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Integrity report for The chemical composition of the Orion star-forming region. III. C, N, Ne, Mg and Fe abundances in B-type stars revisited

A machine-verified record of the checks Pith has run against this paper: detector runs, findings, signed bundle events, and canonical identifiers.

arXiv:1104.3154 · pith:2011:LAZHEJKKXTB2OEVVWJ5TKCRQRI

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Paper page arXiv integrity.json bundle.json

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Signed record

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