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dc.contributor.authorKobayashi, C.
dc.date.accessioned2014-01-16T10:30:41Z
dc.date.available2014-01-16T10:30:41Z
dc.date.issued2002-07
dc.identifier.citationKobayashi , C 2002 , ' Chemodynamical evolution of galaxies ' , Astrophysics and Space Science , vol. 281 , no. 1-2 , pp. 301-304 . https://doi.org/10.1023/A:1019586315326
dc.identifier.issn0004-640X
dc.identifier.otherPURE: 811343
dc.identifier.otherPURE UUID: 2c7a3e95-bdd1-40c3-8608-0a2c6abe2fdd
dc.identifier.otherWOS: 000175921200061
dc.identifier.otherScopus: 0141570491
dc.identifier.otherORCID: /0000-0002-4343-0487/work/62750474
dc.identifier.urihttp://hdl.handle.net/2299/12559
dc.description.abstractI simulate the chemodynamical evolution of the Milky Way and elliptical galaxies using the GRAPE-SPH code. By reproducing the observations, I discuss the origin of elliptical galaxiesen
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.titleChemodynamical evolution of galaxiesen
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/10.1023/A:1019586315326
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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