{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:A3BQNDVC7R7IW4BCQNX6SATB63","short_pith_number":"pith:A3BQNDVC","schema_version":"1.0","canonical_sha256":"06c3068ea2fc7e8b7022836fe90261f6e8420c32922ba46e51451b560754532b","source":{"kind":"arxiv","id":"1105.1481","version":2},"attestation_state":"computed","paper":{"title":"Hydrodynamic Interaction between the Be Star and the Pulsar in the TeV Binary PSR B1259-63/LS 2883","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Akiko Kawachi, Atsuo T. Okazaki, Jumpei Takata, Kimitake Hayasaki, Shigehiro Nagataki, Stanley P. Owocki, Tsuguya Naito","submitted_at":"2011-05-08T00:15:16Z","abstract_excerpt":"We study the interaction between the Be star and the pulsar in the TeV binary PSR B1259-63/LS 2883, using 3-D SPH simulations of the tidal and wind interactions in this Be-pulsar system. We first run a simulation without pulsar wind nor Be wind, taking into account only the gravitational effect of the pulsar on the Be disk. In this simulation, the gas particles are ejected at a constant rate from the equatorial surface of the Be star, which is tilted in a direction consistent with multi-waveband observations. We run the simulation until the Be disk is fully developed and starts to repeat a reg"},"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":"1105.1481","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-05-08T00:15:16Z","cross_cats_sorted":[],"title_canon_sha256":"4db5c86012118dfe7a19388f6deffd125053c2c23f62ff9e2b0cc07a5890664f","abstract_canon_sha256":"da939cea69fdebc708b8ba5c1f1f83ecb97a0bbaf14578eb49afc1eb9e917244"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:02:02.851852Z","signature_b64":"vF4eT1JE+ngZ1oKR7ty0voeRj1UuT3fPSoicEu8vZizaVflrwNtxVreY5aM89qhgAUmzSm9DBhfsi9IWwdgWDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"06c3068ea2fc7e8b7022836fe90261f6e8420c32922ba46e51451b560754532b","last_reissued_at":"2026-05-18T02:02:02.850986Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:02:02.850986Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hydrodynamic Interaction between the Be Star and the Pulsar in the TeV Binary PSR B1259-63/LS 2883","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Akiko Kawachi, Atsuo T. Okazaki, Jumpei Takata, Kimitake Hayasaki, Shigehiro Nagataki, Stanley P. Owocki, Tsuguya Naito","submitted_at":"2011-05-08T00:15:16Z","abstract_excerpt":"We study the interaction between the Be star and the pulsar in the TeV binary PSR B1259-63/LS 2883, using 3-D SPH simulations of the tidal and wind interactions in this Be-pulsar system. We first run a simulation without pulsar wind nor Be wind, taking into account only the gravitational effect of the pulsar on the Be disk. In this simulation, the gas particles are ejected at a constant rate from the equatorial surface of the Be star, which is tilted in a direction consistent with multi-waveband observations. We run the simulation until the Be disk is fully developed and starts to repeat a reg"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1105.1481","kind":"arxiv","version":2},"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":"1105.1481","created_at":"2026-05-18T02:02:02.851136+00:00"},{"alias_kind":"arxiv_version","alias_value":"1105.1481v2","created_at":"2026-05-18T02:02:02.851136+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1105.1481","created_at":"2026-05-18T02:02:02.851136+00:00"},{"alias_kind":"pith_short_12","alias_value":"A3BQNDVC7R7I","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_16","alias_value":"A3BQNDVC7R7IW4BC","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_8","alias_value":"A3BQNDVC","created_at":"2026-05-18T12:26:22.705136+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/A3BQNDVC7R7IW4BCQNX6SATB63","json":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63.json","graph_json":"https://pith.science/api/pith-number/A3BQNDVC7R7IW4BCQNX6SATB63/graph.json","events_json":"https://pith.science/api/pith-number/A3BQNDVC7R7IW4BCQNX6SATB63/events.json","paper":"https://pith.science/paper/A3BQNDVC"},"agent_actions":{"view_html":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63","download_json":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63.json","view_paper":"https://pith.science/paper/A3BQNDVC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1105.1481&json=true","fetch_graph":"https://pith.science/api/pith-number/A3BQNDVC7R7IW4BCQNX6SATB63/graph.json","fetch_events":"https://pith.science/api/pith-number/A3BQNDVC7R7IW4BCQNX6SATB63/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63/action/timestamp_anchor","attest_storage":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63/action/storage_attestation","attest_author":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63/action/author_attestation","sign_citation":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63/action/citation_signature","submit_replication":"https://pith.science/pith/A3BQNDVC7R7IW4BCQNX6SATB63/action/replication_record"}},"created_at":"2026-05-18T02:02:02.851136+00:00","updated_at":"2026-05-18T02:02:02.851136+00:00"}