The Physical Mechanism of Radio-quiet Turn-on Changing-look Active Galactic Nuclei

It is suggested that the variation of the mass accretion rate in the accretion disk may be responsible for the occurrence of most changing-look active galactic nuclei (CL AGNs). However, the viscous timescale of a thin disk is far longer than the observed timescale of CL AGNs. Though this problem ca...

Full description

Saved in:

Bibliographic Details
Published in:	The Astrophysical journal Vol. 988; no. 2; pp. 207 - 213
Main Authors:	Li, Shuang-Liang, Cao, Xinwu
Format:	Journal Article
Language:	English
Published:	Philadelphia The American Astronomical Society 01.08.2025 IOP Publishing
Subjects:	Accretion Accretion disks Active galactic nuclei Advection Black hole physics Magnetic fields Time
ISSN:	0004-637X, 1538-4357
Online Access:	Get full text
Tags:	Add Tag No Tags, Be the first to tag this record!

Be the first to leave a comment!