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dc.contributor.authorKobayashi, C
dc.date.accessioned2014-01-15T15:30:32Z
dc.date.available2014-01-15T15:30:32Z
dc.date.issued2003-04
dc.identifier.citationKobayashi , C 2003 , ' The origin of elliptical galaxies inferred from their metallicity gradients ' , Astrophysics and Space Science , vol. 284 , no. 2 , pp. 853-856 . https://doi.org/10.1023/A:1024066522919
dc.identifier.issn0004-640X
dc.identifier.otherPURE: 811359
dc.identifier.otherPURE UUID: 40e63b45-2b99-4a4a-befb-0d41c3ef31a0
dc.identifier.otherWOS: 000183320500111
dc.identifier.otherScopus: 0346497597
dc.identifier.urihttp://hdl.handle.net/2299/12539
dc.description.abstractWe simulate the chemodynamical evolution of elliptical galaxies using our GRAPE-SPH code. We succeed in reproducing the observed variety of the radial metallicity gradients, from which we discuss the origin of elliptical galaxies.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.subjectEVOLUTION
dc.titleThe origin of elliptical galaxies inferred from their metallicity gradientsen
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
dcterms.dateAccepted2003-04
rioxxterms.versionofrecordhttps://doi.org/10.1023/A:1024066522919
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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