{"paper":{"title":"FIR colours and SEDs of nearby galaxies observed with Herschel","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Boselli, A. Cooray, A. Dariush, A. Jones, A. Papageorgiou, A. Rykala, B. O'Halloran, B. Schulz, C. Giovanardi, C. Vlahakis, C. Wilson, D.A. Garcia-Appadoo, D. Clements, D. Cormier, D. Elbaz, D. Fadda, D.J. Bomans, D. Pierini, E. Corbelli, E. Dwek, E.M. Xilouris, E. Rigby, F. Galliano, G. Gavazzi, G. J. Bendo, G. Wright, H. Gomez, H. Roussel, H. Wozniak, I. De Looze, I. Perez-Fournon, J. Bock, J. Davies, J. Fritz, J. Glenn, J. Stevens, J. Verstappen, K. Isaak, K. Okumura, L. Ciesla, L. Cortese, L. Hunt, L. Levenson, L. Spinoglio, L. Vigroux, M. Baes, M. Bradford, M. Clemens, M. Galametz, M. Griffin, M. Grossi, M. Page, M. Pohlen, M. Sauvage, M. Schirm, M. Symeonidis, M. Trichas, M. Vaccari, M.W.L. Smith, N. Castro-Rodriguez, N. Lu, N. Rangwala, N. Sacchi, P. Chanial, P. Panuzzo, R. Auld, S. Bianchi, S. Charlot, S.C. Madden, S. di Serego Alighieri, S. Eales, S. Hony, S. Oliver, S. Sabatini, S. Sundar, S. Zibetti, T.M. Hughes, T. Parkin, V. Buat, W. Gear, W. Zeilinger","submitted_at":"2010-05-10T13:30:57Z","abstract_excerpt":"We present infrared colours (in the 25-500 mic spectral range) and UV to radio continuum spectral energy distributions of a sample of 51 nearby galaxies observed with SPIRE on Herschel. The observed sample includes all morphological classes, from quiescent ellipticals to active starbursts. Active galaxies have warmer colour temperatures than normal spirals. In ellipticals hosting a radio galaxy, the far-infrared (FIR) emission is dominated bynthe synchrotron nuclear emission. The colour temperature of the cold dust is higher in quiescent E-S0a than in star-forming systems probably because of t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.1537","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"}