Predicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshifts

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dc.creatorAlvensleben, Uta Fritze-v.
dc.date2001-06-07
dc.date.accessioned2026-07-07T01:58:51Z
dc.date.available2026-07-07T01:58:51Z
dc.descriptionIn a 1$^{\rm st}$ step I present results from our new set of evolutionary synthesis models for Simple (= single burst) Stellar Populations ({\bf SSP}s) of various metallicities, and in a 2$^{\rm nd}$ 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.
dc.description6 pages, 1 Fig. To appear in IAU Symp. 207 {\sl Extragalactic Star Clusters}, eds. E. K. Grebel, D. Geisler, D. Minniti
dc.identifierhttps://arxiv.org/abs/astro-ph/0106129
dc.identifierhttp://arxiv.org/abs/astro-ph/0106129
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2879
dc.subjectAstrophysics
dc.titlePredicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshifts
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