Tests of model predictions for the responses of stellar spectra and absorption-line indices to element abundance variations
A method that is widely used to analyse stellar populations in galaxies is to apply the theoretically derived responses of stellar spectra and line indices to element abundance variations, which are hereafter referred to as response functions. These are applied in a differential way, to base models, in order to generate spectra or indices with
Sánchez-Blázquez, P. et al.
Advertised on:
10
2013