The kinematics of young and old stellar populations in nuclear rings of MUSE TIMER galaxies
Context. Studying the stellar kinematics of galaxies is a key tool in the reconstruction of their evolution. However, the current measurements of the stellar kinematics are complicated by several factors, including dust extinction and the presence of multiple stellar populations. Aims: We use integral field spectroscopic data of four galaxies from
Rosado-Belza, D. et al.
Fecha de publicación:
12
2020