The Dawes review 2: nucleosynthesis and stellar yields of low-and intermediate-mass single stars
AI Karakas, JC Lattanzio - Publications of the Astronomical Society of …, 2014 - cambridge.org
The chemical evolution of the Universe is governed by the chemical yields from stars, which
in turn are determined primarily by the initial stellar mass. Even stars as low as 0.9 M⊙ can …
in turn are determined primarily by the initial stellar mass. Even stars as low as 0.9 M⊙ can …
Chemical evolution with rotating massive star yields–I. The solar neighbourhood and the s-process elements
N Prantzos, C Abia, M Limongi, A Chieffi… - Monthly Notices of the …, 2018 - academic.oup.com
We present a comprehensive study of the abundance evolution of the elements from H to U
in the Milky Way halo and local disc. We use a consistent chemical evolution model …
in the Milky Way halo and local disc. We use a consistent chemical evolution model …
Stellar yields from metal-rich asymptotic giant branch models
AI Karakas, M Lugaro - The Astrophysical Journal, 2016 - iopscience.iop.org
We present new theoretical stellar yields and surface abundances for three grids of metal-
rich asymptotic giant branch (AGB) models. Post-processing nucleosynthesis results are …
rich asymptotic giant branch (AGB) models. Post-processing nucleosynthesis results are …
Nuclear astrophysics and the trojan horse method
In this review, we discuss the new recent results of the Trojan Horse Method that is used to
determine reaction rates for nuclear processes in several astrophysical scenarios. The …
determine reaction rates for nuclear processes in several astrophysical scenarios. The …
Evolution, nucleosynthesis, and yields of low-mass asymptotic giant branch stars at different metallicities. II. The FRUITY database
S Cristallo, L Piersanti, O Straniero… - The Astrophysical …, 2011 - iopscience.iop.org
By using updated stellar low-mass stars models, we systematically investigate the
nucleosynthesis processes occurring in asymptotic giant branch (AGB) stars. In this paper …
nucleosynthesis processes occurring in asymptotic giant branch (AGB) stars. In this paper …
The s-process in low-metallicity stars – II. Interpretation of high-resolution spectroscopic observations with asymptotic giant branch models
S Bisterzo, R Gallino, O Straniero… - Monthly Notices of …, 2011 - academic.oup.com
High-resolution spectroscopic observations of 100 metal-poor carbon and s-rich stars
(CEMP-s) collected from the literature are compared with the theoretical nucleosynthesis …
(CEMP-s) collected from the literature are compared with the theoretical nucleosynthesis …
Light elements in the Universe
Due to their production sites, as well as to how they are processed and destroyed in stars,
the light elements are excellent tools to investigate a number of crucial issues in modern …
the light elements are excellent tools to investigate a number of crucial issues in modern …
Presolar grain isotopic ratios as constraints to nuclear and stellar parameters of asymptotic giant branch star nucleosynthesis
Recent models for evolved low-mass stars (with M≲ 3 M⊙), undergoing the asymptotic giant
branch (AGB) phase assume that magnetic flux-tube buoyancy drives the formation of 13 C …
branch (AGB) phase assume that magnetic flux-tube buoyancy drives the formation of 13 C …
Deep mixing in evolved stars. I. The effect of reaction rate revisions from C to Al
S Palmerini, M La Cognata, S Cristallo… - The Astrophysical …, 2011 - iopscience.iop.org
We present computations of nucleosynthesis in low-mass (LM) red giant branch (RGB) and
asymptotic giant branch (AGB) stars of Population I experiencing extended mixing. We adopt …
asymptotic giant branch (AGB) stars of Population I experiencing extended mixing. We adopt …
s-processing in AGB stars revisited. III. Neutron captures from MHD mixing at different metallicities and observational constraints
We present post-process neutron-capture computations for Asymptotic Giant Branch (AGB)
stars of 1.5–3 M⊙ and metallicities− 1.3≤[Fe/H]≤ 0.1. The reference stellar models are …
stars of 1.5–3 M⊙ and metallicities− 1.3≤[Fe/H]≤ 0.1. The reference stellar models are …