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The central region of spiral galaxies as seen by Herschel. M 81, M 99, and M 100

dc.contributor.authorSauvage, M.
dc.contributor.authorSacchi, N.
dc.contributor.authorBendo, G. J.
dc.contributor.authorBoselli, A.
dc.contributor.authorPohlen, M.
dc.contributor.authorWilson, C. D.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorBarlow, M. J.
dc.contributor.authorBock, J. J.
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. C.
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.authorSchulz, B.
dc.contributor.authorSchirm, M. R. P.
dc.contributor.authorSmith, M. W. L.
dc.contributor.authorSpinoglio, L.
dc.contributor.authorStevens, Jason
dc.contributor.authorSrinivasan, 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.accessioned2012-02-21T17:47:20Z
dc.date.available2012-02-21T17:47:20Z
dc.date.issued2010-07-01
dc.identifier.citationSauvage , M , Sacchi , N , Bendo , G J , Boselli , A , Pohlen , M , Wilson , C D , Auld , R , Baes , M , Barlow , M J , Bock , J J , 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 C , 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 , Schulz , B , Schirm , M R P , Smith , M W L , Spinoglio , L , Stevens , J , Srinivasan , S , Symeonidis , M , Trichas , M , Vaccari , M , Vigroux , L , Wozniak , H , Wright , G S & Zeilinger , W W 2010 , ' The central region of spiral galaxies as seen by Herschel. M 81, M 99, and M 100 ' , Astronomy & Astrophysics , vol. 518 , L64 . https://doi.org/10.1051/0004-6361/201014588
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 517542
dc.identifier.otherPURE UUID: 53f0c3a8-90eb-4948-9381-e913f97f068f
dc.identifier.otherBibtex: urn:747bb818845bc5909354d0641aabf9ce
dc.identifier.otherScopus: 77957762399
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747543
dc.identifier.urihttp://hdl.handle.net/2299/7853
dc.description.abstractWith appropriate spatial resolution, images of spiral galaxies in thermal infrared (~10 micron and beyond) often reveal a bright central component, distinct from the stellar bulge, superimposed on a disk with prominent spiral arms. ISO and Spitzer studies have shown that much of the scatter in the mid-infrared colors of spiral galaxies is related to changes in the relative importance of these two components, rather than to other modifications, such as the morphological type or star formation rate, that affect the properties of the galaxy as a whole. With the Herschel imaging capability from 70 to 500 micron, we revisit this two-component approach at longer wavelengths, to see if it still provides a working description of the brightness distribution of galaxies, and to determine its implications on the interpretation of global far-infrared properties of galaxies.en
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.subjectinfrared: galaxies, submillimeter: galaxies, galaxies:, spiral, galaxies: nuclei, galaxies: fundamental parameters
dc.titleThe central region of spiral galaxies as seen by Herschel. M 81, M 99, and M 100en
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/10.1051/0004-6361/201014588
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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