{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:Y56TRV5RLOW6FMIW4ZQ3CARBD6","short_pith_number":"pith:Y56TRV5R","schema_version":"1.0","canonical_sha256":"c77d38d7b15bade2b116e661b102211f83c7de166f231a693d6b770283fad1c3","source":{"kind":"arxiv","id":"astro-ph/9809036","version":1},"attestation_state":"computed","paper":{"title":"X-ray irradiation in low mass binary systems","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. Dubus, J.-M. Hameury, J.-P. Lasota, P.A. Charles","submitted_at":"1998-09-03T13:52:06Z","abstract_excerpt":"We calculate self-consistent models of X-ray irradiated accretion discs in close binary systems. We show that a point X-ray source powered by accretion and located in the disc plane cannot modify the disc structure, mainly because of the self-screening by the disc of its outer regions. Since observations show that the emission of the outer disc regions in low mass X-ray binaries is dominated by the reprocessed X-ray flux, accretion discs in these systems must be either warped or irradiated by a source above the disc plane, or both. We analyse the thermal-viscous stability of irradiated accreti"},"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":"astro-ph/9809036","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1998-09-03T13:52:06Z","cross_cats_sorted":[],"title_canon_sha256":"d2601ae373367718fbefe49a5fd28e6b6cc6a6761f62686dcda0dc3b84dc26db","abstract_canon_sha256":"addfeef48b800b497df040769ac8ad0423f19675f664042fb9476ac2ab11c2b0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:06:59.511295Z","signature_b64":"1k0qiuavkfengQulOrzV4jvLocGu5gbA7eOXsZhjclr2g2PiMSojhKn/QPvM8hfdE4LBVgzi8Zyf7mOmo/PbBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c77d38d7b15bade2b116e661b102211f83c7de166f231a693d6b770283fad1c3","last_reissued_at":"2026-07-04T16:06:59.510882Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:06:59.510882Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray irradiation in low mass binary systems","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. Dubus, J.-M. Hameury, J.-P. Lasota, P.A. Charles","submitted_at":"1998-09-03T13:52:06Z","abstract_excerpt":"We calculate self-consistent models of X-ray irradiated accretion discs in close binary systems. We show that a point X-ray source powered by accretion and located in the disc plane cannot modify the disc structure, mainly because of the self-screening by the disc of its outer regions. Since observations show that the emission of the outer disc regions in low mass X-ray binaries is dominated by the reprocessed X-ray flux, accretion discs in these systems must be either warped or irradiated by a source above the disc plane, or both. We analyse the thermal-viscous stability of irradiated accreti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9809036","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/9809036/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/9809036","created_at":"2026-07-04T16:06:59.510946+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9809036v1","created_at":"2026-07-04T16:06:59.510946+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9809036","created_at":"2026-07-04T16:06:59.510946+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y56TRV5RLOW6","created_at":"2026-07-04T16:06:59.510946+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y56TRV5RLOW6FMIW","created_at":"2026-07-04T16:06:59.510946+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y56TRV5R","created_at":"2026-07-04T16:06:59.510946+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/Y56TRV5RLOW6FMIW4ZQ3CARBD6","json":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6.json","graph_json":"https://pith.science/api/pith-number/Y56TRV5RLOW6FMIW4ZQ3CARBD6/graph.json","events_json":"https://pith.science/api/pith-number/Y56TRV5RLOW6FMIW4ZQ3CARBD6/events.json","paper":"https://pith.science/paper/Y56TRV5R"},"agent_actions":{"view_html":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6","download_json":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6.json","view_paper":"https://pith.science/paper/Y56TRV5R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9809036&json=true","fetch_graph":"https://pith.science/api/pith-number/Y56TRV5RLOW6FMIW4ZQ3CARBD6/graph.json","fetch_events":"https://pith.science/api/pith-number/Y56TRV5RLOW6FMIW4ZQ3CARBD6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6/action/storage_attestation","attest_author":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6/action/author_attestation","sign_citation":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6/action/citation_signature","submit_replication":"https://pith.science/pith/Y56TRV5RLOW6FMIW4ZQ3CARBD6/action/replication_record"}},"created_at":"2026-07-04T16:06:59.510946+00:00","updated_at":"2026-07-04T16:06:59.510946+00:00"}