Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model predictions of light curves from type I x-ray bursts and the amount of the observable radioisotope F18 produced in classical novae, respectively. To address these uncertainties, we have studied the nuclear structure of Ne19 over Ex=4.0-5.1 and 6.1-7.3 MeV using the F19(He3,t)Ne19 reaction. We find the Jp values of the 4.14- and 4.20-MeV levels to be consistent with 9/2- and 7/2-, respectively, in contrast to previous assumptions. We confirm the recently observed triplet of states around 6.4 MeV and find evidence that the state at 6.29 MeV, just below the proton threshold, is either broad or a doublet. Our data also suggest that predicted but ...
International audienceThe main source of gamma ray emission from novae below 511 keV is likely to be...
The rates of the F-18 (p, alpha)O-15 and F-18(p, gamma)Ne-19 reactions in astrophysical environments...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
Background: Classical novae result from thermonuclear explosions producing several γ-ray emitters wh...
Background: Ne19 is an important isotope in nuclear astrophysics due to its role in both the F18(p,α...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
18 pages, 8 figures. Accepted in Nuclear Physics AThe early E $\leq$ 511 keV gamma-ray emission from...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
International audienceClassical novae result from thermonuclear explosions producing several $\gamma...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
Context. Direct observation of ¿-ray emission from the decay of 18F ejected in classical nova outbur...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
The Ne19(p,γ)Na20 reaction is the second step of a reaction chain which breaks out from the hot CNO ...
International audienceThe main source of gamma ray emission from novae below 511 keV is likely to be...
The rates of the F-18 (p, alpha)O-15 and F-18(p, gamma)Ne-19 reactions in astrophysical environments...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
Uncertainties in the thermonuclear rates of the O15(a,¿)19Ne and 18F(p,a)15O reactions affect model ...
Background: Classical novae result from thermonuclear explosions producing several γ-ray emitters wh...
Background: Ne19 is an important isotope in nuclear astrophysics due to its role in both the F18(p,α...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...
The degree to which the (p, gamma) and (p, alpha) reactions destroy F-18 at temperatures (1-4) x 10(...
18 pages, 8 figures. Accepted in Nuclear Physics AThe early E $\leq$ 511 keV gamma-ray emission from...
The degree to which the (p,gamma) and (p,alpha) reactions destroy 18F at temperatures 1-4x10^8 K is ...
International audienceClassical novae result from thermonuclear explosions producing several $\gamma...
[Context] Direct observation of γ-ray emission from the decay of 18F ejected in classical nova outbu...
Context. Direct observation of ¿-ray emission from the decay of 18F ejected in classical nova outbur...
The main source of gamma ray emission from novae below 511 keV is likely to be associated with the β...
The Ne19(p,γ)Na20 reaction is the second step of a reaction chain which breaks out from the hot CNO ...
International audienceThe main source of gamma ray emission from novae below 511 keV is likely to be...
The rates of the F-18 (p, alpha)O-15 and F-18(p, gamma)Ne-19 reactions in astrophysical environments...
The early E < 511 keV gamma-ray emission from novae depends critically on the 18F(p,a)15O reaction. ...