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The Base Models
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Population Synthesis in the
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Results
Model Predictions for Single Stellar Populations
Subsections
The Base Models
New vs. Old Fitting Functions
Abundance-Ratio Effects
Evolutionary Abundance-Ratio Effects
Spectroscopic Abundance-Ratio Effects
A Method for Determining Mean Ages and Metal Abundances of Stellar Populations
Caveats
Ricardo Piorno Schiavon 2006-11-15
