The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. Unfortunately the reaction rate of the 18F(p,a)15O reaction is still largely uncertain due to the unknown strengths of low-lying proton resonances near the 18F+p threshold which play an important role in the nova temperature regime. We report here our last results concerning the study of the d(18F,p)19F(alpha)15N transfer reaction. We show in particular that these two low-lying resonances cannot be neglected. These results are then used to perform a careful study of the remaining uncertainties associated to the 18F(p,a)15O and 18F(p,g)19Ne reaction rates. Comment: 18 pages, 8 figures. Accepted in Nuclear Physics
7 pages, 4 figures, 2 tables, expérience GANIL/SPIRALThe most intense gamma-ray line observable from...
The 18F(p,alpha) reaction was recognized as one of the most important for gamma ray astronomy in nov...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
18 pages, 8 figures. Accepted in Nuclear Physics AThe early E $\leq$ 511 keV gamma-ray emission from...
The 18F(p,alpha)15O reaction is recognized to be one of the most important reactions for nova gamma-...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The ^18F(p, alpha)^15O reaction is recognized as one of the most important reaction for nova gamma-r...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
Context. Direct observation of ¿-ray emission from the decay of 18F ejected in classical nova outbur...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
7 pages, 4 figures, 2 tables, expérience GANIL/SPIRALThe most intense gamma-ray line observable from...
The 18F(p,alpha) reaction was recognized as one of the most important for gamma ray astronomy in nov...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
18 pages, 8 figures. Accepted in Nuclear Physics AThe early E $\leq$ 511 keV gamma-ray emission from...
The 18F(p,alpha)15O reaction is recognized to be one of the most important reactions for nova gamma-...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The ^18F(p, alpha)^15O reaction is recognized as one of the most important reaction for nova gamma-r...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
Context. Direct observation of ¿-ray emission from the decay of 18F ejected in classical nova outbur...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
7 pages, 4 figures, 2 tables, expérience GANIL/SPIRALThe most intense gamma-ray line observable from...
The 18F(p,alpha) reaction was recognized as one of the most important for gamma ray astronomy in nov...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...