s-Process Elements and Galactic Evolution
نویسندگان
چکیده
منابع مشابه
Galactic chemical evolution of Ba-peak elements
The chemical evolution of the Galaxy is followed for the elements affected by neutron capture, in particular for those in the atomic number range 56 to 63 (Ba, La, Ce, Pr, Nd, Sm and Eu). Neutrons by the major C source, released in radiative conditions in the interpulse periods of TP-AGB stars, give rise to an efficient s-processing, making low mass AGB the major contributors to the chemical ev...
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ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1977
ISSN: 0252-9211
DOI: 10.1017/s0252921100067555