Coincidence between morphology and star formation activity through cosmic time: the impact of the bulge growth

The origin of the quenching in galaxies is still highly debated. Different scenarios and processes are proposed. We use multi-band (400-1600 nm) bulge-disc decompositions massive redshift range 00.2) equally distributed number star forming passive regions. vast majority bulges quiescent, while formation localized disc component. Our current findings underline strong correlation state galaxy. A bulge, if present, often independently morphology or activity host Additionally, large probability, hosting bulge. Conversely, has disky shape probable be forming.