After the Big Bang, production of heavy elements in the early Universe takes place starting
from the formation of the first stars, their evolution, and explosion. The first supernova …

In this review, we discuss the present status of three indirect techniques that are used to
determine reaction rates for stellar burning processes, asymptotic normalization coefficients …

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 …

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 …

By using updated stellar low-mass stars models, we systematically investigate the
nucleosynthesis processes occurring in asymptotic giant branch (AGB) stars. In this paper …

Isotope ratios have opened a new window into the study of the details of stellar evolution,
supernovae and galactic chemical evolution. We present the evolution of the isotope ratios …

We provide a set of stellar evolution and nucleosynthesis calculations that applies
established physics assumptions simultaneously to low-and intermediate-mass and massive …

Chemical equilibrium has proven extremely useful for predicting the chemical composition of
AGB atmospheres. Here we use a recently developed code and an updated thermochemical …

We present stellar evolutionary tracks and nucleosynthetic predictions for a grid of stellar
models of low-and intermediate-mass asymptotic giant branch (AGB) stars at Z= 0.001 …

Context. Recent studies show that rotation significantly affects the s-process in massive
stars. Aims. We provide tables of yields for non-rotating and rotating massive stars between …