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Integrity report for Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars

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

arXiv:0909.3585 · pith:2009:4B4QORN4F5K2AGIWHIJWP7F3FB

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Paper page arXiv integrity.json bundle.json

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Signed record

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