Virgo cluster and field dwarf ellipticals in 3D - III. Spatially and temporally resolved stellar populations
We present the stellar population analysis of a sample of 12 dwarf elliptical galaxies, observed with the SAURON integral field unit, using the full-spectrum fitting method. We show that star formation histories (SFHs) resolved into two populations can be recovered even within a limited wavelength range, provided that high signal-to-noise ratio (S
Ryś, A. et al.
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2015