DUSTY TORUS FORMATION BY ANISOTROPIC RADIATIVE PRESSURE FEEDBACK OF ACTIVE GALACTIC NUCLEI
DUSTY TORUS FORMATION BY ANISOTROPIC RADIATIVE PRESSURE FEEDBACK OF ACTIVE GALACTIC NUCLEI
The feedback by active galactic nuclei (AGNs) is significant for the formation and evolution of galaxies. It has been realized that the radiative pressure feedback could be an efficient mechanism due to the existence of dust. In this Letter, we discuss the effect of anisotropic radiative pressure, which is inevitable …