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Integrity report for Exploring the origin of clumpy dust clouds around cool giants. A global 3D RHD model of a dust-forming M-type AGB star

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

arXiv:1902.04074 · pith:2019:DRYIGY6LMTQ2DXHP3R7PE5F7JO

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Paper page arXiv integrity.json bundle.json

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Signed record

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