{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:23WZMJ37SQF5NTWBQOZKWPJKIW","short_pith_number":"pith:23WZMJ37","schema_version":"1.0","canonical_sha256":"d6ed96277f940bd6cec183b2ab3d2a459346733a31b046a956a8ea503c5e65fb","source":{"kind":"arxiv","id":"1807.04789","version":1},"attestation_state":"computed","paper":{"title":"Physical properties of beta Lyr A and its opaque accretion disk","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Meilland, C. Farrington, D. Bonneau, D. Gies, D. Korcakova, D. Mourard, E. Baines, F. Baron, G. Schaefer, H. Bozic, H. McAlister, H. Schmitt, I. Tallon-Bosc, J. Armstrong, J. Budaj, J. Jurysek, J.M. Clausse, J. Monnier, J. Nemravova, M. Broz, M. Slechta, M. Wolf, N. Nardetto, P. Harmanec, P. Svoboad, P. Zasche","submitted_at":"2018-07-12T18:54:51Z","abstract_excerpt":"Mass exchange and mass loss in close binaries can significantly affect their evolution, but a complete self-consistent theory of these processes is still to be developed. Processes such as radiative shielding due to a~hot-spot region, or a~hydrodynamical interaction of different parts of the gas stream have been studied previously. In order to test the respective predictions, it is necessary to carry out detailed observations of binaries undergoing the largescale mass exchange, especially for those that are in the rapid transfer phase. \\bla is an archetype of such a system, having a long and r"},"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":"1807.04789","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-07-12T18:54:51Z","cross_cats_sorted":[],"title_canon_sha256":"9b6f2ee2a407a054c1e10a15fac49e3a8da712e7eb0e831e8051875a55d75c31","abstract_canon_sha256":"64d2c796ff5c4743f5110e0eed29a01d1b4fb804cd5022ffd957178a96f3ec58"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:10:51.421396Z","signature_b64":"iMDuIgdRR/M5phUbXjomSCQXTwJR04hz/YBt4uHLi2nlhLio97+cO2sapSiSc95RmwBRtCjJNdKlvlkkVL66BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d6ed96277f940bd6cec183b2ab3d2a459346733a31b046a956a8ea503c5e65fb","last_reissued_at":"2026-05-18T00:10:51.420779Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:10:51.420779Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Physical properties of beta Lyr A and its opaque accretion disk","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Meilland, C. Farrington, D. Bonneau, D. Gies, D. Korcakova, D. Mourard, E. Baines, F. Baron, G. Schaefer, H. Bozic, H. McAlister, H. Schmitt, I. Tallon-Bosc, J. Armstrong, J. Budaj, J. Jurysek, J.M. Clausse, J. Monnier, J. Nemravova, M. Broz, M. Slechta, M. Wolf, N. Nardetto, P. Harmanec, P. Svoboad, P. Zasche","submitted_at":"2018-07-12T18:54:51Z","abstract_excerpt":"Mass exchange and mass loss in close binaries can significantly affect their evolution, but a complete self-consistent theory of these processes is still to be developed. Processes such as radiative shielding due to a~hot-spot region, or a~hydrodynamical interaction of different parts of the gas stream have been studied previously. In order to test the respective predictions, it is necessary to carry out detailed observations of binaries undergoing the largescale mass exchange, especially for those that are in the rapid transfer phase. \\bla is an archetype of such a system, having a long and r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.04789","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":"1807.04789","created_at":"2026-05-18T00:10:51.420857+00:00"},{"alias_kind":"arxiv_version","alias_value":"1807.04789v1","created_at":"2026-05-18T00:10:51.420857+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.04789","created_at":"2026-05-18T00:10:51.420857+00:00"},{"alias_kind":"pith_short_12","alias_value":"23WZMJ37SQF5","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"23WZMJ37SQF5NTWB","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"23WZMJ37","created_at":"2026-05-18T12:31:59.375834+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/23WZMJ37SQF5NTWBQOZKWPJKIW","json":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW.json","graph_json":"https://pith.science/api/pith-number/23WZMJ37SQF5NTWBQOZKWPJKIW/graph.json","events_json":"https://pith.science/api/pith-number/23WZMJ37SQF5NTWBQOZKWPJKIW/events.json","paper":"https://pith.science/paper/23WZMJ37"},"agent_actions":{"view_html":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW","download_json":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW.json","view_paper":"https://pith.science/paper/23WZMJ37","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1807.04789&json=true","fetch_graph":"https://pith.science/api/pith-number/23WZMJ37SQF5NTWBQOZKWPJKIW/graph.json","fetch_events":"https://pith.science/api/pith-number/23WZMJ37SQF5NTWBQOZKWPJKIW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW/action/storage_attestation","attest_author":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW/action/author_attestation","sign_citation":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW/action/citation_signature","submit_replication":"https://pith.science/pith/23WZMJ37SQF5NTWBQOZKWPJKIW/action/replication_record"}},"created_at":"2026-05-18T00:10:51.420857+00:00","updated_at":"2026-05-18T00:10:51.420857+00:00"}