{"paper":{"title":"ALMA Observations of the Galactic Center: SiO Outflows and High Mass Star Formation near Sgr A*","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Wootten, B. Whitney, D. A. Roberts, D. C. Lis, F. Yusef-Zadeh, H. Bushouse, M. Royster, M. Wardle, M. W. Pound, R. Arendt","submitted_at":"2013-03-14T10:52:56Z","abstract_excerpt":"ALMA observations of the Galactic center with spatial resolution $2.61\"\\times0.97\"$ resulted in the detection of 11 SiO (5-4) clumps of molecular gas within 0.6pc (15$\"$) of Sgr A*, interior to the 2-pc circumnuclear molecular ring. The three SiO (5-4) clumps closest to Sgr A* show the largest central velocities, $\\sim150$ \\kms, and broadest asymmetric linewidths with full width zero intensity (FWZI) $\\sim110-147$ \\kms. The remaining clumps, distributed mainly to the NE of the ionized mini-spiral, have narrow FWZI ($\\sim18-56$ \\kms). Using CARMA SiO (2-1) data, LVG modeling of the the SiO line"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.3403","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"}