{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:BCR562V6RN3BCX3E7A7Y3WXCRE","short_pith_number":"pith:BCR562V6","schema_version":"1.0","canonical_sha256":"08a3df6abe8b76115f64f83f8ddae289294d8a6a4fac1510f247c5567c327b68","source":{"kind":"arxiv","id":"1211.6314","version":1},"attestation_state":"computed","paper":{"title":"On the spin-down mechanism of the X-ray pulsar 4U 2206+54","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"N.G. Beskrovnaya, N.R. Ikhsanov","submitted_at":"2012-11-27T14:29:02Z","abstract_excerpt":"Observations of the X-ray pulsar 4U 2206+54, performed over a 15-year span, show its period, which is now 5555 \\pm 9 s, to increase drastically. Such behavior of the pulsar can be hardly explained in the frame of traditional scenarios of spin evolution of compact stars. The observed spin-down rate of the neutron star in 4U 2206+54 proves to be in good agreement with the value expected within magnetic accretion scenario which takes into account that magnetic field of the accretion stream can under certain conditions affect its geometry and type of flow. The neutron star in this case accretes ma"},"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":"1211.6314","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-11-27T14:29:02Z","cross_cats_sorted":[],"title_canon_sha256":"d18c65a58b3a784bb5a0f47425be06e7a68e1bda7ae4239e8d14d96cc226a0e7","abstract_canon_sha256":"522a51b66d150ea5db894e5ec1a900d93ea8dd7e870397a8964c745fa5773db2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:27:22.832660Z","signature_b64":"JmCm7/bNSz+cJwkQrlAuc5p0tNvuoX5G7T5m/b0vvpTxxX+KoOoFSXafZtgG8hJt9sLAAcg3IR4n2FIG+Ww7DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"08a3df6abe8b76115f64f83f8ddae289294d8a6a4fac1510f247c5567c327b68","last_reissued_at":"2026-05-18T03:27:22.831942Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:27:22.831942Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the spin-down mechanism of the X-ray pulsar 4U 2206+54","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"N.G. Beskrovnaya, N.R. Ikhsanov","submitted_at":"2012-11-27T14:29:02Z","abstract_excerpt":"Observations of the X-ray pulsar 4U 2206+54, performed over a 15-year span, show its period, which is now 5555 \\pm 9 s, to increase drastically. Such behavior of the pulsar can be hardly explained in the frame of traditional scenarios of spin evolution of compact stars. The observed spin-down rate of the neutron star in 4U 2206+54 proves to be in good agreement with the value expected within magnetic accretion scenario which takes into account that magnetic field of the accretion stream can under certain conditions affect its geometry and type of flow. The neutron star in this case accretes ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.6314","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":"1211.6314","created_at":"2026-05-18T03:27:22.832049+00:00"},{"alias_kind":"arxiv_version","alias_value":"1211.6314v1","created_at":"2026-05-18T03:27:22.832049+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.6314","created_at":"2026-05-18T03:27:22.832049+00:00"},{"alias_kind":"pith_short_12","alias_value":"BCR562V6RN3B","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"BCR562V6RN3BCX3E","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"BCR562V6","created_at":"2026-05-18T12:26:58.693483+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/BCR562V6RN3BCX3E7A7Y3WXCRE","json":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE.json","graph_json":"https://pith.science/api/pith-number/BCR562V6RN3BCX3E7A7Y3WXCRE/graph.json","events_json":"https://pith.science/api/pith-number/BCR562V6RN3BCX3E7A7Y3WXCRE/events.json","paper":"https://pith.science/paper/BCR562V6"},"agent_actions":{"view_html":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE","download_json":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE.json","view_paper":"https://pith.science/paper/BCR562V6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1211.6314&json=true","fetch_graph":"https://pith.science/api/pith-number/BCR562V6RN3BCX3E7A7Y3WXCRE/graph.json","fetch_events":"https://pith.science/api/pith-number/BCR562V6RN3BCX3E7A7Y3WXCRE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE/action/storage_attestation","attest_author":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE/action/author_attestation","sign_citation":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE/action/citation_signature","submit_replication":"https://pith.science/pith/BCR562V6RN3BCX3E7A7Y3WXCRE/action/replication_record"}},"created_at":"2026-05-18T03:27:22.832049+00:00","updated_at":"2026-05-18T03:27:22.832049+00:00"}