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The dominant parameters in the model are the $\\beta$ value of the velocity law, the rotation rate of the star, $S_o$, and the ratio of the magnetic field energy density to the disk gravitational energy density, $\\gamma$.\n  The model predictions are comp"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0710.2633","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-10-14T02:34:49Z","cross_cats_sorted":[],"title_canon_sha256":"a54b1ff5c584b291ba342e43c5ebec847622b095d6e61e44f7c79b33d04218f1","abstract_canon_sha256":"31f7120a0523703c220792d85a25d243e06ca910b370ff840b3817c51c04eb41"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:06:14.838391Z","signature_b64":"h11MW+5KEUpZMVR5HZ8M/G7kyJvEfV+DK6M7nf5WQLmsiquO27kEtDJffDWNU+Oo3y7sYmhGMdu8GpMWCjUQDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6e35188e8318c3f11e7400d91d1360e7f331357d16b59f5bd8f64a5f503c1336","last_reissued_at":"2026-07-04T17:06:14.837989Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:06:14.837989Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray Emission from Magnetically Torqued Disks of Oe/Be Stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J. 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