Abundance ratios and IMF slopes in the dwarf elliptical galaxy NGC 1396 with MUSE
Deep observations of the dwarf elliptical (dE) galaxy NGC 1396 (MV = -16.60, Mass ˜4 × 108 M⊙), located in the Fornax cluster, have been performed with the Very Large Telescope/Multi Unit Spectroscopic Explorer spectrograph in the wavelength region from 4750 to 9350 Å. In this paper, we present a stellar population analysis studying chemical
Puzia, T. et al.
Fecha de publicación:
12
2016