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Classical-Nova Contribution to the Milky Way's \(^{26}\)Al Abundance: Exit Channel of the Key \(^{25}\)Al(\(p,\gamma\))\(^{26}\)Si Resonance
Bennett, M B; Wrede, C; Chipps, K A; José, J; Liddick, S N; et al. arXiv.org, Dec 12, 2013.You might have access to this document
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