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dc.contributor.authorFritze, U.
dc.contributor.authorWeilbacher, P.
dc.contributor.authorBicker, J.
dc.date.accessioned2007-12-17T09:59:26Z
dc.date.available2007-12-17T09:59:26Z
dc.date.issued2003
dc.identifier.citationFritze , U , Weilbacher , P & Bicker , J 2003 , ' Chemically consistent evolutionary synthesis ' , Astrophysics and Space Science , vol. 284 , no. 2 , pp. 893-896 . https://doi.org/10.1023/A:1024014800146
dc.identifier.issn0004-640X
dc.identifier.otherPURE: 140132
dc.identifier.otherPURE UUID: 5310a76f-99e8-4f91-9ef6-fe075a1d1a3c
dc.identifier.otherdspace: 2299/1234
dc.identifier.otherScopus: 0347758319
dc.identifier.urihttp://hdl.handle.net/2299/1234
dc.descriptionThe original publication is available at www.springerlink.com . Copyright Springer DOI : 10.1023/A:1024014800146
dc.description.abstractTo account for the range of stellar metallicities in local galaxies and for the increasing importance of low metallicities at higher redshift we present chemically consistent models for the spectral and chemical evolution of galaxies over cosmological timescales. We discuss advantages, limitations and future prospects of our approach.en
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.rightsOpen
dc.titleChemically consistent evolutionary synthesisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2003
rioxxterms.versionofrecordhttps://doi.org/10.1023/A:1024014800146
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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