The Fe group nuclei ^54Cr, ^58Fe, and ^64Ni are readily produced in AGB stars during "s" processing. These nuclides do not require SNe production. ...
Isotopic Anomalies in Cr, Fe and Ni from ``s'' Processing in AGB Stars
Busso, M.
Investigation
2015
Abstract
The Fe group nuclei ^54Cr, ^58Fe, and ^64Ni are readily produced in AGB stars during "s" processing. These nuclides do not require SNe production. ...File in questo prodotto:
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