Abstract
The influence of the radiation flux from the accretion disk on obscuring tori in active galactic nuclei and the inverse effect of torus gravity on the disk and the position of the region of broad emission lines are considered. It is shown that the latter can affect the values of masses of supermassive black holes in the centers of galaxies determined by the reverberation method.
Conflict of Interest
The authors declare no conflict of interest.
Ethical Approval
Not applicable
Data Availability
The datasets used in this study are openly available at [repository link] and the source code is available on GitHub at [GitHub link].
Funding
This work did not receive any external funding.
Cite this article
Generating citation...
Related Research
