58 citations · 226 across the 11 of their papers we have counts for
11 papers
Characterization of the LUNA neutron detector array for the measurement of the 13C(a,n)16O reaction
L. Csedreki, G. F. Ciani, J. Balibrea-Correa +46
We introduce the LUNA neutron detector array developed for the investigation of the 13C(a,n)16O reaction towards its astrophysical s-process Gamow peak in the low-background enviro…
Stellar Population Astrophysics (SPA) with TNG, Fluorine abundances in seven open clusters
Shilpa Bijavara Seshashayana, Henrik Jönsson, Valentina D'Orazi +9
The age, evolution, and chemical properties of the Galactic disk can be effectively ascertained using open clusters. Within the large program Stellar Populations Astrophysics at th…
First direct limit on the 334 keV resonance strength in the Ne(α,γ)Mg reaction
D. Piatti, E. Masha, M. Aliotta +44
In stars, the fusion of Ne and He may produce either Mg, with the emission of a neutron, or Mg and a ray. At high temperature, the () channel domi…
The Radioactive Nuclei Al and Fe in the Cosmos and in the Solar System
Roland Diehl, Maria Lugaro, Alexander Heger +15
The cosmic evolution of the chemical elements from the Big Bang to the present time is driven by nuclear fusion reactions inside stars and stellar explosions. A cycle of matter rec…
The Gaia-ESO Survey: A new approach to chemically characterising young open clusters II. Abundances of the neutron-capture elements Cu, Sr, Y, Zr, Ba, La, and Ce
M. Baratella, V. D'Orazi, V. Sheminova +32
Young open clusters (t<200 Myr) have been observed to exhibit several peculiarities in their chemical compositions, from a slightly sub-solar iron content, super-solar abundances o…
129I and 247Cm in Meteorites Constrain the Last Astrophysical Source of Solar r-process Elements
Benoit Côté, Marius Eichler, Andrés Yagüe +12
The composition of the early Solar System can be inferred from meteorites. Many elements heavier than iron were formed by the rapid neutron-capture process (r process), but the ast…