to IAU
Symposium 241
Symposium 241
Abstract details
A new approach to derive [alpha/Fe] for integrated stellar populations
Abstract
Choosing either an empirical or a theoretical stellar library in stellar
population models is a subject of debate. Theoretical models do not perfectly
match high-resolution spectra of real stars, but we can use them to overcome
the natural limitations of empirical libraries on covering abundance patterns
that differ from solar neighbourhood stars. Here, we will mix stellar
population synthesis models based on both theoretical and empirical libraries,
in order to get the best of each of them and explore how to constrain the
enhanced alpha-elements pattern on galaxies.