{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:UI2BJGKVLS5MAWLL3FYDWWNLWD","short_pith_number":"pith:UI2BJGKV","schema_version":"1.0","canonical_sha256":"a2341499555cbac0596bd9703b59abb0cdb81b9d00cc09faf073cbff9f29a366","source":{"kind":"arxiv","id":"1909.13601","version":1},"attestation_state":"computed","paper":{"title":"The impact of thermal winds on the outburst lightcurves of black hole X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"B. E. Tetarenko, C. Done, G. Dubus, J.-M. Hameury","submitted_at":"2019-09-30T11:36:58Z","abstract_excerpt":"The observed signatures of winds from X-ray binaries are broadly consistent with thermal winds, driven by X-ray irradiation of the outer accretion disc. Thermal winds produce mass outflow rates that can exceed the accretion rate in the disc. We study the impact of this mass loss on the stability and lightcurves of X-ray binaries subject to the thermal-viscous instability, which drives their outbursts. Strong mass loss could shut off outbursts early, as proposed for the 2015 outburst of V404 Cyg. We use an analytical model for thermal (Compton) wind mass loss. Scattering in the strong wind expe"},"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":"1909.13601","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-09-30T11:36:58Z","cross_cats_sorted":[],"title_canon_sha256":"8416537ca69a96ece49f3b0189f2c709b733a102feb2c427cccdd7311f2ba2a1","abstract_canon_sha256":"fd650f844d7095aa9f7c365a8a0f303ae25fce3caa30e339e343201bd319cee1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:22:19.834949Z","signature_b64":"c/MVFm0BBgoqzW87r9CHs+EqM3nxmhV+RKcVEouIsOQjBMrXZwoG4+F7mIdT6JY+bEaVa+dPPmwrlFkc85tyDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a2341499555cbac0596bd9703b59abb0cdb81b9d00cc09faf073cbff9f29a366","last_reissued_at":"2026-07-05T00:22:19.834575Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:22:19.834575Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The impact of thermal winds on the outburst lightcurves of black hole X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"B. E. Tetarenko, C. Done, G. Dubus, J.-M. Hameury","submitted_at":"2019-09-30T11:36:58Z","abstract_excerpt":"The observed signatures of winds from X-ray binaries are broadly consistent with thermal winds, driven by X-ray irradiation of the outer accretion disc. Thermal winds produce mass outflow rates that can exceed the accretion rate in the disc. We study the impact of this mass loss on the stability and lightcurves of X-ray binaries subject to the thermal-viscous instability, which drives their outbursts. Strong mass loss could shut off outbursts early, as proposed for the 2015 outburst of V404 Cyg. We use an analytical model for thermal (Compton) wind mass loss. Scattering in the strong wind expe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.13601","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/1909.13601/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":"1909.13601","created_at":"2026-07-05T00:22:19.834630+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.13601v1","created_at":"2026-07-05T00:22:19.834630+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.13601","created_at":"2026-07-05T00:22:19.834630+00:00"},{"alias_kind":"pith_short_12","alias_value":"UI2BJGKVLS5M","created_at":"2026-07-05T00:22:19.834630+00:00"},{"alias_kind":"pith_short_16","alias_value":"UI2BJGKVLS5MAWLL","created_at":"2026-07-05T00:22:19.834630+00:00"},{"alias_kind":"pith_short_8","alias_value":"UI2BJGKV","created_at":"2026-07-05T00:22:19.834630+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/UI2BJGKVLS5MAWLL3FYDWWNLWD","json":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD.json","graph_json":"https://pith.science/api/pith-number/UI2BJGKVLS5MAWLL3FYDWWNLWD/graph.json","events_json":"https://pith.science/api/pith-number/UI2BJGKVLS5MAWLL3FYDWWNLWD/events.json","paper":"https://pith.science/paper/UI2BJGKV"},"agent_actions":{"view_html":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD","download_json":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD.json","view_paper":"https://pith.science/paper/UI2BJGKV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.13601&json=true","fetch_graph":"https://pith.science/api/pith-number/UI2BJGKVLS5MAWLL3FYDWWNLWD/graph.json","fetch_events":"https://pith.science/api/pith-number/UI2BJGKVLS5MAWLL3FYDWWNLWD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD/action/storage_attestation","attest_author":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD/action/author_attestation","sign_citation":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD/action/citation_signature","submit_replication":"https://pith.science/pith/UI2BJGKVLS5MAWLL3FYDWWNLWD/action/replication_record"}},"created_at":"2026-07-05T00:22:19.834630+00:00","updated_at":"2026-07-05T00:22:19.834630+00:00"}