The separated star formation main sequence of bulges and discs. New clues for the galaxy mass assembly
Disc galaxies are complex systems shaped by different stellar structures such as bulges, discs, and bars. Every galaxy structure keeps a unique memory of their past evolution, thus, understanding the mass assembly of disc galaxies can only be achieved by analysing separately all these independent footprints of past evolution. In this work, we have
Méndez-Abreu, J. et al.
Fecha de publicación:
5
2023