Stars are marvellous caldrons where all the elements of the Universe (apartfrom hydrogen and helium) have been synthesized. The solar system chemical distri-butionis the result of many pollution episodes from already extinct stellar generations, occurred at different epochs before the Sun formation. Main nucleosynthesis channels re-sponsiblefor the formation of heavy elements are the rapid neutron capture process (ther-process) and the slow neutron capture process (the s-process). Hereafter, I will describethe theory of the s-process and the stellar sites where it is active
In order to investigate the site of processes and cosmochronology, ratio between three processes hav...
We attempt to study the ability of asymptotic giant branch stars to produce s-process elements as a ...
Neutron reactions are responsible for the formation of the elements heavier than iron. The correspon...
Stars are marvellous caldrons where all the elements of the Universe (apartfrom hydrogen and helium)...
200 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 1982.A detailed analysis is undert...
In this thesis we shall treat the astrophysical origin of the s-process. The subject, that can at f...
We apply the analytical model developed previously to the Galactic chemical evolution of elements th...
This contribution deals with the important subject of the nucleosynthesis of heavy elements in the G...
Neutron reactions are responsible for the formation of the elements heavier than iron. The correspon...
This article addresses three of the four nucleosynthesis processes involved in producing heavy nucle...
We outline a partial historical summary of the steps through which the nucleosynthesis phenomena ind...
We present a comprehensive study of s-process nucleosynthesis in 15, 20, 25, and 30 $\msun$ stellar ...
About half of the solar abundances of elements heavier than iron are made by the slow neutron captur...
We review the history and the present status of the s-process and point to problems in need of clari...
Observations of planetary nebulae have revealed a wealth of information about the composition of hea...
In order to investigate the site of processes and cosmochronology, ratio between three processes hav...
We attempt to study the ability of asymptotic giant branch stars to produce s-process elements as a ...
Neutron reactions are responsible for the formation of the elements heavier than iron. The correspon...
Stars are marvellous caldrons where all the elements of the Universe (apartfrom hydrogen and helium)...
200 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 1982.A detailed analysis is undert...
In this thesis we shall treat the astrophysical origin of the s-process. The subject, that can at f...
We apply the analytical model developed previously to the Galactic chemical evolution of elements th...
This contribution deals with the important subject of the nucleosynthesis of heavy elements in the G...
Neutron reactions are responsible for the formation of the elements heavier than iron. The correspon...
This article addresses three of the four nucleosynthesis processes involved in producing heavy nucle...
We outline a partial historical summary of the steps through which the nucleosynthesis phenomena ind...
We present a comprehensive study of s-process nucleosynthesis in 15, 20, 25, and 30 $\msun$ stellar ...
About half of the solar abundances of elements heavier than iron are made by the slow neutron captur...
We review the history and the present status of the s-process and point to problems in need of clari...
Observations of planetary nebulae have revealed a wealth of information about the composition of hea...
In order to investigate the site of processes and cosmochronology, ratio between three processes hav...
We attempt to study the ability of asymptotic giant branch stars to produce s-process elements as a ...
Neutron reactions are responsible for the formation of the elements heavier than iron. The correspon...