{"paper":{"title":"O~{\\small VI} absorption in the Milky Way along the Large Magellanic Cloud lines of sight","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Amit Pathak, Ananta C. Pradhan, Jayanta K. Sarma, Jayant Murthy, Rathin Sarma","submitted_at":"2013-07-26T05:50:40Z","abstract_excerpt":"We have used \\textit{Far Ultraviolet Spectroscopic Explorer (FUSE)} observations of the Large Magellanic Cloud (LMC) to determine the O {\\small VI} column densities in the Milky Way (MW) towards 6 LMC lines of sight. The mean column density of O {\\small VI} in the MW is found to be log N(O {\\small VI})=14.257$_{-0.084}^{+0.096}$. The results confirm the patchiness of O {\\small VI} absorption in the MW and the column densities are higher or comparable to the LMC."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.6928","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"}