Single stellar populations in the near-infrared. II. Synthesis models
We present unresolved single stellar population synthesis models in the near-infrared (NIR) range. The extension to the NIR is important for the study of early-type galaxies, since these galaxies are predominantly old and therefore emit most of their light in this wavelength range. The models are based on a library of empirical stellar spectra, the
Meneses-Goytia, S. et al.
Fecha de publicación:
10
2015