{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:Z5XNS7ELEO3ZJUUA2LQCNBVWA6","short_pith_number":"pith:Z5XNS7EL","schema_version":"1.0","canonical_sha256":"cf6ed97c8b23b794d280d2e02686b607830a7bd618388e81dc4c8c7726d91d12","source":{"kind":"arxiv","id":"1111.6975","version":1},"attestation_state":"computed","paper":{"title":"Tracing colliding winds in the UV line orbital variability of gamma-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. Szostek, G. Dubus, M. V. McSwain","submitted_at":"2011-11-29T21:00:05Z","abstract_excerpt":"Gamma-ray binaries emit most of their radiated power beyond ~10 MeV. The non-thermal emission is thought to arise from the interaction of the relativistic wind of a rotation-powered pulsar with the stellar wind of its massive (O or Be) companion star. A powerful pulsar creates an extended cavity, filled with relativistic electrons, in the radiatively-driven wind of the massive star. As a result, the observed P Cyg profiles of UV resonant lines from the stellar wind should be different from those of single massive stars. We propose to use UV emission lines to detect and constrain the colliding "},"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":"1111.6975","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-11-29T21:00:05Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"9896ad51e8c4908e0b6d86492ca26f9b6a6bbdc7fbb020dbdb5093af933cf3ac","abstract_canon_sha256":"7506ccc094c0904ad63d5f50fd7a047a596c91cbb79c904a731835f4c04e7174"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:21.692203Z","signature_b64":"Yn5ZsdnFo6eOpEiwnPCb/q6Fgc7sUNZDlQRe6uwW1HQanISu9PE2NH2wxn5+MwzWD3RhBa8v2yJoi1wvMBXtDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf6ed97c8b23b794d280d2e02686b607830a7bd618388e81dc4c8c7726d91d12","last_reissued_at":"2026-05-18T01:59:21.691454Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:21.691454Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tracing colliding winds in the UV line orbital variability of gamma-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. Szostek, G. Dubus, M. V. McSwain","submitted_at":"2011-11-29T21:00:05Z","abstract_excerpt":"Gamma-ray binaries emit most of their radiated power beyond ~10 MeV. The non-thermal emission is thought to arise from the interaction of the relativistic wind of a rotation-powered pulsar with the stellar wind of its massive (O or Be) companion star. A powerful pulsar creates an extended cavity, filled with relativistic electrons, in the radiatively-driven wind of the massive star. As a result, the observed P Cyg profiles of UV resonant lines from the stellar wind should be different from those of single massive stars. We propose to use UV emission lines to detect and constrain the colliding "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1111.6975","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":"1111.6975","created_at":"2026-05-18T01:59:21.691583+00:00"},{"alias_kind":"arxiv_version","alias_value":"1111.6975v1","created_at":"2026-05-18T01:59:21.691583+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1111.6975","created_at":"2026-05-18T01:59:21.691583+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z5XNS7ELEO3Z","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z5XNS7ELEO3ZJUUA","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z5XNS7EL","created_at":"2026-05-18T12:26:47.523578+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/Z5XNS7ELEO3ZJUUA2LQCNBVWA6","json":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6.json","graph_json":"https://pith.science/api/pith-number/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/graph.json","events_json":"https://pith.science/api/pith-number/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/events.json","paper":"https://pith.science/paper/Z5XNS7EL"},"agent_actions":{"view_html":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6","download_json":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6.json","view_paper":"https://pith.science/paper/Z5XNS7EL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1111.6975&json=true","fetch_graph":"https://pith.science/api/pith-number/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/graph.json","fetch_events":"https://pith.science/api/pith-number/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/action/storage_attestation","attest_author":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/action/author_attestation","sign_citation":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/action/citation_signature","submit_replication":"https://pith.science/pith/Z5XNS7ELEO3ZJUUA2LQCNBVWA6/action/replication_record"}},"created_at":"2026-05-18T01:59:21.691583+00:00","updated_at":"2026-05-18T01:59:21.691583+00:00"}