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Stellar Models with Enhanced Abundances of C, N, O, Ne, Na, Mg, Si, S, Ca, and Ti, in Turn, at Constant Helium and Iron Abundances
VandenBerg, Don A; Bergbusch, Peter A; Dotter, Aaron; Ferguson, Jason W; Michaud, Georges; et al. arXiv.org, Jun 8, 2012.You might have access to this document
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