Abstract
To determine metallicity and age distributions of globular clusters (GCs) in distant galaxies-now accessible, e.g. to Keck spectroscopy-it is important to have reliable calibrations of the color-metallicity, color-age, and index-metallicity relations.
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© 1999 Springer Science+Business Media Dordrecht
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Kurth, O.M., Fritze, U., Alvensleben, U., Fricke, K.J. (1999). Single Stellar Populations. In: Barnes, J.E., Sanders, D.B. (eds) Galaxy Interactions at Low and High Redshift. International Astronomical Union, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4665-4_69
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DOI: https://doi.org/10.1007/978-94-011-4665-4_69
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