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dc.contributor.authorKobayashi, C.
dc.date.accessioned2013-08-21T14:45:01Z
dc.date.available2013-08-21T14:45:01Z
dc.date.issued2004-01
dc.identifier.citationKobayashi , C 2004 , ' Chemodynamical evolution of elliptical galaxies : Metallicity gradients and scaling relations ' , Publications of the Astronomical Society of Australia , vol. 21 , no. 2 , pp. 183-187 . https://doi.org/10.1071/AS04033
dc.identifier.issn1323-3580
dc.identifier.otherPURE: 811169
dc.identifier.otherPURE UUID: 6cf95427-9be1-4358-b94a-f374cbc36e69
dc.identifier.otherWOS: 000236550300017
dc.identifier.otherScopus: 32544437190
dc.identifier.otherORCID: /0000-0002-4343-0487/work/62750481
dc.identifier.urihttp://hdl.handle.net/2299/11438
dc.description.abstractWe simulate the chemodynamical evolution of a hundred elliptical galaxies using our GRAPE-SPH code, and succeed in reproducing the radial metallicity gradients and the global scaling relations such as the fundamental plane. These observations cannot be explained by either monolithic collapse or by major merger alone. Rather it requires a model in which both formation processes arise, such as the present CDM scheme.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Australia
dc.subjectmethods : N-body simulations
dc.subjectgalaxies : abundances
dc.subjectgalaxies : elliptical and lenticular, cD
dc.subjectgalaxies : evolution
dc.subjectgalaxies : formation
dc.titleChemodynamical evolution of elliptical galaxies : Metallicity gradients and scaling relationsen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1071/AS04033
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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