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dc.contributor.authorCortese, L.
dc.contributor.authorBendo, G. J.
dc.contributor.authorBoselli, A.
dc.contributor.authorDavies, J. I.
dc.contributor.authorGomez, H. L.
dc.contributor.authorPohlen, M.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
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.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.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.authorSauvage, M.
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.authorWilson, C. D.
dc.contributor.authorWozniak, H.
dc.contributor.authorWright, G. S.
dc.contributor.authorZeilinger, W. W.
dc.date.accessioned2012-01-31T10:01:08Z
dc.date.available2012-01-31T10:01:08Z
dc.date.issued2010-07-01
dc.identifier.citationCortese , L , Bendo , G J , Boselli , A , Davies , J I , Gomez , H L , Pohlen , M , Auld , R , Baes , M , Bock , J J , Bradford , M , Buat , V , Castro-Rodriguez , N , Chanial , P , Charlot , S , Ciesla , L , Clements , D L , Cooray , A , Cormier , D , Dwek , E , Eales , S A , 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 , Perez-Fournon , I , Rangwala , N , Rigby , E E , Roussel , H , Rykala , A , Sacchi , N , Sauvage , M , Schulz , B , Schirm , M R P , Smith , M W L , Spinoglio , L , Stevens , J , Srinivasan , S , Symeonidis , M , Trichas , M , Vaccari , M , Vigroux , L , Wilson , C D , Wozniak , H , Wright , G S & Zeilinger , W W 2010 , ' Herschel-SPIRE observations of the disturbed galaxy NGC 4438 ' , Astronomy and Astrophysics , vol. 518 , L63 . https://doi.org/10.1051/0004-6361/201014547
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 517667
dc.identifier.otherPURE UUID: 0aa864df-1b7b-4b36-a905-fd181f30972c
dc.identifier.otherBibtex: urn:35b5ad50a1b5ec1c15e900a203564959
dc.identifier.otherScopus: 77957773428
dc.identifier.otherORCID: /0000-0002-4010-8310/work/62747679
dc.identifier.urihttp://hdl.handle.net/2299/7752
dc.description.abstractWe present Herschel-SPIRE observations of the perturbed galaxy NGC 4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4–5 kpc away from the galaxy's disk. The dust closely follows the distribution of the stripped atomic and molecular hydrogen, supporting the idea that gas and dust are perturbed in a similar fashion by the cluster environment. Interestingly, the extra-planar dust lacks a warm temperature component when compared to the material still present in the disk, explaining why it was missed by previous far-infrared investigations. Our study provides evidence for dust stripping in clusters of galaxies and illustrates the potential of Herschel data for our understanding of environmental effects on galaxy evolution.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.subjectgalaxies: evolution, galaxies: individual: NGC 4438, infrared: galaxies, dust, extinction
dc.titleHerschel-SPIRE observations of the disturbed galaxy NGC 4438en
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/10.1051/0004-6361/201014547
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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