{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:KA5AFDSWARAFQ5AWVSYLI7USR7","short_pith_number":"pith:KA5AFDSW","schema_version":"1.0","canonical_sha256":"503a028e560440587416acb0b47e928fe0cf498eb4c79555f9a05dc8491b7d9c","source":{"kind":"arxiv","id":"astro-ph/0406166","version":2},"attestation_state":"computed","paper":{"title":"A Review of Bondi--Hoyle--Lyttleton Accretion","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"R. G. Edgar","submitted_at":"2004-06-07T14:16:05Z","abstract_excerpt":"If a point mass moves through a uniform gas cloud, at what rate does it accrete material? This is the question studied by Bondi, Hoyle and Lyttleton. This paper draws together the work performed in this area since the problem was first studied. Time has shown that, despite the simplifications made, Bondi, Hoyle and Lyttleton made quite accurate predictions for the accretion rate. Bondi--Hoyle--Lyttleton accretion has found application in many fields of astronomy, and these are also discussed."},"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/0406166","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-06-07T14:16:05Z","cross_cats_sorted":[],"title_canon_sha256":"710c98d6256dd9f447d0d69f29d9574f85b03f0b656e33f9be4949e8359efbed","abstract_canon_sha256":"40520ae0e7e262d2786c6394c8b03bb0db2af513284739fd6754082e005f383f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:43:56.496292Z","signature_b64":"optEsetGcYDxSSpbKex99RgNGtU6TXqj/E12qYsNG8GD7SnUB+38WxxLVJxHdnMNae6fOP2lhrWFUVDKxnemBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"503a028e560440587416acb0b47e928fe0cf498eb4c79555f9a05dc8491b7d9c","last_reissued_at":"2026-07-04T16:43:56.495918Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:43:56.495918Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Review of Bondi--Hoyle--Lyttleton Accretion","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"R. G. Edgar","submitted_at":"2004-06-07T14:16:05Z","abstract_excerpt":"If a point mass moves through a uniform gas cloud, at what rate does it accrete material? This is the question studied by Bondi, Hoyle and Lyttleton. This paper draws together the work performed in this area since the problem was first studied. Time has shown that, despite the simplifications made, Bondi, Hoyle and Lyttleton made quite accurate predictions for the accretion rate. Bondi--Hoyle--Lyttleton accretion has found application in many fields of astronomy, and these are also discussed."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0406166","kind":"arxiv","version":2},"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/0406166/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/0406166","created_at":"2026-07-04T16:43:56.495982+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0406166v2","created_at":"2026-07-04T16:43:56.495982+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0406166","created_at":"2026-07-04T16:43:56.495982+00:00"},{"alias_kind":"pith_short_12","alias_value":"KA5AFDSWARAF","created_at":"2026-07-04T16:43:56.495982+00:00"},{"alias_kind":"pith_short_16","alias_value":"KA5AFDSWARAFQ5AW","created_at":"2026-07-04T16:43:56.495982+00:00"},{"alias_kind":"pith_short_8","alias_value":"KA5AFDSW","created_at":"2026-07-04T16:43:56.495982+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":11,"internal_anchor_count":7,"sample":[{"citing_arxiv_id":"2607.07462","citing_title":"Relativistic Common-envelope Dynamics of a Stellar-mass Black Hole II: Kerr Black Hole","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2607.05275","citing_title":"Circumbinary disk formation through AGB star winds","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2606.18341","citing_title":"Orbital evolution of asymmetric binaries within accreting environments","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2606.31477","citing_title":"Multi-wavelength Emission Modeling from Accretion Flows around Isolated Black Holes Including Magnetic Flux Transport","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2606.13202","citing_title":"The first hours and days of the 2021 explosion of the recurrent symbiotic nova RS Ophiuchii","ref_index":45,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15772","citing_title":"Accretion Effects on Primordial Black Hole Reheating Constraints","ref_index":28,"is_internal_anchor":true},{"citing_arxiv_id":"2605.17005","citing_title":"Red novae, their progenitors, and remnants","ref_index":161,"is_internal_anchor":true},{"citing_arxiv_id":"2604.19236","citing_title":"Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26912","citing_title":"Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25560","citing_title":"Massive black holes and their galaxies","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04869","citing_title":"Exploration of the inner region of the system HD 142527","ref_index":192,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7","json":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7.json","graph_json":"https://pith.science/api/pith-number/KA5AFDSWARAFQ5AWVSYLI7USR7/graph.json","events_json":"https://pith.science/api/pith-number/KA5AFDSWARAFQ5AWVSYLI7USR7/events.json","paper":"https://pith.science/paper/KA5AFDSW"},"agent_actions":{"view_html":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7","download_json":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7.json","view_paper":"https://pith.science/paper/KA5AFDSW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0406166&json=true","fetch_graph":"https://pith.science/api/pith-number/KA5AFDSWARAFQ5AWVSYLI7USR7/graph.json","fetch_events":"https://pith.science/api/pith-number/KA5AFDSWARAFQ5AWVSYLI7USR7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7/action/storage_attestation","attest_author":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7/action/author_attestation","sign_citation":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7/action/citation_signature","submit_replication":"https://pith.science/pith/KA5AFDSWARAFQ5AWVSYLI7USR7/action/replication_record"}},"created_at":"2026-07-04T16:43:56.495982+00:00","updated_at":"2026-07-04T16:43:56.495982+00:00"}