The s Process and Beyond

M Lugaro, M Pignatari, R Reifarth… - Annual Review of …, 2023 - annualreviews.org
Neutron captures produce the vast majority of abundances of elements heavier than iron in
the Universe. Beyond the classical slow (s) and rapid (r) processes, there is observational …

LUNA: Status and prospects

C Broggini, D Bemmerer, A Caciolli, D Trezzi - Progress in Particle and …, 2018 - Elsevier
The essential ingredients of nuclear astrophysics are the thermonuclear reactions which
shape the life and death of stars and which are responsible for the synthesis of the chemical …

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 …

Evolution, nucleosynthesis, and yields of AGB stars at different metallicities. III. Intermediate-mass models, revised low-mass models, and the ph-FRUITY interface

S Cristallo, O Straniero, L Piersanti… - The Astrophysical …, 2015 - iopscience.iop.org
We present a new set of models for intermediate-mass asymptotic giant branch (AGB) stars
(4.0, 5.0, and 6.0 M⊙) at different metallicities (− 2.15≤[Fe/H]≤+ 0.15). This set integrates …

Target selection for the apache point observatory Galactic evolution experiment (APOGEE)

G Zasowski, JA Johnson, PM Frinchaboy… - The Astronomical …, 2013 - iopscience.iop.org
ABSTRACT The Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a
high-resolution infrared spectroscopic survey spanning all Galactic environments (ie, bulge …

[LIBRO][B] Supernova explosions

D Branch, JC Wheeler - 2017 - Springer
JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …

NuGrid stellar data set. I. Stellar yields from H to Bi for stars with metallicities Z= 0.02 and Z= 0.01

M Pignatari, F Herwig, R Hirschi… - The Astrophysical …, 2016 - iopscience.iop.org
We provide a set of stellar evolution and nucleosynthesis calculations that applies
established physics assumptions simultaneously to low-and intermediate-mass and massive …

Super-and massive AGB stars–IV. Final fates–initial-to-final mass relation

CL Doherty, P Gil-Pons, L Siess… - Monthly Notices of …, 2015 - academic.oup.com
We explore the final fates of massive intermediate-mass stars by computing detailed stellar
models from the zero-age main sequence until near the end of the thermally pulsing phase …

Super-AGB stars and their role as electron capture supernova progenitors

CL Doherty, P Gil-Pons, L Siess… - Publications of the …, 2017 - cambridge.org
We review the lives, deaths and nucleosynthetic signatures of intermediate-mass stars in the
range≈ 6–12 M⊙, which form super-AGB stars near the end of their lives. The critical mass …

Exploring anticorrelations and light element variations in northern globular clusters observed by the APOGEE survey

S Mészáros, SL Martell, M Shetrone… - The Astronomical …, 2015 - iopscience.iop.org
We investigate the light-element behavior of red giant stars in northern globular clusters
(GCs) observed by the SDSS-III Apache Point Observatory Galactic Evolution Experiment …