The s-process in massive stars at low metallicity: The effect of primary 14N from fast rotating stars

Astrophysical Journal

Volumn 687, Issue 2, 2008, Pages

  Pignatari, M ^a,b   Gallino, R ^c,d   Meynet, G ^e   Hirschi, R ^a,f   Herwig, F ^a,g   Wiescher, M ^b  

^a KEELE UNIVERSITY   (United Kingdom)

^b UNIVERSITY OF NOTRE DAME   (United States)

^c UNIVERSITY OF TURIN   (Italy)

^d MONASH UNIVERSITY   (Australia)

^e UNIVERSITÉ DE GENÈVE   (Switzerland)

^f UNIVERSITY OF TOKYO   (Japan)

^g UNIVERSITY OF VICTORIA   (Canada)

Author keywords

Abundances stars; Chemically peculiar stars; Early type stars; Rotation; Stars

Indexed keywords

EID: 84871273319     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/593350     Document Type: Article

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