Line-driven disc wind in near-Eddington active galactic nuclei: decrease of mass accretion rate due to powerful outflow (2020)

First Author: Nomura M

Attributed to: Durham Astronomy Consolidated Grant 2017-2020 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa948

Publication URI: http://dx.doi.org/10.1093/mnras/staa948

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3