The Origin of Bulges and Discs. The Stellar Mass Growth Unveiled using CALIFA Spectro-Photometric Decompositions
Directly linked to the mass of the dark matter halo where baryons form, the galaxy stellar mass (M_star) is the most important observable parameter to understand galaxy evolution. Still, we have not completely figured out how the growth of the stellar mass in galaxies happen. A fundamental problem stands at the fact that galaxies are complex
Méndez-Abreu, J. et al.
Fecha de publicación:
7
2020