{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:OBF4ZRTIOC44NEDWHIFL7ZUA5W","short_pith_number":"pith:OBF4ZRTI","schema_version":"1.0","canonical_sha256":"704bccc66870b9c690763a0abfe680ed82ecdad783e4fc4b3c557c583b4b115a","source":{"kind":"arxiv","id":"1205.5696","version":1},"attestation_state":"computed","paper":{"title":"Population Synthesis for Symbiotic X-ray Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. G. Kuranov, C.-H. Zhu, G.-L. Lu, K. A. Postnov, L. R. Yungelson, N. Wang","submitted_at":"2012-05-25T13:37:55Z","abstract_excerpt":"Symbiotic X-ray binaries (SyXBs) comprise a rare class of low-mass X-ray binaries. We study the Galactic SyXBs, which we consider as detached binaries composed of low-mass giants and wind-fed neutron star companions, by simulation of the interaction of a magnetized neutron star (NS) with its environment and utilizing a population synthesis code. We focus mainly on the parameters that influence observational appearance of the SyXB: the donor wind velocity (vw) and the angular momentum distribution in the shell of matter settling onto NS. We estimate the birthrate of SyXB as $\\sim 4.1\\times 10^{"},"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":"1205.5696","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-05-25T13:37:55Z","cross_cats_sorted":[],"title_canon_sha256":"4ec90d1ca42af1c6d8def2b926f460300b51556048af700b745e7e98fda325e0","abstract_canon_sha256":"b3ed6e99c1c845198f0803f65ef5f0644bb3aa242ba2010975858b32706b7519"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:17.298424Z","signature_b64":"sf9Jul/n3PzWKi/+rD5tO182gDP1QJYOJ2W76TKsQadinTmntIpYo4Ng4nM76PCV0F3MrwwbXs2Q1PxMe/cfBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"704bccc66870b9c690763a0abfe680ed82ecdad783e4fc4b3c557c583b4b115a","last_reissued_at":"2026-05-18T01:57:17.297875Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:17.297875Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Population Synthesis for Symbiotic X-ray Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. G. Kuranov, C.-H. Zhu, G.-L. Lu, K. A. Postnov, L. R. Yungelson, N. Wang","submitted_at":"2012-05-25T13:37:55Z","abstract_excerpt":"Symbiotic X-ray binaries (SyXBs) comprise a rare class of low-mass X-ray binaries. We study the Galactic SyXBs, which we consider as detached binaries composed of low-mass giants and wind-fed neutron star companions, by simulation of the interaction of a magnetized neutron star (NS) with its environment and utilizing a population synthesis code. We focus mainly on the parameters that influence observational appearance of the SyXB: the donor wind velocity (vw) and the angular momentum distribution in the shell of matter settling onto NS. We estimate the birthrate of SyXB as $\\sim 4.1\\times 10^{"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.5696","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":"1205.5696","created_at":"2026-05-18T01:57:17.297962+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.5696v1","created_at":"2026-05-18T01:57:17.297962+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.5696","created_at":"2026-05-18T01:57:17.297962+00:00"},{"alias_kind":"pith_short_12","alias_value":"OBF4ZRTIOC44","created_at":"2026-05-18T12:27:16.716162+00:00"},{"alias_kind":"pith_short_16","alias_value":"OBF4ZRTIOC44NEDW","created_at":"2026-05-18T12:27:16.716162+00:00"},{"alias_kind":"pith_short_8","alias_value":"OBF4ZRTI","created_at":"2026-05-18T12:27:16.716162+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/OBF4ZRTIOC44NEDWHIFL7ZUA5W","json":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W.json","graph_json":"https://pith.science/api/pith-number/OBF4ZRTIOC44NEDWHIFL7ZUA5W/graph.json","events_json":"https://pith.science/api/pith-number/OBF4ZRTIOC44NEDWHIFL7ZUA5W/events.json","paper":"https://pith.science/paper/OBF4ZRTI"},"agent_actions":{"view_html":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W","download_json":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W.json","view_paper":"https://pith.science/paper/OBF4ZRTI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.5696&json=true","fetch_graph":"https://pith.science/api/pith-number/OBF4ZRTIOC44NEDWHIFL7ZUA5W/graph.json","fetch_events":"https://pith.science/api/pith-number/OBF4ZRTIOC44NEDWHIFL7ZUA5W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W/action/storage_attestation","attest_author":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W/action/author_attestation","sign_citation":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W/action/citation_signature","submit_replication":"https://pith.science/pith/OBF4ZRTIOC44NEDWHIFL7ZUA5W/action/replication_record"}},"created_at":"2026-05-18T01:57:17.297962+00:00","updated_at":"2026-05-18T01:57:17.297962+00:00"}