The Chemical Properties of Milky Way and M31 Globular Clusters. II. Stellar Population Model Predictions
We derive ages, metallicities, and abundance ratios ([α/Fe]) from the integrated spectra of 23 globular clusters in M31 by employing multivariate fits to two different stellar population models. We also perform a parallel analysis on 21 Galactic globular clusters as a consistency check and in order to facilitate a differential analysis. Our
Beasley, Michael A. et al.
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