S-process nucleosynthesis in low mass AGB Stars: Do we really need an improved determination of the 13C(α, n)16O reaction rate?

Nuclear Physics A

Volumn 758, Issue 1-4 SPEC. ISS., 2005, Pages 509-512

  Cristallo, S ^a   Straniero, O ^a   Gallino, R ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^b UNIVERSITY OF TURIN   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 20944432610     PISSN: 03759474     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.nuclphysa.2005.05.181     Document Type: Article

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