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The ^(26)Al(^3He,d)^(27)Si reaction was measured from 0°≤θ_(c.m.)≤35° at E(^3He)=20 MeV using a quadrupole-dipole-dipole-dipole magnetic spectrometer. States in ^(27)Si were observed above the background at 7652 and 7741 keV and upper limits were set for the state at 7592 keV. Implications for the ^(26)Al(p,γ)^(27)Si stellar reaction rate are discussed
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
The ^(26)Al(^3He,d)^(27)Si reaction was measured from 0°≤θ_(c.m.)≤35° at E(^3He)=20 MeV using a quad...
The ^(26)Al(^3He,d)^(27)Si reaction was measured from 0°≤θ_(c.m.)≤35° at E(^3He)=20 MeV using a quad...
The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipo...
The rate of the $$^{25}$$Al(p, $$\gamma $$)$$^{26}$$Si reaction is one of the few key remaining nucl...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
The heavy-ion, fusion-evaporation reaction C12(O16,n) was used to identify γ-decay transitions from ...
The heavy-ion, fusion-evaporation reaction C12(O16,n) was used to identify γ-decay transitions from ...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
The ^(26)Al(^3He,d)^(27)Si reaction was measured from 0°≤θ_(c.m.)≤35° at E(^3He)=20 MeV using a quad...
The ^(26)Al(^3He,d)^(27)Si reaction was measured from 0°≤θ_(c.m.)≤35° at E(^3He)=20 MeV using a quad...
The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipo...
The rate of the $$^{25}$$Al(p, $$\gamma $$)$$^{26}$$Si reaction is one of the few key remaining nucl...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
The heavy-ion, fusion-evaporation reaction C12(O16,n) was used to identify γ-decay transitions from ...
The heavy-ion, fusion-evaporation reaction C12(O16,n) was used to identify γ-decay transitions from ...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
Since the identification of ongoing Al-26 production in the universe, the reaction sequence Mg-24(p,...
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