most citedOrigin of large meteoritic SiC stardust grains in metal-rich AGB stars

35 citations · 55 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.SR202020 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…

astro-ph.SR202035 cited

Origin of large meteoritic SiC stardust grains in metal-rich AGB stars

Maria Lugaro, Borbála Cseh, Blanka Világos +16

Stardust grains that originated in ancient stars and supernovae are recovered from meteorites and carry the detailed composition of their astronomical sites of origin. We present e…

nucl-ex2020

Re-evaluation of the Ne()Mg and Ne()Mg reaction rates

Philip Adsley, Umberto Battino, Andreas Best +11

The competing Ne()Mg and Ne()Mg reactions control the production of neutrons for the weak -process in massive and AGB stars. In both system…

astro-ph.SR2019

The s process in rotating low-mass AGB stars. Nucleosynthesis calculations in models matching asteroseismic constraints

J. W. den Hartogh, R. Hirschi, M. Lugaro +5

Aims. We investigate the s-process during the AGB phase of stellar models whose cores are enforced to rotate at rates consistent with asteroseismology observations of their progeni…

astro-ph.SR2019

NuGrid stellar data set - III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z=0.01, Z=0.02 and Z=0.03

Umberto Battino, Ashley Tattersall, Claudia Lederer-Woods +6

The production of the neutron-capture isotopes beyond iron that we observe today in the solar system is the result of the combined contribution of the r-process, the s- process and…