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...

Celý popis

Podrobná bibliografia

Vydané v:	The Astrophysical journal Ročník 988; číslo 2; s. 207 - 213
Hlavní autori:	Li, Shuang-Liang, Cao, Xinwu
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Philadelphia The American Astronomical Society 01.08.2025 IOP Publishing
Predmet:	Accretion Accretion disks Active galactic nuclei Advection Black hole physics Magnetic fields Time
ISSN:	0004-637X, 1538-4357
On-line prístup:	Získať plný text
Tagy:	Pridať tag Žiadne tagy, Buďte prvý, kto otaguje tento záznam!