activity
20242026
collaborators
Showing astro-ph.SRShow all

16 papers · 1 filter

astro-ph.SR2026

Stellar Interpretation of Meteoritic Data and PLotting for Everyone (SIMPLE): Isotope Mixing Lines for Six Sets of Core-Collapse Supernova Models

Marco Pignatari, Mattias Ek, Georgy V. Makhatadze +15

Bulk meteorites and their inclusions exhibit, for many chemical elements, isotopic variability produced by nucleosynthetic events in stars and supernovae before the formation of th…

astro-ph.SR2026

The NuGrid AGB Evolution and Nucleosynthesis Data Set

Umberto Battino, Marco Pignatari, Ashley Tattersall +2

Asymptotic Giant Branch (AGB) stars play a key role in the chemical evolution of galaxies. These stars are the fundamental stellar site for the production of light elements such as…

astro-ph.SR2026

Impact of newly measured 26Al(n, p)26Mg and 26Al(n, α)23Na reaction rates on the nucleosynthesis of 26Al in stars

Umberto Battino, Claudia Lederer-Woods, Marco Pignatari +6

The cosmic production of the short-lived radioactive nuclide 26Al is crucial for our understanding of the evolution of stars and galaxies. However, simulations of the stellar sites…

astro-ph.SR2025

3D Macro Physics and Light Odd-Z Element Production in O-C Shell Mergers: Implications for production and radiogenic heating inventories of rocky exoplanets

Joshua Issa, Falk Herwig, Stephen J. Mojzsis +1

The light odd-Z elements P, Cl, K, and Sc are underproduced in galactic chemical evolution models compared to spectroscopic observations of stars in the Milky Way. The most promisi…

astro-ph.SR2025

Impact of 3D macro physics and nuclear physics on the p nuclei in O-C shell mergers

Joshua Issa, Falk Herwig, Pavel Denissenkov +1

O-C shell mergers in massive stars are a site for producing the p nuclei by the process, but 1D stellar models rely on mixing length theory, which does not match the radial ve…

astro-ph.SR2025

Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution

Emma Kotar, Shuya Ota, Allyson Dewey +3

In massive stars (initial mass of > 9 solar masses), the weak s (slow neutron capture) process produces elements between Fe and Zr, enriching the Galaxy with these elements through…