Aurora Tumino
Aurora Tumino
FacoltÓ di Ingegneria e Architettura, UniversitÓ degli Studi di Enna "Kore", Enna and Laboratori
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A companion to AB Pic at the planet/brown dwarf boundary
G Chauvin, AM Lagrange, B Zuckerman, C Dumas, D Mouillet, I Song, ...
Astronomy & Astrophysics 438 (3), L29-L32, 2005
The B 11 (p, α 0) Be 8 reaction at sub-Coulomb energies via the Trojan-horse method
C Spitaleri, L Lamia, A Tumino, RG Pizzone, S Cherubini, A Del Zoppo, ...
Physical Review C 69 (5), 055806, 2004
“Trojan horse” method applied to at astrophysical energies
C Spitaleri, S Typel, RG Pizzone, M Aliotta, S Blagus, M Bogovac, ...
Physical Review C 63 (5), 055801, 2001
The Trojan Horse Method in nuclear astrophysics
C Spitaleri, AM Mukhamedzhanov, LD Blokhintsev, M La Cognata, ...
Physics of Atomic Nuclei 74 (12), 1725-1739, 2011
Search for cluster structure of excited states in 14 C
W Von Oertzen, HG Bohlen, M Milin, T Kokalova, S Thummerer, A Tumino, ...
The European Physical Journal A-Hadrons and Nuclei 21 (2), 193-215, 2004
The Fluorine destruction in stars: first experimental study of the 19F (p, α0) 16O reaction at astrophysical energies
M La Cognata, AM Mukhamedzhanov, C Spitaleri, I Indelicato, M Aliotta, ...
The Astrophysical Journal Letters 739 (2), L54, 2011
Validity test of the “Trojan horse” method applied to the reaction
A Tumino, C Spitaleri, A Di Pietro, P Figuera, M Lattuada, A Musumarra, ...
Physical Review C 67 (6), 065803, 2003
Astrophysical S (E) factor of the N 15 (p, α) C 12 reaction at sub-Coulomb energies via the Trojan horse method
M La Cognata, S Romano, C Spitaleri, S Cherubini, V Crucilla, M Gulino, ...
Physical Review C 76 (6), 065804, 2007
A novel approach to measure the cross section of the 18O (p, α) 15N resonant reaction in the 0-200 keV energy range
M La Cognata, C Spitaleri, A Mukhamedzhanov, A Banu, S Cherubini, ...
The Astrophysical Journal 708 (1), 796, 2009
Measurement of the 20 and 90 keV Resonances in the O 18 (p, α) N 15 Reaction via the Trojan Horse Method
M La Cognata, C Spitaleri, AM Mukhamedzhanov, B Irgaziev, RE Tribble, ...
Physical review letters 101 (15), 152501, 2008
Bare-nucleus astrophysical factor of the He 3 (d, p) He 4 reaction via the “Trojan horse” method
M La Cognata, C Spitaleri, A Tumino, S Typel, S Cherubini, L Lamia, ...
Physical Review C 72 (6), 065802, 2005
An increase in the 12 C+ 12 C fusion rate from resonances at astrophysical energies
A Tumino, C Spitaleri, M La Cognata, S Cherubini, GL Guardo, M Gulino, ...
Nature 557 (7707), 687-690, 2018
Persistent asymmetric structure of Sagittarius A* on event horizon scales
VL Fish, MD Johnson, SS Doeleman, AE Broderick, D Psaltis, RS Lu, ...
The Astrophysical Journal 820 (2), 90, 2016
New determination of the 2H (d, p) 3H and 2H (d, n) 3He reaction rates at astrophysical energies
A Tumino, R Sparta, C Spitaleri, AM Mukhamedzhanov, S Typel, ...
The Astrophysical Journal 785 (2), 96, 2014
Suppression of the Coulomb Interaction in the Off-Energy-Shell p− p Scattering from the p+ d→ p+ p+ n Reaction
A Tumino, C Spitaleri, A Mukhamedzhanov, GG Rapisarda, S Cherubini, ...
Physical review letters 98 (25), 252502, 2007
Low-energy d+ d fusion reactions via the Trojan Horse Method
A Tumino, C Spitaleri, AM Mukhamedzhanov, S Typel, M Aliotta, V Burjan, ...
Physics Letters B 700 (2), 111-115, 2011
New high accuracy measurement of the (,) reaction rate at astrophysical temperatures
ML Sergi, C Spitaleri, M La Cognata, A Coc, A Mukhamedzhanov, ...
Physical Review C 82 (3), 032801, 2010
Big bang nucleosynthesis revisited via Trojan Horse method measurements
RG Pizzone, R Spartß, CA Bertulani, C Spitaleri, M La Cognata, ...
The Astrophysical Journal 786 (2), 112, 2014
Investigation of the -cluster structure of and
VZ Goldberg, GV Rogachev, WH Trzaska, JJ Kolata, A Andreyev, ...
Physical Review C 69 (2), 024602, 2004
An updated 6Li (p, α) 3He reaction rate at astrophysical energies with the Trojan horse method
L Lamia, C Spitaleri, RG Pizzone, E Tognelli, A Tumino, S Degl'Innocenti, ...
The Astrophysical Journal 768 (1), 65, 2013
Il sistema al momento non pu˛ eseguire l'operazione. Riprova pi¨ tardi.
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