Synthesis of the elements in stars: forty years of progress
G Wallerstein, I Iben, P Parker, AM Boesgaard… - Reviews of Modern …, 1997 - APS
Abstract Forty years ago Burbidge, Burbidge, Fowler, and Hoyle combined what we would
now call fragmentary evidence from nuclear physics, stellar evolution and the abundances …
now call fragmentary evidence from nuclear physics, stellar evolution and the abundances …
The evolution of CNO elements in galaxies
D Romano - The Astronomy and Astrophysics Review, 2022 - Springer
After hydrogen and helium, oxygen, carbon, and nitrogen—hereinafter, the CNO elements—
are the most abundant species in the universe. They are observed in all kinds of …
are the most abundant species in the universe. They are observed in all kinds of …
A new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase
We introduce a new generation of PARSEC–COLIBRI stellar isochrones that includes a
detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB) phase …
detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB) phase …
The Dawes review 2: nucleosynthesis and stellar yields of low-and intermediate-mass single stars
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 …
Stellar yields from metal-rich asymptotic giant branch models
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 …
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 …
(4.0, 5.0, and 6.0 M⊙) at different metallicities (− 2.15≤[Fe/H]≤+ 0.15). This set integrates …
Evolution of low-and intermediate-mass stars to the end of the asymptotic giant branch with mass loss
E Vassiliadis, PR Wood - … Journal, Part 1 (ISSN 0004-637X) …, 1993 - adsabs.harvard.edu
The results of stellar evolution calculations from the main sequence through to the end of the
asymptotic giant branch (AGB) phase with mass loss are presented. It is shown that typical …
asymptotic giant branch (AGB) phase with mass loss are presented. It is shown that typical …
Evolution of asymptotic giant branch stars-II. Optical to far-infrared isochrones with improved tp-agb models
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) …
the greatly-improved treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) …
[BOG][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 …
explosion in the literature and many review articles, there had not been one since that of …
[BOG][B] Evolution of stars and stellar populations
M Salaris, S Cassisi - 2005 - books.google.com
Evolution of Stars and Stellar Populations is a comprehensive presentation of the theory of
stellar evolution and its application to the study of stellar populations in galaxies. Taking a …
stellar evolution and its application to the study of stellar populations in galaxies. Taking a …