Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-shell burning. In particular, the strengths of low-energy resonances with E<200 keV in 25Mg(p,γ)26Al determine the production of 26Al and a precise knowledge of these nuclear data is highly desirable. Absolute measurements at such low energies are often very difficult and hampered by γ-ray background as well as changing target stoichiometry during the measurements. The latter problem can be partly avoided using higher-energy resonances of the same reaction as a normalization reference. Hence the parameters of suitable resonances have to be studied with adequate precision. In the present work we report on new measurements of the resonance strengths ω...
Background: The Ne22(p,γ)Na23 reaction is the most uncertain process in the neon-sodium cycle of hyd...
Background: Shell hydrogen burning during the asymptotic giant branch (AGB) phase through the oxygen...
The γ-decay properties of an excited state in 26Al at 6398.3(8) keV have been reexamined using the 1...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-shell b...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-shell b...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-burning...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-burning...
The NeNa and the MgAl cycles play a fundamental role in the nucleosynthesis of asymptotic giant bran...
The cosmic 1.809 MeV γ-ray emitted by the radioactive nucleus 26Al in the Galaxy is one of the key o...
The COMPTEL instrument performed the first mapping of the 1.809 MeV photons in the Galaxy, triggerin...
In the present work we report on a new measurement of resonance strengths ωγ in the reaction 25Mg(p...
Resonace strengths of selected resonances in the Ep=0.3−2.1 MeV region in the (p, γ) reactions on 23...
Gamma-ray decay schemes have been measured with bare and Compton-suppressed Ge detectors at low-ener...
Background: The Ne22(p,γ)Na23 reaction is the most uncertain process in the neon-sodium cycle of hyd...
Background: Shell hydrogen burning during the asymptotic giant branch (AGB) phase through the oxygen...
The γ-decay properties of an excited state in 26Al at 6398.3(8) keV have been reexamined using the 1...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-shell b...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-shell b...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-burning...
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-burning...
The NeNa and the MgAl cycles play a fundamental role in the nucleosynthesis of asymptotic giant bran...
The cosmic 1.809 MeV γ-ray emitted by the radioactive nucleus 26Al in the Galaxy is one of the key o...
The COMPTEL instrument performed the first mapping of the 1.809 MeV photons in the Galaxy, triggerin...
In the present work we report on a new measurement of resonance strengths ωγ in the reaction 25Mg(p...
Resonace strengths of selected resonances in the Ep=0.3−2.1 MeV region in the (p, γ) reactions on 23...
Gamma-ray decay schemes have been measured with bare and Compton-suppressed Ge detectors at low-ener...
Background: The Ne22(p,γ)Na23 reaction is the most uncertain process in the neon-sodium cycle of hyd...
Background: Shell hydrogen burning during the asymptotic giant branch (AGB) phase through the oxygen...
The γ-decay properties of an excited state in 26Al at 6398.3(8) keV have been reexamined using the 1...