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dc.contributor.authorTamburro, D.
dc.contributor.authorRix, H-W.
dc.contributor.authorWalter, F.
dc.contributor.authorBrinks, E.
dc.contributor.authorde Blok, W.J.G.
dc.contributor.authorKennicutt, R.C.
dc.contributor.authorMac Low, M.M.
dc.date.accessioned2008-12-17T14:29:06Z
dc.date.available2008-12-17T14:29:06Z
dc.date.issued2008
dc.identifier.citationTamburro , D , Rix , H-W , Walter , F , Brinks , E , de Blok , W J G , Kennicutt , R C & Mac Low , M M 2008 , ' Geometrically derived timescales for star formation in spiral galaxies ' , The Astronomical Journal , vol. 136 , no. 6 , pp. 2872-2885 . https://doi.org/10.1088/0004-6256/136/6/2872
dc.identifier.issn0004-6256
dc.identifier.otherPURE: 148494
dc.identifier.otherPURE UUID: 9b60198b-60ac-43d2-8548-afc5ba3569e6
dc.identifier.otherdspace: 2299/2706
dc.identifier.otherScopus: 59449097215
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407849
dc.identifier.urihttp://hdl.handle.net/2299/2706
dc.descriptionOriginal article can be found at: http://www.iop.org/EJ/journal/aj Copyright American Astronomical Society DOI: 10.1088/0004-6256/136/6/2872 [Full text of this article is not available in the UHRA]
dc.language.isoeng
dc.relation.ispartofThe Astronomical Journal
dc.titleGeometrically derived timescales for star formation in spiral galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-6256/136/6/2872
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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