High-redshift SMBHs can grow from stellar-mass seeds via chaotic accretion

Author(s):
Zubovas, K.; King, A.R.
Published
2021
Publication type
Article / Letter to editor
AccretionAccretion discsGalaxies: activeQuasars: generalAstrophysics - astrophysics of galaxies
Date issued
2021
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2021), Vol. 501, no. 3, p. 4289-4297
hdl
1887/3270769
doi
10.1093/mnras/stab004
URL
https://ui.adsabs.harvard.edu/abs/2021MNRAS.501.4289Z