{"paper":{"title":"The far-infrared spectrum of Arp 220","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Dpto. Astrof\\'isica Molecular e Infrarroja), Eduardo Gonz\\'alez-Alfonso (Universidad de Alcal\\'a de Henares), Howard A. Smith (Harvard-Smithsonian Center for Astrophysics), Jacqueline Fischer (Naval Research Laboratory), Jos\\'e Cernicharo (CSIC","submitted_at":"2004-06-18T18:03:50Z","abstract_excerpt":"ISO/LWS grating observations of the ultraluminous infrared galaxy Arp 220 shows absorption in molecular lines of OH, H$_2$O, CH, NH, and NH$_3$, as well as in the [O I] 63 $\\mu$m line and emission in the [C II] 158 $\\mu$m line. We have modeled the continuum and the emission/absorption of all observed features by means of a non-local radiative transfer code. The continuum from 25 to 1300 $\\mu$m is modeled as a warm (106 K) nuclear region that is optically thick in the far-infrared, attenuated by an extended region (size 2$''$) that is heated mainly through absorption of nuclear infrared radiati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0406427","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"}