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dc.contributor.authorBendo, G. J.
dc.contributor.authorWilson, C. D.
dc.contributor.authorPohlen, M.
dc.contributor.authorSauvage, M.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorBarlow, M.J.
dc.contributor.authorBock, J. J.
dc.contributor.authorBoselli, A.
dc.contributor.authorBradford, M.
dc.contributor.authorBuat, V.
dc.contributor.authorCastro-Rodriguez, N.
dc.contributor.authorChanial, P.
dc.contributor.authorCharlot, S.
dc.contributor.authorCiesla, L.
dc.contributor.authorClements, D. L.
dc.contributor.authorCooray, A.
dc.contributor.authorCormier, D.
dc.contributor.authorCortese, L.
dc.contributor.authorDavies, J.I.
dc.contributor.authorDwek, E.
dc.contributor.authorEales, S.A.
dc.contributor.authorElbaz, D.
dc.contributor.authorGalametz, M.
dc.contributor.authorGalliano, F.
dc.contributor.authorGear, W.K.
dc.contributor.authorGlenn, J.
dc.contributor.authorGomez, H.L.
dc.contributor.authorGriffin, M.
dc.contributor.authorHony, S.
dc.contributor.authorIsaak, K.G.
dc.contributor.authorLevenson, L. R.
dc.contributor.authorLu, N.
dc.contributor.authorMadden, S.
dc.contributor.authorO'Halloran, B.
dc.contributor.authorOkumura, K.
dc.contributor.authorOliver, S.
dc.contributor.authorPage, M. J.
dc.contributor.authorPanuzzo, P.
dc.contributor.authorPapageorgiou, A.
dc.contributor.authorParkin, T.J.
dc.contributor.authorPerez-Fournon, I.
dc.contributor.authorRangwala, N.
dc.contributor.authorRigby, E. E.
dc.contributor.authorRoussel, H.
dc.contributor.authorRykala, A.
dc.contributor.authorSacchi, N.
dc.contributor.authorSchulz, B.
dc.contributor.authorSchirm, M. R. P.
dc.contributor.authorSmith, M. W. L.
dc.contributor.authorSpinoglio, L.
dc.contributor.authorStevens, Jason
dc.contributor.authorSundar, S.
dc.contributor.authorSymeonidis, M.
dc.contributor.authorTrichas, M.
dc.contributor.authorVaccari, M.
dc.contributor.authorVigroux, L.
dc.contributor.authorWozniak, H.
dc.contributor.authorWright, G. S.
dc.contributor.authorZeilinger, W.W.
dc.date.accessioned2012-01-31T13:01:00Z
dc.date.available2012-01-31T13:01:00Z
dc.date.issued2010-07-01
dc.identifier.citationBendo , G J , Wilson , C D , Pohlen , M , Sauvage , M , Auld , R , Baes , M , Barlow , M J , Bock , J J , Boselli , A , Bradford , M , Buat , V , Castro-Rodriguez , N , Chanial , P , Charlot , S , Ciesla , L , Clements , D L , Cooray , A , Cormier , D , Cortese , L , Davies , J I , Dwek , E , Eales , S A , Elbaz , D , Galametz , M , Galliano , F , Gear , W K , Glenn , J , Gomez , H L , Griffin , M , Hony , S , Isaak , K G , Levenson , L R , Lu , N , Madden , S , O'Halloran , B , Okumura , K , Oliver , S , Page , M J , Panuzzo , P , Papageorgiou , A , Parkin , T J , Perez-Fournon , I , Rangwala , N , Rigby , E E , Roussel , H , Rykala , A , Sacchi , N , Schulz , B , Schirm , M R P , Smith , M W L , Spinoglio , L , Stevens , J , Sundar , S , Symeonidis , M , Trichas , M , Vaccari , M , Vigroux , L , Wozniak , H , Wright , G S & Zeilinger , W W 2010 , ' The Herschel Space Observatory view of dust in M81 ' , Astronomy and Astrophysics , vol. 518 , L65 . https://doi.org/10.1051/0004-6361/201014568
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 517157
dc.identifier.otherPURE UUID: 56e75a27-2409-4596-bafe-45924d0e2c1f
dc.identifier.otherBibtex: urn:e0a7d11eb4e9d053c72ba146821be1b2
dc.identifier.otherScopus: 77957761390
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747626
dc.identifier.urihttp://hdl.handle.net/2299/7759
dc.description.abstractWe use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70–500 μm in the nearby spiral galaxy M81. We find that the ratios of wave bands between 160 and 500 μm are primarily dependent on radius but that the ratio of 70 to 160 μm emission shows no clear dependence on surface brightness or radius. These results along with analyses of the spectral energy distributions imply that the 160–500 μm emission traces 15–30 K dust heated by evolved stars in the bulge and disc whereas the 70 μm emission includes dust heated by the active galactic nucleus and young stars in star forming regions.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rightsOpen
dc.subjectgalaxies: ISM, galaxies: spiral, galaxies: individual: M81
dc.titleThe Herschel Space Observatory view of dust in M81en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2010-07-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201014568
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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