activity
19982026
most citedNucleosynthesis and mixing on the Asymptotic Giant Branch. III. Predicted and observed s-process abundances

431 citations · 3.5k across the 42 of their papers we have counts for

collaborators

42 papers

astro-ph.SR2026★ 1 cited

Slow White Dwarf Mergers as a New Galactic Source of Trans-Iron Elements

Umberto Battino, Claudia Lederer-Woods, Claudia Travaglio +2

The astrophysical origins of the heaviest stable elements that we observe today in the Solar System are still not fully understood. Recent studies have demonstrated that H-accretin…

astro-ph.SR2025

Trans-Fe elements from Type Ia Supernovae. I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs

Umberto Battino, James Keegans, Megan Allen +9

Type Ia supernovae (SNIa) are thermonuclear explosions of white dwarfs in binary systems. They are central to galactic chemical evolution and serve as standardizable candles in cos…

astro-ph.HE2023★ 15 cited

Type Ia Supernova Nucleosynthesis: Metallicity-Dependent Yields

James D Keegans, Marco Pignatari, Richard J Stancliffe +7

Type Ia supernova explosions (SNIa) are fundamental sources of elements for the chemical evolution of galaxies. They efficiently produce intermediate-mass (with Z between 11 and 20…

nucl-ex2022★ 51 cited

Horizons: Nuclear Astrophysics in the 2020s and Beyond

H. Schatz, A. D. Becerril Reyes, A. Best +162

Nuclear Astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the…

nucl-ex2021★ 8 cited

Measurement of the 91Zr(p,gamma)92mNb cross section motivated by type Ia supernova nucleosynthesis

Gy. Gyürky, Z. Halász, G. G. Kiss +6

The synthesis of heavy, proton rich isotopes is a poorly understood astrophysical process. Thermonuclear (type Ia) supernova explosions are among the suggested sites and the abunda…

astro-ph.SR2020★ 20 cited

Heavy Elements Nucleosynthesis On Accreting White Dwarfs: building seeds for the p-process

Umberto Battino, Marco Pignatari, Claudia Travaglio +5

The origin of the proton-rich trans-iron isotopes in the solar system is still uncertain. Single-degenerate thermonuclear supernovae (SNIa) with n-capture nucleosynthesis seeds ass…