{"paper":{"title":"ALMA Observations of Warm Molecular Gas and Cold Dust in NGC 34","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. S. Evans, B. Schulz, C. Cao, C. K. Xu (IPAC), D. B. Sanders, E. J. Murphy, J. Chu, J. M. Mazzarella, L. Armus, N. Lu, P. Appleton, P. van der Werf, R. Meijerink, S. Haan, S. Lord, S. Stierwalt, T. Diaz-Santos, V. Charmandaris, Y. Gao, Y.-H. Zhao","submitted_at":"2014-04-04T22:05:19Z","abstract_excerpt":"We present ALMA Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435$\\mu m$ dust continuum emission in the nuclear region of NGC 34, a local luminous infrared galaxy (LIRG) at a distance of 84 Mpc (1\" = 407 pc) which contains a Seyfert 2 active galactic nucleus (AGN) and a nuclear starburst. The CO emission is well resolved by the ALMA beam ($\\rm 0.\"26\\times 0.\"23$), with an integrated flux of $\\rm f_{CO~(6-5)} = 1004\\; (\\pm 151) \\; Jy\\; km\\; s^{-1}$. Both the morphology and kinematics of the CO (6-5) emission are rather regular, consistent wit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.1402","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"}