The importance of $^{22}$Ne($\alpha$, n)$^{25}$Mg as s-process neutron source and the s-process thermometer $^{151}$Sm

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Neutron capture nucleosynthesis provides a sensitive tool for testing He burning scenarios in massive stars as well as in low mass AGB stars. During this phase of stellar evolution nuclei in the mass region between Fe and Bi are producted by the slow neutron capture process ($\emph{s}$-process). Bec...

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Detalles Bibliográficos
Autores principales: Ferrari, A, Leal, L C, Kitis, G, Guber, K H, Cox, J, Quaranta, A, Koehler, P E
Lenguaje:eng
Publicado: 2002
Acceso en línea:http://cds.cern.ch/record/5848

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