{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:6SZSLMTCTJFCMQ27NKECDONDQ7","short_pith_number":"pith:6SZSLMTC","schema_version":"1.0","canonical_sha256":"f4b325b2629a4a26435f6a8821b9a387e681c35dc988ad141245b2e78c339e11","source":{"kind":"arxiv","id":"astro-ph/0601067","version":1},"attestation_state":"computed","paper":{"title":"Rotation in the ZAMS: Be and Bn stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Torres (UNLP), C. Martayan (GEPI), J. Zorec (IAP), L. Cidale (UNLP), Y. Fr\\'emat (ROB)","submitted_at":"2006-01-04T07:50:45Z","abstract_excerpt":"We show that Be stars belong to a high velocity tail of a single B-type star rotational velocity distribution in the MS. This implies that: 1) the number fraction N(Be)/N(Be+B) is independent of the mass; 2) Bn stars having ZAMS rotational velocities higher than a given limit might become Be stars."},"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":"astro-ph/0601067","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-01-04T07:50:45Z","cross_cats_sorted":[],"title_canon_sha256":"d9a805bb32233733b8204e41e2c4316d8f40f4b0841a233c54b7216e15a7cea2","abstract_canon_sha256":"c4ef76b69eef5a090d1e989408fa1bad977892a5c40b0a707c6a6b3f7495b66f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:10.793555Z","signature_b64":"10ZmykXdIR8hOBMiFIjHM18kiEqR7axHj5Bt1o2Btq1QlrVrfvQ8YWYwdoRxAfwKXZUHvNF5Zs8SEfC8f2e2Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f4b325b2629a4a26435f6a8821b9a387e681c35dc988ad141245b2e78c339e11","last_reissued_at":"2026-05-18T01:09:10.792778Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:10.792778Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rotation in the ZAMS: Be and Bn stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Torres (UNLP), C. Martayan (GEPI), J. Zorec (IAP), L. Cidale (UNLP), Y. Fr\\'emat (ROB)","submitted_at":"2006-01-04T07:50:45Z","abstract_excerpt":"We show that Be stars belong to a high velocity tail of a single B-type star rotational velocity distribution in the MS. This implies that: 1) the number fraction N(Be)/N(Be+B) is independent of the mass; 2) Bn stars having ZAMS rotational velocities higher than a given limit might become Be stars."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0601067","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0601067","created_at":"2026-05-18T01:09:10.792919+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0601067v1","created_at":"2026-05-18T01:09:10.792919+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0601067","created_at":"2026-05-18T01:09:10.792919+00:00"},{"alias_kind":"pith_short_12","alias_value":"6SZSLMTCTJFC","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"6SZSLMTCTJFCMQ27","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"6SZSLMTC","created_at":"2026-05-18T12:25:53.939244+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7","json":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7.json","graph_json":"https://pith.science/api/pith-number/6SZSLMTCTJFCMQ27NKECDONDQ7/graph.json","events_json":"https://pith.science/api/pith-number/6SZSLMTCTJFCMQ27NKECDONDQ7/events.json","paper":"https://pith.science/paper/6SZSLMTC"},"agent_actions":{"view_html":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7","download_json":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7.json","view_paper":"https://pith.science/paper/6SZSLMTC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0601067&json=true","fetch_graph":"https://pith.science/api/pith-number/6SZSLMTCTJFCMQ27NKECDONDQ7/graph.json","fetch_events":"https://pith.science/api/pith-number/6SZSLMTCTJFCMQ27NKECDONDQ7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7/action/storage_attestation","attest_author":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7/action/author_attestation","sign_citation":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7/action/citation_signature","submit_replication":"https://pith.science/pith/6SZSLMTCTJFCMQ27NKECDONDQ7/action/replication_record"}},"created_at":"2026-05-18T01:09:10.792919+00:00","updated_at":"2026-05-18T01:09:10.792919+00:00"}