{"paper":{"title":"A Monte Carlo Study of Flux Ratios of Raman Scattered O~VI Features at 6825 \\AA\\ and 7082 \\AA\\ in Symbiotic Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Dae-Sub Lee, Hee-Won Lee, Jeong-Eun Heo, Seok-Jun Chang, Young-Min Lee","submitted_at":"2016-10-23T10:16:28Z","abstract_excerpt":"Symbiotic stars are regarded as wide binary systems consisting of a hot white dwarf and a mass losing giant. They exhibit unique spectral features at 6825 \\AA\\ and 7082 \\AA, which are formed via Raman scattering of \\ion{O}{6}$\\lambda\\lambda$ 1032 and 1038 with atomic hydrogen. We adopt a Monte Carlo technique to generate the same number of \\ion{O}{6}$\\lambda$1032 and $\\lambda$1038 line photons and compute the flux ratio $F(6825)/F(7082)$ of these Raman scattered \\ion{O}{6} features formed in neutral regions with a simple geometric shape as a function of \\ion{H}{1} column density $N_{HI}$. In c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.07139","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"}