First inverse kinematics study of the \(^{22}\)Ne\((p,\gamma)^{23}\)Na reaction and its role in AGB...
First inverse kinematics study of the \(^{22}\)Ne\((p,\gamma)^{23}\)Na reaction and its role in AGB star and classical nova nucleosynthesis
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Author / Creator
Williams, M , Lennarz, A , Laird, A M , Battino, U , Connolly, J José D , Ruiz, C , Chen, A , Davids, B , Esker, N , Fulton, B R , Garg, R , Gay, x M , Greife, U , Hager, U , Hutcheon, D , Lovely, M , Lyons, S , Psaltis, A , Riley, J E and Tattersall, A
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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The abundances of sodium and oxygen are observed to be anti-correlated in all well-studied globular clusters. Asymptotic giant branch (AGB) stars undergoing hot bottom burning (HBB) are thought to be prime candidates for producing sodium-rich oxygen-poor material and expelling it into the cluster ISM. The 22Ne(p,gamma)23Na reaction has been shown t...
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Full title
First inverse kinematics study of the \(^{22}\)Ne\((p,\gamma)^{23}\)Na reaction and its role in AGB star and classical nova nucleosynthesis
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TN_cdi_proquest_journals_2301669411
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2301669411
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1910.01698
