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Integrity report for Pulsational instability of supergiant protostars: Do they grow supermassive by accretion?

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

arXiv:1302.6065 · pith:2013:7MYW57SLF7L62VF6BE2BJ2C3OM

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Paper page arXiv integrity.json bundle.json

Detector runs

Findings

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Signed record

The machine-readable record for this paper lives at /pith/7MYW57SLF7L62VF6BE2BJ2C3OM/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.