{"paper":{"title":"Multiline observations of S255IR with ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(2) Institute of Astronomy, Academia Sinica, Astrophysics, Igor Zinchenko (1), Nizhny Novgorod, Petr Zemlyanukha (1) ((1) Institute of Applied Physics of the Russian Academy of Sciences, Russia, Sheng-Yuan Liu (2), Taipei, Taiwan), Yu-Nung Su (2)","submitted_at":"2017-11-16T05:45:36Z","abstract_excerpt":"We present preliminary results of the high resolution $ (0.10^{\\prime\\prime} \\times 0.15^{\\prime\\prime}) $ observations of the high mass star forming region S255IR with ALMA in several spectral windows from ~ 335 GHz to ~ 350 GHz. The main target lines were C$^{34}$S(7-6), CH$_3$CN($19_K-18_K$), CO(3-2) and SiO(8-7), however many other lines of various molecules have been detected, too. We present sample spectra and maps, discuss briefly the source structure and kinematics. A new, never predicted methanol maser line has been discovered."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.05936","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"}