Abstract:

Understanding the relationship between black hole mass and the size of the broad line region (BLR) is crucial for unraveling the intricate mechanisms governing active galactic nuclei (AGN) and quasars. This paper presents a comprehensive investigation into the quantitative aspects of the relationship between black hole mass and BLR size. Utilizing data from various observational campaigns, theoretical models, and advanced statistical methods, this research aims to provide insights into the underlying physical processes connecting these two fundamental AGN properties. The results contribute to the broader understanding of AGN physics and can have implications for cosmological studies and the evolution of galaxies

Description:

Active Galactic Nuclei, Energetic, Dynamic, Mass.