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- W1673877243 abstract "Color‐color distributions of extragalactic globular cluster systems are widely used to resolve stellar populations within their parent galaxies. However, the color predictions of the various SSP models differ significantly, resulting in model dependent age and metallicity estimates for the different stellar populations. Given that those constrain the formation and evolution of the host galaxy, this model dependency has to be removed from the analysis or quantified. Here we compare the cumulative age distributions as derived from Monte‐Carlo simulations and based on various SSP models with each other and use them to derive the age structure in globular cluster systems in early‐type galaxies." @default.
- W1673877243 created "2016-06-24" @default.
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- W1673877243 date "2009-01-01" @default.
- W1673877243 modified "2023-10-18" @default.
- W1673877243 title "Probing galaxy evolution using Globular Clusters and their integrated broad band colors" @default.
- W1673877243 cites W1515007647 @default.
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- W1673877243 doi "https://doi.org/10.1063/1.3141527" @default.
- W1673877243 hasPublicationYear "2009" @default.
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