NuGrid Stellar Data Set. II. Stellar Yields from H to Bi for Stellar Models with Mzams = 1 to 25Msun and Z = 0.0001 to 0.02

Abstract

We provide here a significant extension of the NuGrid Set 1 models in mass coverage and toward lower metallicity, adopting the same physics assumptions. The combined data set now includes the initial masses M/Msun = 1, 1.65, 2, 3, 4, 5, 6, 7, 12, 15, 20, 25 for Z = 0.02, 0.01, 0.006, 0.001, 0.0001 with alpha-enhanced composition for the lowest three metallicities. These models are computed with the MESA stellar evolution code and are evolved up to the AGB, the white dwarf stage, or until core collapse. The nucleosynthesis was calculated for all isotopes in post-processing with the NuGrid mppnp code. Explosive nucleosynthesis is based on semi-analytic 1D shock models. Metallicity-dependent mass loss, convective boundary mixing in low- and intermediate mass models and H and He core burning massive star models is included. Convective O-C shell mergers in some stellar models lead to the strong production of odd-Z elements P, Cl, K and Sc. In AGB models with hot dredge-up the convective boundary mixing efficiency is reduced to accommodate for its energetic feedback. In both low-mass and massive star models at the lowest metallicity H-ingestion events are observed and lead to i-process nucleosynthesis and substantial N-15 production. Complete yield data tables, derived data products and online analytic data access are provided.

Published. Detailed online data available at Canadian Astronomical Data Center, DOI:10.11570/18.0002 (http://www.canfar.phys.uvic.ca/vospace/nodes/AstroDataCitationDOI/CISTI.CANFAR/18.0002/18.0002.html?view=data). See Appendix for details

References in corpus (19)

• Modules for Experiments in Stellar Astrophysics (MESA)
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Theory of Core-Collapse Supernovae
• Galactic chemical evolution: Carbon through Zinc
• The nucleosynthesis of Al26 and Fe60 in solar metallicity stars extending in mass from 11 to 120 Msun: the hydrostatic and explosive contributions
• Very low metallicity massive star models: Pre-SN evolution and primary nitrogen production
• Effects of rotation on the evolution of primordial stars
• The evolution of runaway stellar collision products
• The Status of Multi-Dimensional Core-Collapse Supernova Models
• Evolution and nucleosynthesis of asymptotic giant branch stellar models of low metallicity
• Can Extra Mixing in RGB and AGB Stars Be Attributed to Magnetic Mechanisms?
• s-Process Nucleosynthesis in Advanced Burning Phases of Massive Stars
• Super and massive AGB stars - III. Nucleosynthesis in metal-poor and very metal-poor stars - Z=0.001 and 0.0001
• i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs
• Evolution of Thermally Pulsing Asymptotic Giant Branch Stars IV. Constraining Mass-Loss & Lifetimes of Low Mass, Low Metallicity AGB Stars
• On Carbon Burning in Super Asymptotic Giant Branch Stars
• Heavy elements in Globular Clusters: the role of AGB stars
• Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning
• Cyberhubs: Virtual Research Environments for Astronomy

Cited by in corpus (109)

• Neutron Star Mergers Might not be the Only Source of r-Process Elements in the Milky Way
• r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos
• Simulating an Isolated Dwarf Galaxy with Multi-Channel Feedback and Chemical Yields from Individual Stars
• Is GW190521 the merger of black holes from the first stellar generations?
• Pop III $\text{i}$-process Nucleosynthesis and the Elemental Abundances of SMSS J0313-6708 and the Most Iron-Poor Stars
• Remnants and ejecta of thermonuclear electron-capture supernovae: Constraining oxygen-neon deflagrations in high-density white dwarfs
• Enrichment of the hot intracluster medium: observations
• Missing Red Supergiants and Carbon Burning
• New full evolutionary sequences of H and He atmosphere massive white dwarf stars using MESA
• NuGrid stellar data set - III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z=0.01, Z=0.02 and Z=0.03
• 3D hydrodynamic simulations of C ingestion into a convective O shell
• Re-evaluation of the ${}^{22}$Ne($\alpha ,\gamma$)${}^{26}$Mg and ${}^{22}$Ne($\alpha ,n$)${}^{25}$Mg reaction rates
• The s process in AGB stars as constrained by a large sample of Barium stars
• The gas, metal and dust evolution in low-metallicity local and high-redshift galaxies
• Convective H-He Interactions in Massive Population III Stellar Evolution Models
• i-Process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-Peak Neutron-Capture Elements
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• Grids of stellar models with rotation VII: Models from 0.8 to 300 M${}_{\odot }$ at super-solar metallicity (Z = 0.020)
• Metal Mixing and Ejection in Dwarf Galaxies is Dependent on Nucleosynthetic Source
• Abundance ratios in GALAH DR2 and their implications for nucleosynthesis
• The evolution of CNO elements in galaxies
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• The intermediate neutron capture process. III. The i-process in AGB stars of different masses and metallicities without overshoot
• Phosphorus-rich stars with unusual abundances are challenging theoretical predictions
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• The physics of Core-Collapse Supernovae: explosion mechanism and explosive nucleosynthesis
• ${}^{60}$Fe in core-collapse supernovae and prospects for X-ray and $\gamma$-ray detection in supernova remnants
• SYGMA: Stellar Yields for Galactic Modeling Applications
• Aluminium-26 from massive binary stars I: non-rotating models
• Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency
• Convective boundary mixing in a post-He core burning massive star model
• Evidence for sub-Chandrasekhar Type Ia supernovae from the last major merger
• The $\gamma$-process nucleosynthesis in core-collapse supernovae. I. A novel analysis of $\gamma$-process yields in massive stars
• Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System
• The impact of (n,$\gamma$) reaction rate uncertainties of unstable isotopes on the i-process nucleosynthesis of the elements from Ba to W
• The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
• Exploring Chemical Homogeneity in Dwarf Galaxies: A VLT-MUSE study of JKB 18
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• 3D1D hydro-nucleosynthesis simulations. I. Advective-reactive post-processing method and its application to H ingestion into He-shell flash convection in rapidly accreting white dwarfs
• The energy distribution of the first supernovae
• Radioactive nuclei in the early Solar System: analysis of the 15 isotopes produced by core-collapse supernovae
• Trans-iron Ge, As, Se, and heavier elements in the dwarf metal-poor stars, HD~19445, HD~84937, HD~94028, HD~140283, and HD~160617
• First inverse kinematics study of the ${}^{22}$Ne$(p,\gamma {)}^{23}$Na reaction and its role in AGB star and classical nova nucleosynthesis
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Impact of Convective Boundary Mixing on the TP-AGB
• Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution
• 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?
• Chemical Evolution of Fluorine in the Milky Way
• Measurement of 73Ge(n,g) cross sections and implications for stellar nucleosynthesis
• Study of (${}^6$Li, $d$) and (${}^6$Li, $t$) reactions on ${}^{22}$Ne and implications for $s$-process nucleosynthesis
• Characterizing the Circumgalactic Medium of the Lowest-Mass Galaxies: A Case Study of IC 1613
• Enrichment of the Galactic disc with neutron-capture elements: Mo and Ru
• EDGE-INFERNO: Simulating every observable star in faint dwarf galaxies and their consequences for resolved-star photometric surveys
• 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
• BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
• Disc dichotomy signature in the vertical distribution of [Mg/Fe] and the delayed gas infall scenario
• Nucleosynthetic yields of Z=$10^{-5}$ intermediate-mass stars
• 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
• Type Ia Supernova Nucleosynthesis: Metallicity-Dependent Yields
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM
• Chemical abundances in Seyfert galaxies X. Sulphur abundance estimates
• Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates
• The Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars
• Reanalysis of neutron-capture elements in the benchmark r-rich star CS 31082-001
• Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium
• Explaining the ${}^{12}\text{C}{/}^{13}\text{C}$ ratio in the Galactic halo: the contribution from shell mergers in primordial massive stars
• Progenitor-mass-dependent yields amplify intrinsic scatter in dwarf-galaxy elemental abundance ratios
• Unveiling the chemical fingerprint of phosphorus-rich stars I. In the infrared region of APOGEE-2
• First inverse kinematics measurement of key resonances in the ${}^{22}\text{Ne}(p,\gamma {)}^{23}\text{Na}$ reaction at stellar temperatures
• Peeking beneath the precision floor -- II. Probing the chemo-dynamical histories of the potential globular cluster siblings, NGC 288 and NGC 362
• Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars
• Isotopic ratios for C, N, Si, Al, and Ti in C-rich presolar grains from massive stars
• The ${}^{22}$Ne($\alpha$,n)${}^{25}$Mg reaction -- state of the art, astrophysics, and perspectives
• Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
• The NuGrid AGB Evolution and Nucleosynthesis Data Set
• The s process in massive stars, a benchmark for neutron capture reaction rates
• The cosmological lithium problem
• Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars
• The $\gamma$-process nucleosynthesis in core-collapse supernovae II. Effect of the explosive recipe
• On the Contribution of Very Massive Stars to the Sulfur Abundance in Star-Forming Galaxies: the Role of PISN
• Impact of newly measured 26Al(n, p)26Mg and 26Al(n, α)23Na reaction rates on the nucleosynthesis of 26Al in stars
• Exploring circumstellar effects on the lithium and calcium abundances in massive Galactic O-rich AGB stars
• First models of s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver
• SHADES -- ${}^{22}$Ne($\alpha$,n)${}^{25}$Mg reaction rate in the Gamow window
• Reconstructing the Milky Way chemical map with Galactic Chemical Evolution tool OMEGA+ from SDSS-MWM
• Assessing stellar yields in Galaxy chemical evolution: observational stellar abundance patterns
• Silicon Isotopic Composition of Mainstream Presolar SiC Grains Revisited: The Impact of Nuclear Reaction Rate Uncertainties
• The SPAr burning: proton captures powering carbon-oxygen shell mergers in massive stars
• Constraining the Synthesis of the Lightest p Nucleus 74Se
• Self-Organization In Stellar Evolution: Size-Complexity Rule
• Thorne-Żytkow Objects
• Unevolved Li-rich stars at low metallicity: a possible formation pathway through novae
• Strontium-84 Enrichments in Presolar Grains Provide First Evidence of p-process Nucleosynthesis in Core-collapse Supernovae
• Production of heavy $\alpha$-elements and ${}^{44}$Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers
• Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• A Large-scale Approach to Modelling Molecular Biosignatures: The Diatomics
• Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs
• X-ray and radio data obtained by XMM-Newton and VLA constrain the stellar wind of the magnetic quasi-Wolf-Rayet star in HD45166
• A Theoretical Study of the Structure and Elemental Abundances of HD 20794
• EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Chemical abundances in Seyfert galaxies -- VII. Direct abundance determination of neon based on optical and infrared emission lines
• Project ThaiPASS: International Outreach Blending Astronomy and Python
• Isotopic Compositions of Ruthenium Predicted from the NuGrid Project
• The Two-infall Model Revisited: Constraints on Milky Way Bulge Assembly from >30,000 Galactic Chemical Evolution Models and Machine Learning