{"paper":{"title":"W43: the closest molecular complex of the Galactic Bar?","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"F. Heitsch, F. Motte, F. Schuller, F. Wyrowski, K. M. Menten, L. Bronfman, N. Schneider, P. Carlhoff, P. Schilke, Q. Nguyen Luong, S. Bontemps, T. Henning","submitted_at":"2011-02-17T00:10:42Z","abstract_excerpt":"We used a large database extracted from Galaxy-wide surveys of H {\\scriptsize I}, $^{13}$CO 1-0, $8 \\micron$ and $870 \\micron$ continuum to trace diffuse atomic gas, low- to medium-density molecular gas, high-density molecular gas, and star formation activity which we complemented by dedicated $^{12}$CO 2--1, 3--2 observations of the W43 region. From the detailed 3D (space-space-velocity) analysis of the molecular and atomic cloud tracers through the region and despite its wide velocity range (\\emph{FWHM}$\\sim22.3 \\kms$ around $\\vlsr\\sim 95.9 \\kms$), we identified W43 as a large (equivalent di"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.3460","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"}