U. Battino

activity

20132026

most citedNuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z = 0.02 and Z = 0.01

230 citations · 742 across the 17 of their papers we have counts for

collaborators

Showing 2020Show all

3 papers · 1 filter

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…

astro-ph.SR2020★ 35 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★ 58 cited

Re-evaluation of the $^{22}$ Ne( $α, γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α, n$ ) $^{25}$ Mg reaction rates

Philip Adsley, Umberto Battino, Andreas Best +11

The competing $^{22}$ Ne( $α, γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α, n$ ) $^{25}$ Mg reactions control the production of neutrons for the weak $s$ -process in massive and AGB stars. In both system…

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

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

Re-evaluation of the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates

Re-evaluation of the $^{22}$ Ne( $α, γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α, n$ ) $^{25}$ Mg reaction rates