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Did you mean: person:("F. ferrari")
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Valoración de los servicios ecosistémicos urbanos desde un enfoque interdisciplinario
Free accessDOAJ | 2022| -
ChAMBRe: a new atmospheric simulation chamber for aerosol modelling and bio-aerosol research
Free accessDOAJ | 2018| -
The Study of Key Reactions Shaping the Post-Main Sequence Evolution of Massive Stars in Underground Facilities
Free accessBASE | 2021|Contributors: F. Ferraro -
A new study of the 22Ne(p,gamma)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance
Free accessBASE | 2014|Contributors: F. Ferraro -
Effect of beam energy straggling on resonant yield in thin gas targets: The cases 22Ne(p, γ)23Na and 14N(p, γ)15O
LetterIOP Institute of Physics | 2018| -
22Ne and 23Na ejecta from intermediate-mass stars: the impact of the new LUNA rate for 22Ne(p,γ)23Na
Free accessBASE | 2017|Contributors: F. Ferraro -
Improved astrophysical rate for the 18O(p,α)15N reaction by underground measurements
Free accessDOAJ | 2019| -
The impact of the revised 17O(p; alpha)14N reaction rate on 17O stellar abundances and yields
Free accessBASE | 2017|Contributors: F. Ferraro -
Improved background suppression for radiative capture reactions at LUNA with HPGe and BGO detectors
PaperIOP Institute of Physics | 2018| -
Direct measurements of low-energy resonance strengths of the 23Na(p,γ)24Mg reaction for astrophysics
Free accessDOAJ | 2019| -
Direct measurements of low-energy resonance strengths of the 23Na(p,γ)24Mg reaction for astrophysics
Free accessBASE | 2019| -
Direct Measurement of the 13C(α,n)16O Cross Section into the s-Process Gamow Peak
Free accessBASE | 2021| -
First direct limit on the 334 keV resonance strength in $$^{22}$$Ne($$\alpha $$,$$\gamma $$)$$^{26}$$Mg reaction [First direct limit on the 334 keV resonance strength in Ne-22(alpha, gamma)Mg-26 reaction]
Free accessBASE | 2022|Contributors: F. Ferraro
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