The s -Process in Massive Stars at Low Metallicity: The Effect of Primary 14 N from Fast Rotating Stars (2008)
Attributed to:
Stellar Astrophysics at Keele
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1086/593350
Publication URI: http://dx.doi.org/10.1086/593350
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2