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dc.contributor.authorAlatalo, Katherine
dc.contributor.authorNyland, Kristina
dc.contributor.authorGraves, Genevieve
dc.contributor.authorDeustua, Susana
dc.contributor.authorShapiro Griffin, Kristen
dc.contributor.authorDuc, Pierre-Alain
dc.contributor.authorCappellari, Michele
dc.contributor.authorMcDermid, Richard M.
dc.contributor.authorDavis, Timothy A.
dc.contributor.authorCrocker, Alison F.
dc.contributor.authorYoung, Lisa M.
dc.contributor.authorChang, Philip
dc.contributor.authorScott, Nicholas
dc.contributor.authorCales, Sabrina L.
dc.contributor.authorBayet, Estelle
dc.contributor.authorBlitz, Leo
dc.contributor.authorBois, Maxime
dc.contributor.authorBournaud, Frédéric
dc.contributor.authorBureau, Martin
dc.contributor.authorDavies, Roger L.
dc.contributor.authorde Zeeuw, P. T.
dc.contributor.authorEmsellem, Eric
dc.contributor.authorKhochfar, Sadegh
dc.contributor.authorKrajnović, Davor
dc.contributor.authorKuntschner, Harald
dc.contributor.authorMorganti, Raffaella
dc.contributor.authorNaab, Thorsten
dc.contributor.authorOosterloo, Tom
dc.contributor.authorSarzi, Marc
dc.contributor.authorSerra, Paolo
dc.contributor.authorWeijmans, Anne-Marie
dc.date.accessioned2014-09-18T14:31:01Z
dc.date.available2014-09-18T14:31:01Z
dc.date.issued2013-12-23
dc.identifier.citationAlatalo , K , Nyland , K , Graves , G , Deustua , S , Shapiro Griffin , K , Duc , P-A , Cappellari , M , McDermid , R M , Davis , T A , Crocker , A F , Young , L M , Chang , P , Scott , N , Cales , S L , Bayet , E , Blitz , L , Bois , M , Bournaud , F , Bureau , M , Davies , R L , de Zeeuw , P T , Emsellem , E , Khochfar , S , Krajnović , D , Kuntschner , H , Morganti , R , Naab , T , Oosterloo , T , Sarzi , M , Serra , P & Weijmans , A-M 2013 , ' NGC 1266 as a local candidate for rapid cessation of star formation ' , Astrophysical Journal , vol. 780 , no. 2 , 186 . https://doi.org/10.1088/0004-637X/780/2/186en
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 144053336
dc.identifier.otherPURE UUID: f0408675-2ece-4919-906d-d14c1ee2e5ef
dc.identifier.otherBibCode: 2014ApJ...780..186A
dc.identifier.otherScopus: 84891277712
dc.identifier.otherORCID: /0000-0002-5908-6852/work/40233455
dc.identifier.urihttp://hdl.handle.net/10023/5448
dc.description.abstractWe present new Spectrographic Areal Unit for Research on Optical Nebulae (SAURON) integral-field spectroscopy and Swift Ultraviolet Optical Telescope (UVOT) observations of molecular outflow host galaxy NGC 1266 that indicate NGC 1266 has experienced a rapid cessation of star formation. Both the SAURON maps of stellar population age and the Swift UVOT observations demonstrate the presence of young (~ 1 Gyr by cyclically injecting turbulent energy into the dense molecular gas via a radio jet, inhibiting star formation.
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2013. The American Astronomical Society. All rights reserved. This is an Accepted Manuscript of an article published online in the Astrophysical Journal on 23 December 2013, available online: http://iopscience.iop.org/0004-637X/780/2/186/en
dc.subjectGalaxies: activeen
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: individual: NGC 1266en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleNGC 1266 as a local candidate for rapid cessation of star formationen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1088/0004-637X/780/2/186
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2014ApJ...780..186Aen


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