An empirical spectral library of chemically well characterized stars for stellar population modelling
With the goal of assembling a new generation of more realistic single stellar population (SSP) models, we have obtained magnesium abundances for nearly 80% of the stars of the widely employed MILES empirical spectral library. Additional spectroscopic observations of carefully selected stars have recently been obtained to improve the parametric
de Castro Milone, André et al.
Fecha de publicación:
8
2012