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dc.contributor.authorWillett, Kyle W.
dc.contributor.authorSchawinski, Kevin
dc.contributor.authorSimmons, Brooke D.
dc.contributor.authorMasters, Karen L.
dc.contributor.authorSkibba, Ramin A.
dc.contributor.authorKaviraj, Sugata
dc.contributor.authorMelvin, Thomas
dc.contributor.authorWong, O. Ivy
dc.contributor.authorNichol, Robert C.
dc.contributor.authorCheung, Edmond
dc.contributor.authorLintott, Chris J.
dc.contributor.authorFortson, Lucy
dc.date.accessioned2020-01-23T01:10:55Z
dc.date.available2020-01-23T01:10:55Z
dc.date.issued2015-03-19
dc.identifier.citationWillett , K W , Schawinski , K , Simmons , B D , Masters , K L , Skibba , R A , Kaviraj , S , Melvin , T , Wong , O I , Nichol , R C , Cheung , E , Lintott , C J & Fortson , L 2015 , ' Galaxy Zoo : the dependence of the star formation-stellar mass relation on spiral disk morphology ' , Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/stv307
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 18991551
dc.identifier.otherPURE UUID: 0ffe5443-ba89-4f37-88aa-46665c800d82
dc.identifier.otherArXiv: http://arxiv.org/abs/1502.03444v1
dc.identifier.otherScopus: 84930830339
dc.identifier.otherORCID: /0000-0002-5601-575X/work/77850201
dc.identifier.urihttp://hdl.handle.net/2299/22111
dc.description© 2015 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. Code and data are available at https://github.com/willettk/gzmainsequence
dc.description.abstractWe measure the stellar mass-star formation rate relation in star-forming disk galaxies at z1. Of the galaxies lying significantly above the M-SFR relation in the local Universe, more than 50% are mergers. We interpret this as evidence that the spiral arms, which are imperfect reflections of the galaxy's current gravitational potential, are either fully independent of the various quenching mechanisms or are completely overwhelmed by the combination of outflows and feedback. The arrangement of the star formation can be changed, but the system as a whole regulates itself even in the presence of strong dynamical forcing.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.GA
dc.titleGalaxy Zoo : the dependence of the star formation-stellar mass relation on spiral disk morphologyen
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.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stv307
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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