{"paper":{"title":"Far-Ultraviolet Spectral Images of the Vela Supernova Remnant: Supplements and Comparisons with other Wavelength Images","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Il-Joong Kim, Jerry Edelstein, Kwang-Il Seon, Kyoung-Wook Min, Wonyong Han","submitted_at":"2012-10-31T02:44:34Z","abstract_excerpt":"We present the improved far-ultraviolet (FUV) emission-line images of the entire Vela supernova remnant (SNR) using newly processed SPEAR/FIMS data. The incomplete C III {\\lambda}977 and O VI {\\lambda}{\\lambda}1032, 1038 images presented in the previous study are updated to cover the whole region. The C IV {\\lambda}{\\lambda}1548, 1551 image with a higher resolution and new images at Si IV {\\lambda}{\\lambda}1394, 1403, O IV] {\\lambda}1404, He II {\\lambda}1640.5, and O III] {\\lambda}{\\lambda}1661, 1666 are also shown. Comparison of emission line ratios for two enhanced FUV regions reveals that t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.8219","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"}