Add to ORKGAbout half of the solar abundances of elements heavier than iron are made by the slow neutron capture process (the s process) occurring in low and intermediate-mass asymptotic giant branch (AGB) stars. Elements are dredged from the core to the surface an
The intermediate neutron-capture process is thought to arise when protons are mixed in a convective ...
Asymptotic giant branch (AGB) stars are a main site of production of nuclei heavier than iron via th...
The intermediate neutron-capture process is thought to arise when protons are mixed in a convective ...
Approximately half of the solar abundances of nuclei heavier than iron are created in the deep layer...
Asymptotic giant branch (AGB) stars are responsible for the production of the main component of the ...
Asymptotic giant branch (AGB) stars are responsible for the production of the main component of the ...
Asymptotic giant branch (AGB) stars are initially low and intermediate mass stars undergoing recurre...
Aims. We explore modifications to the current scenario for the slow neutron-capture proces...
Spectroscopic observations of stars belonging to open clusters, with well-determined ages and distan...
Observations of planetary nebulae have revealed a wealth of information about the composition of hea...
Context. Barium (Ba) stars are dwarf and giant stars enriched in elements heavier than iron produce...
We attempt to study the ability of asymptotic giant branch stars to produce s-process elements as a ...
We attempt to study the ability of asymptotic giant branch stars to produce s-process elements as a ...
We find that galactic disk objects are reproduced by a spread of a factor of two in the effectivenes...
In this review, we discuss the impact of s-process nucleosynthesis in asymptotic giant branch stars ...
The intermediate neutron-capture process is thought to arise when protons are mixed in a convective ...
Asymptotic giant branch (AGB) stars are a main site of production of nuclei heavier than iron via th...
The intermediate neutron-capture process is thought to arise when protons are mixed in a convective ...
Approximately half of the solar abundances of nuclei heavier than iron are created in the deep layer...
Asymptotic giant branch (AGB) stars are responsible for the production of the main component of the ...
Asymptotic giant branch (AGB) stars are responsible for the production of the main component of the ...
Asymptotic giant branch (AGB) stars are initially low and intermediate mass stars undergoing recurre...
Aims. We explore modifications to the current scenario for the slow neutron-capture proces...
Spectroscopic observations of stars belonging to open clusters, with well-determined ages and distan...
Observations of planetary nebulae have revealed a wealth of information about the composition of hea...
Context. Barium (Ba) stars are dwarf and giant stars enriched in elements heavier than iron produce...
We attempt to study the ability of asymptotic giant branch stars to produce s-process elements as a ...
We attempt to study the ability of asymptotic giant branch stars to produce s-process elements as a ...
We find that galactic disk objects are reproduced by a spread of a factor of two in the effectivenes...
In this review, we discuss the impact of s-process nucleosynthesis in asymptotic giant branch stars ...
The intermediate neutron-capture process is thought to arise when protons are mixed in a convective ...
Asymptotic giant branch (AGB) stars are a main site of production of nuclei heavier than iron via th...
The intermediate neutron-capture process is thought to arise when protons are mixed in a convective ...