Surface brightness fluctuations to constrain secondary stellar populations: revealing very low-metallicity stars in massive galaxies
The aim of this work is to explore the potential of surface brightness fluctuations (SBF) for studying composite stellar populations (CSP). To do so, we have computed the standard (mean) and SBF spectra with E-MILES stellar population synthesis code. We have created a set of models composed by different mass fractions of two single stellar
Rodríguez-Beltrán, P. et al.
Advertised on:
10
2021