▪ Abstract The current status of modeling the evolution and nucleosynthesis of asymptotic
giant branch (AGB) stars is reviewed. The principles of AGB evolution have been …

▪ Abstract This review emphasizes the mass loss processes that affect the fates of single
stars with initial masses between one and nine solar masses. Just one epoch of mass loss …

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 large set of theoretical isochrones, whose distinctive features mostly reside on
the greatly-improved treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) …

We present the colibri code for computing the evolution of stars along the thermally pulsing
asymptotic giant branch (TP-AGB) phase. Compared to purely synthetic TP-AGB codes …

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

We present new synthetic models of the TP-AGB evolution. They are computed for 7 values
of initial metal content (Z from 0.0001 to 0.03) and for initial masses between 0.5 and 5.0 …

We present the results of s-process nucleosynthesis calculations for asymptotic giant branch
(AGB) stars of different metallicities and different initial stellar masses (1.5 and 3 M☉), and …

We provide here a significant extension of the NuGrid Set 1 models in mass coverage and
towards lower metallicity, adopting the same physics assumptions. The combined data set …

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 …