{"paper":{"title":"A $10^{10}$ Solar Mass Flow of Molecular Gas in the Abell 1835 Brightest Cluster Galaxy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. C. Edge, A. C. Fabian, A. N. Vantyghem, B. R. McNamara, C.C. Kirkpatrick, C. P. O'Dea, E. Egami, F. Combes, G.M. Voit, G. Tremblay, H.R. Russell, J.B.R. Oonk, J. N. Bregman, M. Donahue, N. W. Murray, P. E. J. Nulsen, P. Salome, R. A. Main, S. A. Baum, S. Hamer","submitted_at":"2014-03-17T20:00:26Z","abstract_excerpt":"We report ALMA Early Science observations of the Abell 1835 brightest cluster galaxy (BCG) in the CO (3-2) and CO (1-0) emission lines. We detect $5\\times 10^{10}~\\rm M_\\odot$ of molecular gas within 10 kpc of the BCG. Its ensemble velocity profile width of $\\sim 130 ~\\rm km~s^{-1}$ FWHM is too narrow for the molecular cloud sto be supported in the galaxy by dynamic pressure. The gas may instead be supported in a rotating, turbulent disk oriented nearly face-on. Roughly $10^{10}~\\rm M_\\odot$ of molecular gas is projected $3-10 ~\\rm kpc$ to the north-west and to the east of the nucleus with lin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.4249","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"}