Gamma-ray decay schemes have been measured with bare and Compton-suppressed Ge detectors at low-energy resonances (EP < 340 keV) in the (p, γ) reactions on 25Mg, 26Mg and 27Al. Altogether 58 new decay branches have been observed and a new 26Mg(p, γ)27Al resonance has been found at EP = 154.5 ± 1.0 keV. The new branchings lead to Jπ; T determinations (or limitations) for two states in 26Al and four states in 28Si. The absolute strengths of the 25Mg(p, γ)26Al and 26Mg(p, γ)27Al resonances have also been obtained, and the uncertainties of the stellar rates, deduced from the available data for both reactions, are significantly reduced. Some astrophysical consequences are discussed. © 1990.SCOPUS: ar.jinfo:eu-repo/semantics/publishe
The 26mAl(p,γ)27Si reaction is thought have a significant impact of the nucleosynthesis of both 26Mg...
The \u3b3-decays of eleven resonances in the 28Si(\u3b1,\u3b3)32S reaction below E\u3b1 = 3.83 MeV h...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
A gamma-ray spectroscopy study of ;{26g}Al+p resonant states in 27Si is presented. Excitation energi...
The gamma-ray spectra from twelve 27Al(p, γ)28Si resonances in the Ep = 500 to 800 keV region were i...
The gamma-ray spectra of thirty 26Mg(p, γ)27Al resonances in the range Ep = 0.3−2.8 MeV, were measur...
The γ-decay properties of an excited state in 26Al at 6398.3(8) keV have been reexamined using the 1...
The astrophysical 25Al(p,γ) 26Si reaction represents one of the key remaining uncertainties in accur...
The COMPTEL instrument performed the first mapping of the 1.809 MeV photons in the Galaxy, triggerin...
The astrophysical 25Al(p,γ)26Si reaction represents one of the key remaining uncertainties in accura...
The yield of 8–13 MeV γ radiation from the 24Mg(α, γ)28Si reaction has been measured in the Eα = 1.2...
The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipo...
The measurements described in the preceding paper (I) are used to obtain the position, spin and isob...
The creation site of 26Al is still under debate. It is thought to be produced in hydrogen burning an...
The reactions 26Alg(p,γ)27Si and 26Alm(p,γ)27Si are important for influencing the galactic abundance...
The 26mAl(p,γ)27Si reaction is thought have a significant impact of the nucleosynthesis of both 26Mg...
The \u3b3-decays of eleven resonances in the 28Si(\u3b1,\u3b3)32S reaction below E\u3b1 = 3.83 MeV h...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...
A gamma-ray spectroscopy study of ;{26g}Al+p resonant states in 27Si is presented. Excitation energi...
The gamma-ray spectra from twelve 27Al(p, γ)28Si resonances in the Ep = 500 to 800 keV region were i...
The gamma-ray spectra of thirty 26Mg(p, γ)27Al resonances in the range Ep = 0.3−2.8 MeV, were measur...
The γ-decay properties of an excited state in 26Al at 6398.3(8) keV have been reexamined using the 1...
The astrophysical 25Al(p,γ) 26Si reaction represents one of the key remaining uncertainties in accur...
The COMPTEL instrument performed the first mapping of the 1.809 MeV photons in the Galaxy, triggerin...
The astrophysical 25Al(p,γ)26Si reaction represents one of the key remaining uncertainties in accura...
The yield of 8–13 MeV γ radiation from the 24Mg(α, γ)28Si reaction has been measured in the Eα = 1.2...
The 26Al(3He,d)27Si reaction was measured from 0°≤θc.m.≤35° at E(3He)=20 MeV using a quadrupole-dipo...
The measurements described in the preceding paper (I) are used to obtain the position, spin and isob...
The creation site of 26Al is still under debate. It is thought to be produced in hydrogen burning an...
The reactions 26Alg(p,γ)27Si and 26Alm(p,γ)27Si are important for influencing the galactic abundance...
The 26mAl(p,γ)27Si reaction is thought have a significant impact of the nucleosynthesis of both 26Mg...
The \u3b3-decays of eleven resonances in the 28Si(\u3b1,\u3b3)32S reaction below E\u3b1 = 3.83 MeV h...
International audienceThe Galactic 1.809-MeV γ-ray signature from the β decay of $^{26g}$Al is a dom...