{"paper":{"title":"Cold gas dynamics in Hydra-A: evidence for a rotating disk","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. C. Edge, A. C. Fabian, A. M. Swinbank, B. R. McNamara, C. L. Sarazin, C. P. O'Dea, F. Combes, G. J. Ferland, G. Tremblay, H. R. Russell, J. B. R. Oonk, M. Donahue, M. N. Bremer, N. P. H. Nesvadba, P. Salom\\'e, R. Mittal, S. A. Baum, S. L. Hamer","submitted_at":"2013-10-16T20:00:03Z","abstract_excerpt":"We present multi-frequency observations of the radio galaxy Hydra-A (3C218) located in the core of a massive, X-ray luminous galaxy cluster. IFU spectroscopy is used to trace the kinematics of the ionised and warm molecular hydrogen which are consistent with a ~ 5 kpc rotating disc. Broad, double-peaked lines of CO(2-1), [CII]157 $\\mu$m and [OI]63 $\\mu$m are detected. We estimate the mass of the cold gas within the disc to be M$_{gas}$ = 2.3 $\\pm$ 0.3 x 10$^9$ M$_{\\odot}$. These observations demonstrate that the complex line profiles found in the cold atomic and molecular gas are related to th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.4501","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"}