State-of-the-art simulations of line-driven accretion disc winds: realistic radiation hydrodynamics leads to weaker outflows (2024)

First Author: Higginbottom N

Attributed to: Astrophysics at Southampton funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stad3830

Publication URI: http://dx.doi.org/10.1093/mnras/stad3830

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3