{"paper":{"title":"Super-Eddington stellar winds: unifying radiative-enthalpy vs. flux-driven models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Eliot Quataert, Richard H. D. Townsend, Stanley P. Owocki","submitted_at":"2017-08-25T15:56:43Z","abstract_excerpt":"We derive semi-analytic solutions for optically thick, super-Eddington stellar winds, induced by an assumed steady energy addition $\\Delta {\\dot E}$ concentrated around a near-surface heating radius $R$ in a massive star of central luminosity $L_\\ast$. We show that obtaining steady wind solutions requires both that the resulting total luminosity $L_o = L_\\ast + \\Delta {\\dot E}$ exceed the Eddington luminosity, $\\Gamma_o \\equiv L_o/L_{Edd} > 1$, and that the induced mass loss rate be such that the \"photon-tiring\" parameter $m \\equiv {\\dot M} GM/R L_o \\le 1-1/\\Gamma_o$, ensuring the luminosity i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.07790","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"}