Prefer a chat interface with context about you and your work?
An Accretion Model for the Growth of the Central Black Hole Associated with Ionization Instability in Quasars
A possible accretion model associated with the ionization instability of quasar disks is proposed to address the growth of the central black hole (BH) harbored in the host galaxy. The evolution of quasars in cosmic time is assumed to change from a highly active state to a quiescent state triggered …