{"paper":{"title":"The He II Fowler lines and the O III and N III Bowen fluorescence lines in the symbiotic nova RR Tel","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"France), GEPI, Italy; (2) CIFIST Marie Curie Excellence Team; (3) Observatoire de Paris, J. Danziger (1), Meudon, P. Bonifacio (1)(2)(3) ((1) INAF-Osservatorio Astronomico di Trieste, P. Selvelli (1), Trieste","submitted_at":"2006-11-30T13:22:20Z","abstract_excerpt":"A new measure of reddening (E$_{(B-V)}$$\\sim$0.00) has been obtained from the comparison between the observed and the theoretical intensity decrement for 20 emission lines of the $\\ion{He}{ii}$ Fowler (n$\\to$3) series. This value has been confirmed by the STIS and IUE continuum distribution, and by the value of n$_H$ from the damped profile of the IS H Ly-$\\alpha$ line. We have obtained very accurate measurements for about thirty Bowen lines of $\\ion{O}{iii}$ and a precise determination of the efficiency in the O1 and O3 excitation channels (18 % and 0.7 %, respectively). The relative $\\ion{O}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0611943","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":""},"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"}