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

collaborators
Showing 2016Show all

5 papers · 1 filter

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…

nucl-ex2016★ 17 cited

Shell and explosive hydrogen burning

A. Boeltzig, C. G. Bruno, F. Cavanna +10

The nucleosynthesis of light elements, from helium up to silicon, mainly occurs in Red Giant and Asymptotic Giant Branch stars and Novae. The relative abundances of the synthesized…

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…

nucl-ex2016★ 55 cited

Direct measurement of low-energy Ne(p,)Na resonances

R. Depalo, F. Cavanna, M. Aliotta +30

The Ne(p,)Na reaction is the most uncertain process in the neon-sodium cycle of hydrogen burning. At temperatures relevant for nucleosynthesis in asymptotic giant…

nucl-ex2016★ 76 cited

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

C. G. Bruno, D. A. Scott, M. Aliotta +32

The O(p,)N reaction plays a key role in various astrophysical scenarios, from asymptotic giant branch stars to classical novae. It affects the synthesis of rare is…