Chemically consistent evolutionary synthesis

dc.contributor.author	Fritze, U.
dc.contributor.author	Weilbacher, P.
dc.contributor.author	Bicker, J.
dc.date.accessioned	2007-12-17T09:59:26Z
dc.date.available	2007-12-17T09:59:26Z
dc.date.issued	2003
dc.identifier.citation	Fritze , 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.issn	0004-640X
dc.identifier.other	dspace: 2299/1234
dc.identifier.uri	http://hdl.handle.net/2299/1234
dc.description	The original publication is available at www.springerlink.com . Copyright Springer DOI : 10.1023/A:1024014800146
dc.description.abstract	To 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.format.extent	165688
dc.language.iso	eng
dc.relation.ispartof	Astrophysics and Space Science
dc.title	Chemically consistent evolutionary synthesis	en
dc.contributor.institution	School of Physics, Astronomy and Mathematics
dc.description.status	Peer reviewed
rioxxterms.versionofrecord	10.1023/A:1024014800146
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true