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dc.contributor.authorKelvin, Lee S.
dc.contributor.authorBremer, Malcolm N.
dc.contributor.authorPhillipps, Steven
dc.contributor.authorJames, Philip A.
dc.contributor.authorDavies, Luke J. M.
dc.contributor.authorPropris, Roberto De
dc.contributor.authorMoffett, Amanda J.
dc.contributor.authorPercival, Susan M.
dc.contributor.authorBaldry, Ivan K.
dc.contributor.authorCollins, Chris A.
dc.contributor.authorAlpaslan, Mehmet
dc.contributor.authorBland-Hawthorn, Joss
dc.contributor.authorBrough, Sarah
dc.contributor.authorCluver, Michelle
dc.contributor.authorDriver, Simon P.
dc.contributor.authorHashemizadeh, Abdolhosein
dc.contributor.authorHolwerda, Benne W.
dc.contributor.authorLaine, Jarkko
dc.contributor.authorLara-Lopez, Maritza A.
dc.contributor.authorLiske, Jochen
dc.contributor.authorMaciejewski, Witold
dc.contributor.authorNapolitano, Nicola R.
dc.contributor.authorPenny, Samantha J.
dc.contributor.authorPopescu, Cristina C.
dc.contributor.authorSansom, Anne E.
dc.contributor.authorSutherland, Will
dc.contributor.authorTaylor, Edward N.
dc.contributor.authorKampen, Eelco van
dc.contributor.authorWang, Lingyu
dc.date.accessioned2018-04-27T09:30:14Z
dc.date.available2018-04-27T09:30:14Z
dc.date.issued2018-07
dc.identifier.citationKelvin , L S , Bremer , M N , Phillipps , S , James , P A , Davies , L J M , Propris , R D , Moffett , A J , Percival , S M , Baldry , I K , Collins , C A , Alpaslan , M , Bland-Hawthorn , J , Brough , S , Cluver , M , Driver , S P , Hashemizadeh , A , Holwerda , B W , Laine , J , Lara-Lopez , M A , Liske , J , Maciejewski , W , Napolitano , N R , Penny , S J , Popescu , C C , Sansom , A E , Sutherland , W , Taylor , E N , Kampen , E V & Wang , L 2018 , ' Galaxy and Mass Assembly (GAMA) : variation in galaxy structure across the green valley ' , Monthly Notices of the Royal Astronomical Society , vol. 477 , no. 3 , pp. 4116-4130 . https://doi.org/10.1093/mnras/sty933en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 252910754
dc.identifier.otherPURE UUID: b0489c4a-608c-4e6e-91df-662231be0410
dc.identifier.otherArXiv: http://arxiv.org/abs/1804.04470v1
dc.identifier.otherScopus: 85047936073
dc.identifier.otherWOS: 000433893700090
dc.identifier.urihttps://hdl.handle.net/10023/13246
dc.description.abstractUsing a sample of 472 local Universe (z < 0.06) galaxies in the stellar mass range 10. 25 < log M*/Mʘ < 10.75, we explore the variation in galaxy structure as a function of morphology and galaxy colour. Our sample of galaxies is sub-divided into red, green and blue colour groups and into elliptical and non-elliptical (disk-type) morphologies. Using KiDS and VIKING derived postage stamp images, a group of eight volunteers visually classified bars, rings, morphological lenses, tidal streams, shells and signs of merger activity for all systems. We find a significant surplus of rings(2.3σ) and lenses (2.9σ) in disk-type galaxies as they transition across the green valley. Combined, this implies a joint ring/lens green valley surplus significance of 3.3σ relative to equivalent disk-types within either the blue cloud or the red sequence. We recover a bar fraction of ∼44% which remains flat with colour, however, we find that the presence of a bar acts to modulate the incidence of rings and (to a lesser extent) lenses, with rings in barred disk-type galaxies more common by ∼ 20−30 percentage points relative to their unbarred counterparts, regardless of colour. Additionally, green valley disk-type galaxies with a bar exhibit a significant 3.0σ surplus of lenses relative to their blue/red analogues. The existence of such structures rules out violent transformative events as the primary end-of-life evolutionary mechanism, with a more passive scenario the favoured candidate for the majority of galaxies rapidly transitioning across the green valley.
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1093/mnras/sty933en
dc.subjectGalaxies: elliptical and lenticular, cDen
dc.subjectGalaxies: spiralen
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: star formationen
dc.subjectGalaxies: statisticsen
dc.subjectGalaxies: structureen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleGalaxy and Mass Assembly (GAMA) : variation in galaxy structure across the green valleyen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/sty933
dc.description.statusPeer revieweden


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