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dc.contributor.authorFritze, U.
dc.date.accessioned2008-02-21T10:52:43Z
dc.date.available2008-02-21T10:52:43Z
dc.date.issued2002
dc.identifier.citationFritze , U 2002 , Predicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshifts . in In: Procs of Extragalactic Star Clusters - IAU Symposium 207 . Astronomical Society of the Pacific , pp. 642-8 .
dc.identifier.otherPURE: 147288
dc.identifier.otherPURE UUID: 5efe2c8a-91f0-41f1-956d-7c8c325e7c3d
dc.identifier.otherdspace: 2299/1664
dc.identifier.urihttp://hdl.handle.net/2299/1664
dc.descriptionCopyright International Astronomical Union
dc.description.abstractIn a 1st step I present results from our new set of evolutionary synthesis models for Simple (= single burst) Stellar Populations (SSPs) of various metallicities, and in a 2nd step I combine these results with the information we have about the redshift evolution of spiral galaxies’ ISM abundances. The aim is to provide a grid of color and luminosity distibutions of any secondary GC population formed at some time in the past in those mergers for comparison with observations.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Extragalactic Star Clusters - IAU Symposium 207
dc.titlePredicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshiftsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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