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dc.contributor.authorCioni, M-R.L.
dc.contributor.authorBekki, K.
dc.contributor.authorClementini, G.
dc.contributor.authorde Blok, W.J.G.
dc.contributor.authorEmerson, J.P.
dc.contributor.authorEvans, Chris J.
dc.contributor.authorde Grijs, R.
dc.contributor.authorGibson, B. K.
dc.contributor.authorGirardi, L.
dc.contributor.authorGroenewegen, M.A.T.
dc.contributor.authorIvanov, V.D.
dc.contributor.authorLeisy, P.
dc.contributor.authorMarconi, M.
dc.contributor.authorMastropietro, C.
dc.contributor.authorMoore, B.
dc.contributor.authorNaylor, T.
dc.contributor.authorOliveira, J.M.
dc.contributor.authorRipepi, V.
dc.contributor.authorvan Loon, J. Th
dc.contributor.authorWilkinson, Mark
dc.contributor.authorWood, P.R.
dc.date.accessioned2013-12-16T15:00:14Z
dc.date.available2013-12-16T15:00:14Z
dc.date.issued2008-01
dc.identifier.citationCioni , M-RL , Bekki , K , Clementini , G , de Blok , W J G , Emerson , J P , Evans , C J , de Grijs , R , Gibson , B K , Girardi , L , Groenewegen , M A T , Ivanov , V D , Leisy , P , Marconi , M , Mastropietro , C , Moore , B , Naylor , T , Oliveira , J M , Ripepi , V , van Loon , J T , Wilkinson , M & Wood , P R 2008 , ' The Magellanic Clouds as a Template for the Study of Stellar Populations and Galaxy Interactions ' Publications of the Astronomical Society of Australia , vol. 25 , no. 03 , pp. 121-128 . https://doi.org/10.1071/AS07046
dc.identifier.issn1323-3580
dc.identifier.otherPURE: 2601323
dc.identifier.otherPURE UUID: f32375b0-5379-4804-949d-634fc2aab371
dc.identifier.otherScopus: 53849142586
dc.identifier.urihttp://hdl.handle.net/2299/12346
dc.description.abstractThe Magellanic System represents one of the best places to study the formation and evolution of galaxies. Photometric surveys of various depths, areas and wavelengths have had a significant impact on our understanding of the system; however, a complete picture is still lacking. VMC (the VISTA near-infrared YJKs survey of the Magellanic System) will provide new data to derive the spatially resolved star formation history and to construct a three-dimensional map of the system. These data combined with those from other ongoing and planned surveys will give us an absolutely unique view of the system opening up the doors to truly new science!en
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Australia
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.titleThe Magellanic Clouds as a Template for the Study of Stellar Populations and Galaxy Interactionsen
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.identifier.urlhttp://adsabs.harvard.edu/abs/2008PASA...25..121C
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeSubmitted Version
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1071/AS07046
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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