F. Pantaleo

activity

20162026

most citedImproved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNA

76 citations · 596 across the 39 of their papers we have counts for

collaborators

Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2017

Origin of meteoritic stardust unveiled by a revised proton-capture rate of $^{17}$ O

M. Lugaro, A. I. Karakas, C. G. Bruno +34

Stardust grains recovered from meteorites provide high-precision snapshots of the isotopic composition of the stellar environment in which they formed. Attributing their origin to…

astro-ph.SR2016★ 49 cited

$^{22}$ Ne and $^{23}$ Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for $^{22}$ Ne(p, $γ$ ) $^{23}$ Na

A. Slemer, P. Marigo, D. Piatti +36

We investigate the impact of the new LUNA rate for the nuclear reaction $^{22}$ Ne $(p, γ)^{23}$ Na on the chemical ejecta of intermediate-mass stars, with particular focus on the ther…

astro-ph.SR2016★ 32 cited

The impact of the revised $^{17}$ O $(p, α)^{14}$ N reaction rate on $^{17}$ O stellar abundances and yields

O. Straniero, C. G. Bruno, M. Aliotta +33

Context. Material processed by the CNO cycle in stellar interiors is enriched in 17O. When mixing processes from the stellar surface reach these layers, as occurs when stars become…

Origin of meteoritic stardust unveiled by a revised proton-capture rate of 17O

22Ne and 23Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for 22Ne(p,γ)23Na

The impact of the revised 17O(p,α)14N reaction rate on 17O stellar abundances and yields

Origin of meteoritic stardust unveiled by a revised proton-capture rate of $^{17}$ O

$^{22}$ Ne and $^{23}$ Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for $^{22}$ Ne(p, $γ$ ) $^{23}$ Na

The impact of the revised $^{17}$ O $(p, α)^{14}$ N reaction rate on $^{17}$ O stellar abundances and yields