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dc.contributor.authorBoselli, A.
dc.contributor.authorCiesla, L.
dc.contributor.authorBuat, V.
dc.contributor.authorCortese, L.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorBendo, G. J.
dc.contributor.authorBianchi, S.
dc.contributor.authorBock, J.
dc.contributor.authorBomans, D. J.
dc.contributor.authorBradford, M.
dc.contributor.authorCastro-Rodriguez, N.
dc.contributor.authorChanial, P.
dc.contributor.authorCharlot, S.
dc.contributor.authorClemens, M.
dc.contributor.authorClements, D.
dc.contributor.authorCorbelli, E.
dc.contributor.authorCooray, A.
dc.contributor.authorCormier, D.
dc.contributor.authorDariush, A.
dc.contributor.authorDavies, J.
dc.contributor.authorde Looze, I.
dc.contributor.authordi Serego Alighieri, S.
dc.contributor.authorDwek, E.
dc.contributor.authorEales, S.
dc.contributor.authorElbaz, D.
dc.contributor.authorFadda, D.
dc.contributor.authorFritz, J.
dc.contributor.authorGalametz, M.
dc.contributor.authorGalliano, F.
dc.contributor.authorGarcia-Appadoo, D. A.
dc.contributor.authorGavazzi, G.
dc.contributor.authorGear, W.
dc.contributor.authorGiovanardi, C.
dc.contributor.authorGlenn, J.
dc.contributor.authorGomez, H.
dc.contributor.authorGriffin, M.
dc.contributor.authorGrossi, M.
dc.contributor.authorHony, S.
dc.contributor.authorHughes, T. M.
dc.contributor.authorHunt, L.
dc.contributor.authorIsaak, K.
dc.contributor.authorJones, A.
dc.contributor.authorLevenson, L.
dc.contributor.authorLu, N.
dc.contributor.authorMadden, S. C.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOkumura, K.
dc.contributor.authorOliver, S.
dc.contributor.authorPage, M.
dc.contributor.authorPanuzzo, P.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorParkin, T.
dc.contributor.authorPerez-Fournon, I.
dc.contributor.authorPierini, D.
dc.contributor.authorPohlen, M.
dc.contributor.authorRangwala, N.
dc.contributor.authorRigby, E.
dc.contributor.authorRoussel, H.
dc.contributor.authorRykala, A.
dc.contributor.authorSabatini, S.
dc.contributor.authorSacchi, N.
dc.contributor.authorSauvage, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorSchirm, M.
dc.contributor.authorSmith, M. W. L.
dc.contributor.authorSpinoglio, L.
dc.contributor.authorStevens, J.
dc.contributor.authorSundar, S.
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTrichas, M.
dc.contributor.authorVaccari, M.
dc.contributor.authorVerstappen, J.
dc.contributor.authorVigroux, L.
dc.contributor.authorVlahakis, C.
dc.contributor.authorWilson, C.
dc.contributor.authorWozniak, H.
dc.contributor.authorWright, G.
dc.contributor.authorXilouris, E. M.
dc.contributor.authorZeilinger, W.
dc.contributor.authorZibetti, S.
dc.date.accessioned2012-01-18T12:01:05Z
dc.date.available2012-01-18T12:01:05Z
dc.date.issued2010-07-01
dc.identifier.citationBoselli , A , Ciesla , L , Buat , V , Cortese , L , Auld , R , Baes , M , Bendo , G J , Bianchi , S , Bock , J , Bomans , D J , Bradford , M , Castro-Rodriguez , N , Chanial , P , Charlot , S , Clemens , M , Clements , D , Corbelli , E , Cooray , A , Cormier , D , Dariush , A , Davies , J , de Looze , I , di Serego Alighieri , S , Dwek , E , Eales , S , Elbaz , D , Fadda , D , Fritz , J , Galametz , M , Galliano , F , Garcia-Appadoo , D A , Gavazzi , G , Gear , W , Giovanardi , C , Glenn , J , Gomez , H , Griffin , M , Grossi , M , Hony , S , Hughes , T M , Hunt , L , Isaak , K , Jones , A , Levenson , L , Lu , N , Madden , S C , O'Halloran , B , Okumura , K , Oliver , S , Page , M , Panuzzo , P , Papageorgiou , A , Parkin , T , Perez-Fournon , I , Pierini , D , Pohlen , M , Rangwala , N , Rigby , E , Roussel , H , Rykala , A , Sabatini , S , Sacchi , N , Sauvage , M , Schulz , B , Schirm , M , Smith , M W L , Spinoglio , L , Stevens , J , Sundar , S , Symeonidis , M , Trichas , M , Vaccari , M , Verstappen , J , Vigroux , L , Vlahakis , C , Wilson , C , Wozniak , H , Wright , G , Xilouris , E M , Zeilinger , W & Zibetti , S 2010 , ' FIR colours and SEDs of nearby galaxies observed with Herschel ' , Astronomy and Astrophysics , vol. 518 , L61 . https://doi.org/10.1051/0004-6361/201014534
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 517998
dc.identifier.otherPURE UUID: b0cd3ff4-f1d7-4e80-a6d9-87ef4d23ba70
dc.identifier.otherBibtex: urn:5d1fe8c9188153ebfbcaf5e3d71b48af
dc.identifier.otherScopus: 77957765221
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747578
dc.identifier.urihttp://hdl.handle.net/2299/7681
dc.description.abstractWe present infrared colours (in the 25–500 μm 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 by the synchrotron nuclear emission. The colour temperature of the cold dust is higher in quiescent E-S0a than in star-forming systems probably because of the different nature of their dust heating sources (evolved stellar populations, X-ray, fast electrons) and dust grain properties. In contrast to the colour temperature of the warm dust, the f350/f500 index sensitive to the cold dust decreases with star formation and increases with metallicity, suggesting an overabundance of cold dust or an emissivity parameter β < 2 in low metallicity, active systems.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.subjectgalaxies: ISM, galaxies: spiral, galaxies: elliptical and lenticular, cD, infrared: galaxies
dc.titleFIR colours and SEDs of nearby galaxies observed with Herschelen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201014534
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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