activity
20122026
most citedImproved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNA

76 citations · 615 across the 18 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2017

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

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

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

We investigate the impact of the new LUNA rate for the nuclear reaction NeNa on the chemical ejecta of intermediate-mass stars, with particular focus on the ther…

astro-ph.SR2016★ 32 cited

The impact of the revised ON reaction rate on 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…

astro-ph.SR2014★ 48 cited

Effects of nuclear cross sections on F nucleosynthesis at low metallicities

S. Cristallo, A. Di Leva, G. Imbriani +4

The origin of fluorine is a longstanding problem in nuclear astrophysics. It is widely recognized that Asymptotic Giant Branch (AGB) stars are among the most important contributors…

astro-ph.SR2012★ 58 cited

First Direct Measurement of the ^{17}O(p,γ)^{18}F Reaction Cross-Section at Gamow Energies for Classical Novae

D. A. Scott, A. Caciolli, A. DiLeva +29

Classical novae are important contributors to the abundances of key isotopes, such as the radioactive ^{18}F, whose observation by satellite missions could provide constraints on n…