The Dawes Review 2: Nucleosynthesis and stellar yields of low and intermediate-mass single stars
arXiv:1405.0062 · doi:10.1017/pasa.2014.21
Abstract
The chemical evolution of the Universe is governed by the chemical yields from stars, which in turn is determined primarily by the initial stellar mass. Even stars as low as 0.9Msun can, at low metallicity, contribute to the chemical evolution of elements. Stars less massive than about 10Msun experience recurrent mixing events that can significantly change the surface composition of the envelope, with observed enrichments in carbon, nitrogen, fluorine, and heavy elements synthesized by the slow neutron capture process (the s-process). Low and intermediate mass stars release their nucleosynthesis products through stellar outflows or winds, in contrast to massive stars that explode as core-collapse supernovae. Here we review the stellar evolution and nucleosynthesis for single stars up to ~10Msun from the main sequence through to the tip of the asymptotic giant branch (AGB). We include a discussion of the main uncertainties that affect theoretical calculations and review the latest observational data, which are used to constrain uncertain details of the stellar models. We finish with a review of the stellar yields available for stars less massive than about 10Msun and discuss efforts by various groups to address these issues and provide homogeneous yields for low and intermediate-mass stars covering a broad range of metallicities.
Invited Review accepted by Publications of the Astronomical Society of Australia; 70 pages
References in corpus (49)
- Pre-Supernova Evolution of Massive Single and Binary Stars
- Galactic chemical evolution: Carbon through Zinc
- Magnetorotationally driven Supernovae as the origin of early galaxy -process elements?
- Carbon Enhanced Metal-Poor Stars. I. Chemical Compositions of 26 Stars
- Evidence for TP-AGB stars in high redshift galaxies, and their effect on deriving stellar population parameters
- A Bitter Pill: The Primordial Lithium Problem Worsens
- Stellar Models and Yields of Asymptotic Giant Branch Stars
- The Supernova Channel of Super-AGB Stars
- Deep Mixing of He-3: Reconciling Big Bang and Stellar Nucleosynthesis
- Production of Light Element Primary Process nuclei in neutrino-driven winds
- Multiple stellar populations in three rich Large Magellanic Cloud star clusters
- Can Extra Mixing in RGB and AGB Stars Be Attributed to Magnetic Mechanisms?
- The chemical composition of red giant stars in four intermediate-age clusters of the Large Magellanic Cloud
- Rubidium-Rich Asymptotic Giant Branch Stars
- Stellar Archaeology -- Exploring the Universe with Metal-Poor Stars
- s-Process Nucleosynthesis in Advanced Burning Phases of Massive Stars
- Nitrogen abundances in giant stars of the globular cluster NGC 6752
- Super and massive AGB stars - III. Nucleosynthesis in metal-poor and very metal-poor stars - Z=0.001 and 0.0001
- Chemical Transport and Spontaneous Layer Formation in Fingering Convection in Astrophysics
- Nucleosynthesis Predictions for Intermediate-Mass AGB Stars: Comparison to Observations of Type I Planetary Nebulae
- The Magellanic zoo: Mid-infrared Spitzer spectroscopy of evolved stars and circumstellar dust in the Magellanic Clouds
- Thermohaline mixing and gravitational settling in carbon-enhanced metal-poor stars
- Planetary Nebula Abundances and Morphology: Probing the Chemical Evolution of the Milky Way
- Magnetic Mixing in Red Giant and Asymptotic Giant Branch Stars
- Discovery of two distinct red clumps in NGC419: a rare snapshot of a cluster at the onset of degeneracy
- First full evolutionary computation of the He-flash induced mixing in Population II stars
- Supernova Fallback: A Possible Site for the r-Process
- The Role of Planet Accretion in Creating the Next Generation of Red Giant Rapid Rotators
- Deep Mixing and Metallicity: Carbon Depletion in Globular Cluster Giants
- Fe and Al Abundances for 180 Red Giants in the Globular Cluster Omega Centauri (NGC 5139)
- The Chemical Evolution of Helium in Globular Clusters: Implications for the Self-Pollution Scenario
- Heavy elements in Globular Clusters: the role of AGB stars
- High resolution infrared spectra of NGC 6440 and NGC 6441: two massive Bulge Globular Clusters
- Abundances in intermediate-mass AGB stars undergoing third dredge-up and hot-bottom burning
- The trigger of the AGB superwind: the importance of carbon
- Mass loss and yield uncertainty in low-mass asymptotic giant branch stars
- Cosmological implications of dwarf spheroidal chemical evolution
- The Planetary Nebula population of the Sagittarius Dwarf Spheroidal Galaxy
- Hubble Space Telescope Images of Magellanic Cloud Planetary Nebulae
- The Super Lithium-Rich Red Giant Rapid Rotator G0928+73.2600: A Case for Planet Accretion?
- On the Iron content of NGC 1978 in the LMC: a metal rich, chemically homogeneous cluster
- Red Giant stars in the Large Magellanic Cloud clusters
- Molecular shells in IRC+10216: Evidence for non-isotropic and episodic mass loss enhancement
- Near-Infrared Spectroscopy of Carbon-Enhanced Metal-Poor Stars. I. A SOAR/OSIRIS Pilot Study
- Detection of Fluorine in the Halo Planetary Nebula BoBn 1: Evidence For a Binary Progenitor Star
- Stellar Nucleosynthesis in the Hyades Open Cluster
- The impact of the 18F(a,p)21Ne reaction on asymptotic giant branch nucleosynthesis
- Red clump stars of the Milky Way - laboratories of extra-mixing
- Metal-rich carbon stars in the Sagittarius Dwarf Spheroidal galaxy
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