{"paper":{"title":"Super-Eddington Black-Hole Models for SS 433","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Toru Okuda","submitted_at":"2002-02-25T11:19:04Z","abstract_excerpt":"We examine highly super-Eddington black-hole models for SS 433, based on two-dimensional hydrodynamical calculations coupled with radiation transport. The super-Eddington accretion flow with a small viscosity parameter,\n $\\alpha = 10^{-3}$, results in a geometrically and optically thick disk with a large opening angle of $\\sim 60^{\\circ}$ to the equatorial plane and a very rarefied, hot, and optically thin high-velocity jets region around the disk.\n The thick accretion flow consists of two different zones: an inner advection-dominated zone and an outer convection-dominated zone. The high-veloc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0202446","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"}