{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:GPNXUKUTECKMM4TDR5HMA7IK47","short_pith_number":"pith:GPNXUKUT","schema_version":"1.0","canonical_sha256":"33db7a2a932094c672638f4ec07d0ae7d8b49e5f4673fe16e9450a8ba53a5215","source":{"kind":"arxiv","id":"1009.3433","version":1},"attestation_state":"computed","paper":{"title":"Mixing in two magnetic OB stars discovered by the MiMeS collaboration","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Thierry Morel","submitted_at":"2010-09-17T14:31:43Z","abstract_excerpt":"Recent observational and theoretical arguments suggest that magnetic OB stars may suffer more mixing than their non magnetic analogs. We present the results of an NLTE abundance study revealing a lack of CN-cycled material at the surface of two magnetic stars discovered by the MiMeS project (NGC2244 #201 and HD 57682). The existence of a strong magnetic field is therefore not a sufficient condition for deep mixing in main-sequence OB 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":"1009.3433","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-09-17T14:31:43Z","cross_cats_sorted":[],"title_canon_sha256":"9391301db6e85ce97320f0d598b25e448b84d8183f42186960bd58246411d0eb","abstract_canon_sha256":"9c8cf7d151c174f5de182d63d158e35f6302a230331194cae4cf958a54fad4d3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:24.986909Z","signature_b64":"FKrwD2xQNzZ0ADJrexxMXlVCOKzoCYXNOoV/zGQjD0MK8xYD5M9LtbqS5cC9oCSOpHk0U/971kAPiQnw5QpoDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"33db7a2a932094c672638f4ec07d0ae7d8b49e5f4673fe16e9450a8ba53a5215","last_reissued_at":"2026-05-18T02:05:24.986182Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:24.986182Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mixing in two magnetic OB stars discovered by the MiMeS collaboration","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Thierry Morel","submitted_at":"2010-09-17T14:31:43Z","abstract_excerpt":"Recent observational and theoretical arguments suggest that magnetic OB stars may suffer more mixing than their non magnetic analogs. We present the results of an NLTE abundance study revealing a lack of CN-cycled material at the surface of two magnetic stars discovered by the MiMeS project (NGC2244 #201 and HD 57682). The existence of a strong magnetic field is therefore not a sufficient condition for deep mixing in main-sequence OB stars."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.3433","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":"1009.3433","created_at":"2026-05-18T02:05:24.986302+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.3433v1","created_at":"2026-05-18T02:05:24.986302+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.3433","created_at":"2026-05-18T02:05:24.986302+00:00"},{"alias_kind":"pith_short_12","alias_value":"GPNXUKUTECKM","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_16","alias_value":"GPNXUKUTECKMM4TD","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_8","alias_value":"GPNXUKUT","created_at":"2026-05-18T12:26:07.630475+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/GPNXUKUTECKMM4TDR5HMA7IK47","json":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47.json","graph_json":"https://pith.science/api/pith-number/GPNXUKUTECKMM4TDR5HMA7IK47/graph.json","events_json":"https://pith.science/api/pith-number/GPNXUKUTECKMM4TDR5HMA7IK47/events.json","paper":"https://pith.science/paper/GPNXUKUT"},"agent_actions":{"view_html":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47","download_json":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47.json","view_paper":"https://pith.science/paper/GPNXUKUT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.3433&json=true","fetch_graph":"https://pith.science/api/pith-number/GPNXUKUTECKMM4TDR5HMA7IK47/graph.json","fetch_events":"https://pith.science/api/pith-number/GPNXUKUTECKMM4TDR5HMA7IK47/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47/action/storage_attestation","attest_author":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47/action/author_attestation","sign_citation":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47/action/citation_signature","submit_replication":"https://pith.science/pith/GPNXUKUTECKMM4TDR5HMA7IK47/action/replication_record"}},"created_at":"2026-05-18T02:05:24.986302+00:00","updated_at":"2026-05-18T02:05:24.986302+00:00"}