Star Formation Rate in Active Galaxies

This study aims to investigate the relationship between the star formation rate (SFR) in active galaxies and the activity of their central supermassive black holes. Active galaxies, such as Seyfert galaxies and quasars, exhibit intense emissions across various wavelengths due to the presence of actively accreting black holes at their cores. Un- derstanding this connection is crucial for unraveling the complex processes that drive galaxy evolution. The study utilizes multi-wavelength observations and analyzes SFR indicators in active galaxies to shed light on the interplay between black hole activity and star formation. The findings contribute to our understanding of galaxy evolution and the role of black holes in shaping star formation processes.