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Mapping the interstellar medium in galaxies with Herschel/SPIRE

dc.contributor.authorEales, S. A.
dc.contributor.authorSmith, M. W. L.
dc.contributor.authorWilson, C. D.
dc.contributor.authorBendo, G. J.
dc.contributor.authorCortese, L.
dc.contributor.authorPohlen, M.
dc.contributor.authorBoselli, A.
dc.contributor.authorGomez, H. L.
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-Rodríguez, 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.authorDavies, J. I.
dc.contributor.authorDwek, E.
dc.contributor.authorElbaz, D.
dc.contributor.authorGalametz, M.
dc.contributor.authorGalliano, F.
dc.contributor.authorGear, W. K.
dc.contributor.authorGlenn, J.
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.authorPérez-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.authorSauvage, M.
dc.contributor.authorSchulz, B.
dc.contributor.authorSchirm, M. R. P.
dc.contributor.authorSpinoglio, L.
dc.contributor.authorSrinivasan, S.
dc.contributor.authorStevens, Jason
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.accessioned2012-01-31T10:01:05Z
dc.date.available2012-01-31T10:01:05Z
dc.date.issued2010-07-01
dc.identifier.citationEales , S A , Smith , M W L , Wilson , C D , Bendo , G J , Cortese , L , Pohlen , M , Boselli , A , Gomez , H L , Auld , R , Baes , M , Barlow , M J , Bock , J J , Bradford , M , Buat , V , Castro-Rodríguez , N , Chanial , P , Charlot , S , Ciesla , L , Clements , D L , Cooray , A , Cormier , D , Davies , J I , Dwek , E , Elbaz , D , Galametz , M , Galliano , F , Gear , W K , Glenn , J , 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 , Pérez-Fournon , I , Rangwala , N , Rigby , E E , Roussel , H , Rykala , A , Sacchi , N , Sauvage , M , Schulz , B , Schirm , M R P , Spinoglio , L , Srinivasan , S , Stevens , J , Symeonidis , M , Trichas , M , Vaccari , M , Vigroux , L , Wozniak , H , Wright , G S & Zeilinger , W W 2010 , ' Mapping the interstellar medium in galaxies with Herschel/SPIRE ' , Astronomy and Astrophysics , vol. 518 , L62 . https://doi.org/10.1051/0004-6361/201014536
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 517421
dc.identifier.otherPURE UUID: 8bdf0421-d6a4-42d1-b1f9-760240eeb66b
dc.identifier.otherBibtex: urn:db6051789eb4c5f474dc4ceced1f07e9
dc.identifier.otherScopus: 77957813887
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747539
dc.identifier.urihttp://hdl.handle.net/2299/7751
dc.description.abstractThe standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter, we use SPIRE observations of the galaxies M 99 and M 100 to explore the alternative approach of mapping the interstellar medium using the continuum emission from the dust. We have compared the methods by measuring the relationship between the star-formation rate and the surface density of gas in the galaxies using both methods. We find the two methods give relationships with a similar dispersion, confirming that observing the continuum emission from the dust is a promising method of mapping the interstellar medium in galaxies.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.subjectgalaxies: ISM, galaxies: spiral, dust, extinction, ISM: abundances
dc.titleMapping the interstellar medium in galaxies with Herschel/SPIREen
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/10.1051/0004-6361/201014536
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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