALMA observations of CS, SiS, SiO and HCN
• The Oxygen Abundance in the Solar Neighborhood
• The most metal-rich asymptotic giant branch stars
• Chemical enrichment in the cool core of the Centaurus cluster of galaxies
• Chemical Abundances of Planetary Nebulae in the Substructures of M31 -- II. The Extended Sample and A Comparison Study with the Outer-disk Group
• A high-mass Planetary Nebula in a Galactic Open Cluster
• Spatially Resolved X-ray Spectroscopy of Kepler's Supernova Remnant: Distinct Properties of the Circumstellar Medium and the Ejecta
• Modelling the nucleosynthetic properties of carbon-enhanced metal-poor RR Lyrae stars
• Supernova 1604, Kepler's supernova, and its remnant
• Developing a self-consistent AGB wind model: I. Chemical, thermal, and dynamical coupling
• Peeking beneath the precision floor I: metallicity spreads and multiple elemental dispersions in the globular clusters NGC 288 and NGC 362
• BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
• Galactic planetary nebulae with precise nebular abundances as a tool to understand the evolution of asymptotic giant branch stars
• Heavy element abundances in P-rich stars: A new site for the s-process?
• How do atomic code uncertainties affect abundance measurements in the intracluster medium?
• Probing O-enrichment in C-rich dust planetary nebulae
• Chemical evolution of ${}^{26}$Al and ${}^{60}$Fe in the Milky Way
• HIP 10725: The First Solar Twin/Analogue Field Blue Straggler
• Bridging the Gap between Intermediate and Massive Stars I: Validation of MESA against the State-of-the-Art Monash Stellar Evolution Program for a 2$M_{\odot }$ AGB Star
• Nucleosynthetic yields of Z=$10^{-5}$ intermediate-mass stars
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• CNO and F abundances in the barium star HD 123396
• Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
• A chemical signature from fast-rotating low-metallicity massive stars: ROA 276 in omega Centauri
• Inhomogeneous Galactic Chemical Evolution: Modelling Ultra-Faint Dwarf Galaxies of the Large Magellanic Cloud
• The Pristine Inner Galaxy Survey (PIGS) VII: a discovery of the first inner Galaxy CEMP-r/s star
• Discovery of a Metal-poor, Luminous Post-AGB Star that Failed the Third Dredge-up
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• Star formation within globular clusters:discrete multiple bursts and top-light mass functions
• Co-spatial Long-slit UV/Optical Spectra of Ten Galactic Planetary Nebulae with HST/STIS II. Nebular Models, Central Star Properties and He+CNO Synthesis
• Towards a fully consistent Milky Way disk model -- IV. The impact of Gaia DR2 and APOGEE
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• A Census of Thermally-Pulsing AGB stars in the Andromeda Galaxy and a First Estimate of their Contribution to the Global Dust Budget
• On the presence of metallofullerenes in fullerene-rich circumstellar envelopes
• Nitrogen evolution in the halo, thick disc, thin disc and bulge of the Galaxy
• Observational constraints on the origin of the elements. VI. Origin and evolution of neutron-capture elements as probed by the Gaia-ESO survey
• Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
• GalCEM I -- An Open-Source Detailed Isotopic Chemical Evolution Code
• Explaining the ${}^{12}\text{C}{/}^{13}\text{C}$ ratio in the Galactic halo: the contribution from shell mergers in primordial massive stars
• Physical properties of the fullerene C60-containing planetary nebula SaSt 2-3
• Formation of ultra-compact dwarf galaxies from supergiant molecular clouds
• First detection of AlF line emission towards M-type AGB stars
• Characterization of M-stars in the LMC in the JWST era
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Lithium in red giants: the roles of the He-core flash and the luminosity bump
• The chemistry of extragalactic carbon stars
• Near-infrared chemical abundances of stars in the Sculptor dwarf galaxy
• Outside-in stellar formation in the spiral galaxy M33?
• Chemical evolution of ultra-faint dwarf galaxies: testing the IGIMF
• On the delay times of merging double neutron stars
• Uncertainties in AGB Evolution and Nucleosynthesis
• Modeling Increased Metal Production in Galaxy Clusters with Pair-Instability Supernovae
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• A New Grid of Synthetic Spectra for the Analysis of [WC]-type Central Stars of Planetary Nebulae
• Observational nuclear astrophysics: neutron-capture element abundances in old, metal-poor stars
• Spectroscopic study of four metal-poor carbon stars from the Hamburg/ESO Survey: On confirming the low-mass nature of their companions
• Observational constraints on the origin of the elements. IX. 3D NLTE abundances of metals in the context of Galactic Chemical Evolution Models and 4MOST
• A molecular line survey of a sample of AGB stars and planetary nebulae
• A panchromatic view of star cluster formation in a simulated dwarf galaxy starburst
• The population of planetary nebulae near the Galactic centre: chemical abundances
• Rotational mixing in carbon-enhanced metal-poor stars with s-process enrichment
• Colour-magnitude diagram in simulations of galaxy formation
• Physical properties of the very young PN Hen3-1357 (Stingray Nebula) based on multiwavelength observations
• The undiscovered ultra-diffuse galaxies of the Local Group
• Chemical Abundances in the PN Wray16-423 in the Sagittarius Dwarf Spheroidal Galaxy: Constraining the Dust Composition
• He abundances in disc galaxies -- I. Predictions from cosmological chemodynamical simulations
• Star Formation and Chemical Enrichment in Protoclusters
• Stellar ($n,\gamma$) cross section of ${}^{23}$Na
• Peeking beneath the precision floor -- II. Probing the chemo-dynamical histories of the potential globular cluster siblings, NGC 288 and NGC 362
• The evolution of the galaxy and the birth of the solar system: The short-lived nuclides connection
• Chemistry in the dIrr galaxy Leo A
• Can Galactic chemical evolution explain the oxygen isotopic variations in the Solar System?
• Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars
• Mergers all the way down: stellar collisions and kinematics of a dense hierarchically forming massive star cluster in a dwarf starburst
• Detailed Chemical Abundances of Star Clusters in the Large Magellanic Cloud
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• Adding a Suite of Chemical Abundances to the MACER Code for the Evolution of Massive Elliptical Galaxies
• Physical and chemical properties of Wolf-Rayet planetary nebulae
• Probing the nucleosynthetic contribution of low-metallicity, low-mass star companions of CEMP stars
• Evolution of Hen\,3-1357, the Stingray Nebula
• Cloud-cloud collisions triggering star formation in galaxy simulations
• HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
• Europium, we have a problem. Modelling r-process enrichment across Local Group galaxies
• The ${}^{22}$Ne($\alpha$,n)${}^{25}$Mg reaction -- state of the art, astrophysics, and perspectives
• A neutron star candidate in the long-period binary 56 UMa
• Evolution of radioactive elements in the LMC: predictions for future gamma-ray surveys
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Measuring Dwarf Galaxy Intrinsic Abundance Scatter with Mid-resolution Spectroscopic Surveys: Calibrating APOGEE Abundance Errors
• Light Element Chemistry and the Double Red Giant Branch in the Galactic Globular Cluster NGC 288
• A Carbon-enhanced Lyman Limit System: Signature of the First Generation of Stars?
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• The cosmological lithium problem
• Planetary nebulae with Wolf-Rayet-type central stars -- IV. NGC 1501 and its mixing layer
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy
• Nitrogen Abundance Distribution in the inner Milky Way
• New Constraints on Sodium Production in Globular Clusters From the ${}^{23}$Na${(}^3$He$,\text{d}{)}^{24}$Mg Reaction
• Metallicity gradients in M31, M33, NGC 300 and the Milky Way using abundances of different elements
• Stellar Populations in a semi-analytic model I: bulges of Milky Way-like galaxies
• A survey of extremely metal-poor gas at cosmic noon: evidence of elevated [O/Fe]
• Constraints on $R$-process Nucleosynthesis from ${}^{129}$I and ${}^{247}$Cm in the Early Solar System
• Dating N loud AGNs at high redshift: GS3073 as a snapshot of wCen like evolution of a nuclear star cluster
• High-resolution spectroscopic study of dwarf stars in the northern sky: Na to Zn abundances in two fields with radii of 20 degrees
• Strength of the E_R = 127 keV, 26Al(p,g)27Si resonance
• The impact of improved plasma diagnostics on modeling the X-ray Universe
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• s-process Enriched Post-AGB Star J003643.94-723722.1 in the SMC with an Extreme C/O Ratio and the First Precise Detection of Lead
• Ionized carbon around IRC +10216
• Assessing stellar yields in Galaxy chemical evolution: observational stellar abundance patterns
• Binary stellar evolution yields in galactic chemical evolution calculations
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• History of the mass ejection in K 4-37: from the AGB to the evolved planetary nebula phase
• On the Thermally Pulsing Asymptotic Giant Branch Contribution to the Light of Nearby Disk Galaxies
• Bulge Fossil Fragments as a new population of factories of gravitational wave sources in the Galaxy
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• Extragalactic Planetary Nebulae: tracers of the chemical evolution of nearby galaxies
• Fluorine abundances in CEMP stars at the lowest metallicity: Hints on the nature of the first stars
• The Missing Link: Testing Galactic Chemical Evolution Models with the First Multi-Isotopic Abundances in Solar Twin Stars
• The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios
• Unevolved Li-rich stars at low metallicity: a possible formation pathway through novae
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Probing the dynamical and kinematical structures of detached shells around AGB stars
• Observations of the planetary nebula RWT 152 with OSIRIS/GTC
• Aluminium-26 production in low- and intermediate-mass binary systems
• The LEGARE Project. I. Chemical evolution model of the Nuclear Stellar Disc in a Bayesian framework
• Physical Conditions and Chemical Abundances of the Variable Planetary Nebula IC 4997
• Interrelations between Astrochemistry and Galactic Dynamics
• Full abundance study of two newly discovered barium giants
• Morpho-kinematic and photoionization models of the multipolar structures in planetary nebula NGC 6572
• Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
• Modelling the chemical evolution of the Milky Way
• Dust contribution to the panchromatic galaxy emission
• The aluminium-26 distribution in a cosmological simulation of a Milky Way-type Galaxy
• Massive stars: stellar models and stellar yields, impact on Galactic Archaeology
• Rapid evolution of [WC] stars in the Magellanic Clouds
• Planetary nebulae with Wolf-Rayet-type central stars -- III. A detailed view of NGC 6905 and its central star
• The planetary nebula nature and properties of IRAS18197-1118
• The curious conundrum regarding sulfur and oxygen abundances in planetary nebulae
• Reduce, Reuse, Recycle: Planetary Nebulae as Green Galactic Citizens
• The assembly history of NGC 1365 through chemical archaeology
• Precision Analysis of ${}^{12}\mathrm{C}{/}^{13}\mathrm{C}$ Ratios in Orion IRc2 Acetylene Isotopologues via ${\chi }^2$ Fitting
• AGB nucleosynthesis at low metallicity: what can we learn from carbon- and s-elements-enhanced metal-poor stars
• The Metallicity Distribution Function in Outer Halo Fields of Simulated Elliptical Galaxies Compared to Observations of NGC 5128
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• A Census of Sun's Ancestors and their Contributions to the Solar System Chemical Composition
• On the Galactic chemical evolution of sulphur. Sulphur abundances from the [S i] 1082 nm line in giants
• EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy
• The Two-infall Model Revisited: Constraints on Milky Way Bulge Assembly from >30,000 Galactic Chemical Evolution Models and Machine Learning
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Gas and dust from extremely metal-poor AGB stars
• Rapid early gas accretion for the inner Galactic disc
• The chemical DNA of the Magellanic Clouds VI. Origin and evolution of neutron-capture elements in the SMC
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• Viability of novae as sources of Galactic lithium
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Short-lived Radionuclides in the Milky Way Galaxy
• The Impact of the New ${}^{59}$Fe Decay Rates on ${}^{60}$Fe and ${}^{26}$Al Nucleosynthesis in Massive Stars
• A comparative study on three modes of s-process nucleosynthesis in extremely metal-poor AGB stars