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Line-driven disc wind in near-Eddington active galactic nuclei: decrease of mass accretion rate due to powerful outflow (2018)

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/10.48550/arxiv.1811.01966

Publication URI: https://arxiv.org/abs/1811.01966

Type: Other