On the driver of relativistic effect strength in Seyfert galaxies
On the driver of relativistic effect strength in Seyfert galaxies
Spectroscopy of X-ray emission lines emitted in accretion discs around supermassive black holes is one of the most powerful probes of the accretion flow physics and geometry, while also providing in principle observational constraints on the black hole spin.[...] We aim at determining the ultimate physical driver of the strength …