{"paper":{"title":"[O~{\\small VI} from the SBs of the LMC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Amit Pathak, Ananta C. Pradhan, D. K. Ojha, Jayant Murthy","submitted_at":"2013-07-04T08:47:38Z","abstract_excerpt":"We have presented the observations of O {\\small VI} absorption at 1032 \\AA\\ towards 22 sightlines in 10 superbubbles (SBs) of the Large Magellanic Cloud (LMC) using the data obtained from the {\\em Far Ultraviolet Spectroscopic Explorer (FUSE)}. The estimated abundance of O {\\small VI} in the SBs varies from a minimum of (1.09 $\\pm$0.22)$\\times10^{14}$ atoms/cm$^{2}$ in SB N206 to a maximum of (3.71$\\pm$0.23)$\\times10^{14}$ atoms/cm$^{2}$ in SB N70. We find about a 46% excess in the abundance of O {\\small VI} in the SBs compared to the non-SB lines of sight. Even inside a SB, O {\\small VI} colu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.1240","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"}