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dc.contributor.authorKaviraj, S.
dc.contributor.authorDevriendt, J.
dc.contributor.authorDubois, Y.
dc.contributor.authorSlyz, A.
dc.contributor.authorWelker, C.
dc.contributor.authorPichon, C.
dc.contributor.authorPeirani, S.
dc.contributor.authorBorgne, D. Le
dc.date.accessioned2017-07-19T16:37:22Z
dc.date.available2017-07-19T16:37:22Z
dc.date.issued2015-09-21
dc.identifier.citationKaviraj , S , Devriendt , J , Dubois , Y , Slyz , A , Welker , C , Pichon , C , Peirani , S & Borgne , D L 2015 , ' Galaxy merger histories and the role of merging in driving star formation at z >1 ' , Monthly Notices of the Royal Astronomical Society , vol. 452 , no. 3 , pp. 2845-2850 . https://doi.org/10.1093/mnras/stv1500
dc.identifier.issn1365-2966
dc.identifier.otherPURE: 10376386
dc.identifier.otherPURE UUID: 4d804530-f0c3-4756-a42e-b590bc7772b9
dc.identifier.otherArXiv: http://arxiv.org/abs/1411.2595v1
dc.identifier.otherScopus: 84945263047
dc.identifier.urihttp://hdl.handle.net/2299/19002
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
dc.description.abstractWe use Horizon-AGN, a hydrodynamical cosmological simulation, to explore the role of mergers in the evolution of massive (M > 10^10 MSun) galaxies around the epoch of peak cosmic star formation (1zR(4:1 3 are 'blue' (i.e. have significant associated star formation), the proportion of 'red' mergers increases rapidly at ztodays stellar mass was formed.en
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.subjectastro-ph.GA
dc.titleGalaxy merger histories and the role of merging in driving star formation at z>1en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2015-09-21
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stv1500
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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