{"paper":{"title":"ALMA Imaging of the CO(6-5) Line Emission in NGC 7130","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Aaron Evans, Chen Cao, C. Kevin Xu, Eric Murphy, Hanae Inami, Lee Armus, Loreto Barcos-Munoz, Nanyao Lu, Paul van der Werf, Philip Appleton, Tanio Diaz-Santos, Vassilis Charmandaris, Yinghe Zhao, Yu Gao","submitted_at":"2016-02-23T07:49:20Z","abstract_excerpt":"In this paper, we report our high-resolution ($0^{\\prime\\prime}.20\\times0^{\\prime\\prime}.14$ or $\\sim$$70\\times49$ pc) observations of the CO(6-5) line emission, which probes warm and dense molecular gas, and the 434 $\\mu$m dust continuum in the nuclear region of NGC 7130, obtained with the Atacama Large Millimeter Array (ALMA). The CO line and dust continuum fluxes detected in our ALMA observations are $1230\\pm74$ Jy km s$^{-1}$ and $814\\pm52$ mJy, respectively, which account for 100% and 51% of their total respective fluxes. We find that the CO(6-5) and dust emissions are generally spatially"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.07070","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"}