{"paper":{"title":"The distribution and kinematics of interstellar O~{\\small VI} in the Milky Way}","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Amit Pathak, Jayanta K. Sarma, Jayanta Murthy, Rathin Sarma","submitted_at":"2016-10-04T14:03:57Z","abstract_excerpt":"We present the results of a survey of interstellar O~{\\small VI} absorption in the Milky Way (MW) towards {69} stars in the Large Magellanic Cloud (LMC) obtained with the \\textit{Far Ultraviolet Spectroscopic Explorer (FUSE)}. The integrated MW O~{\\small VI} column densities log N(O~{\\small VI}) are in the range from 13.68 to 14.73 with a mean of {14.26$_{-0.09}^{+0.07}$} atoms cm$^{-2}$. The O~{\\small VI} exponential scale height is found to be {2.28$\\pm$1.06} kpc. The O~{\\small VI} column density correlates with the Doppler parameter $\\it b$. The O~{\\small VI} velocity dispersion ranges from"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.01001","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"}